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Harry Cliff: Particle Physics and the Large Hadron Collider | Lex Fridman Podcast #92


small model | large model

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The following is a conversation with Harry Cliff,
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a particle physicist at the University of Cambridge,
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working on the Large Hadron Collider beauty experiment
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that specializes in investigating the slight differences
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between matter and antimatter
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by studying a type of particle called the beauty quark
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or b quark.
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In this way, he's part of the group of physicists
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who are searching for the evidence of new particles
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that can answer some of the biggest questions
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in modern physics.
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He's also an exceptional communicator of science
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with some of the clearest and most captivating explanations
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of basic concepts in particle physicists
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that I've ever heard.
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So when I visited London, I knew I had to talk to him.
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And we did this conversation
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at the Royal Institute Lecture Theatre,
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which has hosted lectures for over two centuries
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from some of the greatest scientists
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and science communicators in history,
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from Michael Faraday to Carl Sagan.
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This conversation was recorded
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before the outbreak of the pandemic.
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And now, here's my conversation with Harry Kliff.
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Let's start with probably one of the coolest things
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that human beings have ever created,
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the Large Hadron Collider, OHC.
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What is it?
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How does it work?
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Okay, so it's essentially this gigantic
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27 kilometer circumference particle accelerator.
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It's this big ring.
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It's buried about 100 meters underneath the surface
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in the countryside just outside Geneva in Switzerland.
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And really what it's for, ultimately,
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is to try to understand what are the basic building blocks
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of the universe.
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So you can think of it in a way
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as like a gigantic microscope,
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and the analogy is actually fairly precise, so.
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Gigantic microscope.
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Effectively, except it's a microscope
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that looks at the structure of the vacuum.
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In order for this kind of thing to study particles,
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which are the microscopic entities, it has to be huge.
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It's a gigantic microscope.
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So what do you mean by studying vacuum?
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Okay, so I mean, so particle physics as a field
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is kind of badly named in a way,
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because particles are not the fundamental ingredients
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of the universe.
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They're not fundamental at all.
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So the things that we believe
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are the real building blocks of the universe
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are objects, invisible fluid like objects
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called quantum fields.
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So these are fields like the magnetic field
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around a magnet that exists everywhere in space.
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They're always there.
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In fact, actually, it's funny that we're
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in the Royal Institution,
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because this is where the idea of the field
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was effectively invented by Michael Faraday
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doing experiments with magnets and coils of wire.
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So he noticed that, you know,
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it was a very famous experiment that he did
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where he got a magnet and put on top of it a piece of paper
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and then sprinkled iron filings.
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And he found the iron filings arranged themselves
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into these kind of loops,
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which was actually mapping out the invisible influence
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of this magnetic field, which is a thing, you know,
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we've all experienced, we've all felt, held a magnet
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or two poles of magnet and pushed them together
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and felt this thing, this force pushing back.
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So these are real physical objects.
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And the way we think of particles in modern physics
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is that they are essentially little vibrations,
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little ripples in these otherwise invisible fields
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that are everywhere.
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They fill the whole universe.
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You know, I don't, I apologize perhaps
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for the ridiculous question.
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Are you comfortable with the idea
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of the fundamental nature of our reality being fields?
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Because to me, particles, you know,
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a bunch of different building blocks makes more sense
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sort of intellectually, sort of visually,
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like it seems to, I seem to be able to visualize
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that kind of idea easier.
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Are you comfortable psychologically with the idea
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that the basic building block is not a block, but a field?
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I think it's, I think it's quite a magical idea.
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I find it quite appealing.
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And it's, well, it comes from a misunderstanding
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of what particles are.
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So like when you, when we do science at school
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and we draw a picture of an atom,
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you draw like, you know, a nucleus with some protons
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and neutrons, these little spheres in the middle,
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and then you have some electrons that are like little flies
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flying around the atom.
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And that is a completely misleading picture
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of what an atom is like.
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It's nothing like that.
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The electron is not like a little planet orbiting the atom.
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It's this spread out, wibbly wobbly wave like thing.
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And we know we've known that since, you know,
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the early 20th century, thanks to quantum mechanics.
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So when we, we, we carry on using this word particle
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because sometimes when we do experiments,
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particles do behave like they're little marbles
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or little bullets, you know.
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So in the LHC, when we collide particles together,
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you'll get, you know, you'll get like hundreds of particles
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all flying out through the detector
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and they all take a trajectory and you can see
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from the detector where they've gone
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and they look like they're little bullets.
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So they behave that way, you know, a lot of the time.
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When you really study them carefully,
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you'll see that they are not little spheres.
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They are these ethereal disturbances
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in these underlying fields.
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So this is really how we think nature is,
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which is surprising, but also I think kind of magic.
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So, you know, we are, our bodies are basically made up
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of like little knots of energy
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in these invisible objects that are all around us.
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And what is the story of the vacuum when it comes to LHC?
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So why did you mention the word vacuum?
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Okay, so if we just, if we go back to like the physics,
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we do know.
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So atoms are made of electrons,
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which were discovered a hundred or so years ago.
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And then in the nucleus of the atom,
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you have two other types of particles.
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There's an up, something called an up quark
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and a down quark.
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And those three particles make up every atom in the universe.
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So we think of these as ripples in fields.
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So there is something called the electron field
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and every electron in the universe is a ripple moving
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about in this electron field.
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So the electron field is all around us, we can't see it,
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but every electron in our body is a little ripple
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in this thing that's there all the time.
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And the quark fields are the same.
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So there's an up quark field and an up quark
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is a little ripple in the up quark field.
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And the down quark is a little ripple
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in something else called the down quark field.
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So these fields are always there.
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Now there are potentially, we know about a certain number
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of fields in what we call the standard model
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of particle physics.
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And the most recent one we discovered was the Higgs field.
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And the way we discovered the Higgs field
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was to make a little ripple in it.
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So what the LHC did, it fired two protons into each other,
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very, very hard with enough energy
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that you could create a disturbance in this Higgs field.
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And that's what shows up as what we call the Higgs boson.
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So this particle that everyone was going on about
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eight or so years ago is proof really,
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the particle in itself is, I mean, it's interesting,
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but the thing that's really interesting is the field.
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Because it's the Higgs field that we believe
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is the reason that electrons and quarks have mass.
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And it's that invisible field that's always there
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that gives mass to the particles.
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The Higgs boson is just our way
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of checking it's there basically.
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And so the Large Hadron Collider,
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in order to get that ripple in the Higgs field,
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it requires a huge amount of energy.
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Yeah, I suppose.
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And so that's why you need this huge,
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that's why size matters here.
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So maybe there's a million questions here,
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but let's backtrack.
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Why does size matter in the context of a particle collider?
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So why does bigger allow you for higher energy collisions?
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Right, so the reason, well, it's kind of simple really,
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which is that there are two types of particle accelerator
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that you can build.
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One is circular, which is like the LHC,
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the other is a great long line.
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So the advantage of a circular machine
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is that you can send particles around a ring
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and you can give them a kick every time they go around.
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So imagine you have a, there's actually a bit of the LHC,
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that's about only 30 meters long,
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where you have a bunch of metal boxes,
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which have oscillating 2 million volt electric fields
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inside them, which are timed so that when a proton
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goes through one of these boxes,
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the field it sees as it approaches is attractive.
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And then as it leaves the box,
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it flips and becomes repulsive
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and the proton gets attracted
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and kicked out the other side, so it gets a bit faster.
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So you send it, and then you send it back round again.
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And it's incredible, like the timing of that,
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the synchronization, wait, really?
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Yeah, yeah, yeah, yeah.
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I think there's going to be a multiplicative effect
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on the questions I have.
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Is, okay, let me just take that attention for a second.
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The orchestration of that, is that fundamentally
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a hardware problem or a software problem?
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Like what, how do you get that?
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I mean, I should first of all say, I'm not an engineer.
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So the guys, I did not build the LHC,
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so they're people much, much better at this stuff than I.
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For sure, but maybe.
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But from your sort of intuition,
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from the echoes of what you understand,
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what you heard of how it's designed, what's your sense?
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What's the engineering aspects of it?
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The acceleration bit is not challenging.
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Okay, I mean, okay, there's always challenges
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with everything, but basically you have these,
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the beams that go around the LHC, the beams of particles
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are divided into little bunches.
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So they're called, they're a bit like swarms of bees,
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if you like, and there are around,
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I think it's something of the order 2000 bunches
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spaced around the ring.
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And they, if you're at a given point on the ring,
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counting bunches, you get 40 million bunches
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passing you every second.
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So they come in like cars going past
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on a very fast motorway.
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So you need to have, if you're an electric field
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that you're using to accelerate the particles,
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that needs to be timed so that as a bunch of protons arrives,
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it's got the right sign to attract them
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and then flips at the right moment.
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But I think the voltage in those boxes
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oscillates at hundreds of megahertz.
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So the beams are like 40 megahertz,
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but it's oscillating much more quickly than the beam.
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So I think it's difficult engineering,
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but in principle, it's not a really serious challenge.
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The bigger problem.
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There's probably engineers like screaming at you right now.
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Probably, but I mean, okay.
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So in terms of coming back to this thing,
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why is it so big?
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Well, the reason is you wanna get the particles
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through that accelerating element over and over again.
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So you wanna bring them back round.
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So that's why it's round.
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The question is why couldn't you make it smaller?
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Well, the basic answer is that these particles
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are going unbelievably quickly.
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So they travel at 99.9999991% of the speed of light
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in the LHC.
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And if you think about, say,
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driving your car around a corner at high speed,
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if you go fast, you need a lot of friction in the tires
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to make sure you don't slide off the road.
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So the limiting factor is how powerful a magnet can you make
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because what we do is magnets are used
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to bend the particles around the ring.
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And essentially the LHC, when it was designed,
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was designed with the most powerful magnets
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that could conceivably be built at the time.
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And so that's your kind of limiting factor.
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So if you wanted to make the machine smaller,
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that means a tighter bend,
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you need to have a more powerful magnet.
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So it's this toss up between how strong are your magnets
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versus how big a tunnel can you afford.
link |
00:13:49.920
The bigger the tunnel, the weaker the magnets can be.
link |
00:13:51.560
The smaller the tunnel, the stronger they've gotta be.
link |
00:13:54.080
Okay, so maybe can we backtrack to the Standard Model
link |
00:13:57.680
and say what kind of particles there are, period,
link |
00:14:00.800
and maybe the history of kind of assembling
link |
00:14:04.560
that the Standard Model of physics
link |
00:14:06.880
and then how that leads up to the hopes and dreams
link |
00:14:10.400
and the accomplishments of the Large Hadron Collider.
link |
00:14:12.800
Yeah, sure, okay.
link |
00:14:14.000
So all of 20th century physics in like five minutes.
link |
00:14:16.720
Yeah, please.
link |
00:14:17.560
Okay, so, okay, the story really begins properly.
link |
00:14:21.280
End of the 19th century, the basic view of matter
link |
00:14:24.760
is that matter is made of atoms
link |
00:14:26.720
and the atoms are indestructible, immutable little spheres
link |
00:14:30.280
like the things we were talking about
link |
00:14:31.480
that don't really exist.
link |
00:14:32.600
And there's one atom for every chemical element.
link |
00:14:35.280
So there's an atom for hydrogen, for helium,
link |
00:14:36.880
for carbon, for iron, et cetera, and they're all different.
link |
00:14:39.800
Then in 1897, experiments done
link |
00:14:41.880
at the Cavendish Laboratory in Cambridge,
link |
00:14:43.280
which is where I'm still, where I'm based,
link |
00:14:45.840
showed that there are actually smaller particles
link |
00:14:48.720
inside the atom, which eventually became known as electrons.
link |
00:14:51.640
So these are these negatively charged things
link |
00:14:53.200
that go around the outside.
link |
00:14:54.840
A few years later, Ernest Rutherford,
link |
00:14:57.080
very famous nuclear physicist,
link |
00:14:58.680
one of the pioneers of nuclear physics
link |
00:15:00.000
shows that the atom has a tiny nugget in the center,
link |
00:15:03.480
which we call the nucleus,
link |
00:15:04.400
which is a positively charged object.
link |
00:15:05.840
So then by like 1910, 11, we have this model of the atom
link |
00:15:09.080
that we learn in school,
link |
00:15:09.960
which is you've got a nucleus, electrons go around it.
link |
00:15:13.240
Fast forward a few years, the nucleus,
link |
00:15:16.280
people start doing experiments with radioactivity
link |
00:15:18.480
where they use alpha particles
link |
00:15:20.840
that are spat out of radioactive elements as bullets,
link |
00:15:24.520
and they fire them at other atoms.
link |
00:15:26.800
And by banging things into each other,
link |
00:15:28.560
they see that they can knock bits out of the nucleus.
link |
00:15:31.200
So these things come out called protons, first of all,
link |
00:15:33.880
which are positively charged particles
link |
00:15:36.040
about 2000 times heavier than the electron.
link |
00:15:38.800
And then 10 years later, more or less,
link |
00:15:41.160
a neutral particle is discovered called the neutron.
link |
00:15:43.880
So those are the three basic building blocks of atoms.
link |
00:15:47.000
You have protons and neutrons in the nucleus
link |
00:15:49.400
that are stuck together by something called the strong force,
link |
00:15:51.800
the strong nuclear force,
link |
00:15:53.200
and you have electrons in orbit around that,
link |
00:15:55.800
held in by the electromagnetic force,
link |
00:15:57.920
which is one of the forces of nature.
link |
00:16:00.440
That's sort of where we get to by like 1932, more or less.
link |
00:16:04.840
Then what happens is physics is nice and neat.
link |
00:16:07.440
In 1932, everything looks great, got three particles
link |
00:16:09.520
and all the atoms are made of, that's fine.
link |
00:16:11.160
But then cloud chamber experiments.
link |
00:16:13.960
These are devices that can be used to,
link |
00:16:16.000
the first device is capable of imaging subatomic particles
link |
00:16:18.600
so you can see their tracks.
link |
00:16:19.600
And they're used to study cosmic rays,
link |
00:16:21.760
particles that come from outer space
link |
00:16:23.760
and bang into the atmosphere.
link |
00:16:25.640
And in these experiments,
link |
00:16:28.120
people start to see a whole load of new particles.
link |
00:16:29.840
So they discover for one thing antimatter,
link |
00:16:31.560
which is the sort of a mirror image of the particles.
link |
00:16:34.440
So we discovered that there's also,
link |
00:16:35.960
as well as a negatively charged electron,
link |
00:16:37.440
there's something called a positron,
link |
00:16:38.520
which is a positively charged version of the electron.
link |
00:16:40.480
And there's an antiproton, which is negatively charged.
link |
00:16:43.240
And then a whole load of other weird particles
link |
00:16:45.600
start to get discovered.
link |
00:16:46.480
And no one really knows what they are.
link |
00:16:48.800
This is known as the zoo of particles.
link |
00:16:50.960
Are these discoveries from the first theoretical discoveries
link |
00:16:55.160
or are they discoveries in an experiment?
link |
00:16:58.360
So like, yeah, what's the process of discovery
link |
00:17:01.120
for these early sets of particles?
link |
00:17:03.280
It's a mixture.
link |
00:17:04.120
The early stuff around the atom is really
link |
00:17:06.040
experimentally driven.
link |
00:17:07.200
It's not based on some theory.
link |
00:17:09.000
It's exploration in the lab using equipment.
link |
00:17:11.640
So it's really people just figuring out,
link |
00:17:12.920
getting hands on with the phenomena,
link |
00:17:14.400
figuring out what these things are.
link |
00:17:16.000
And the theory comes a bit later.
link |
00:17:17.600
That's not always the case.
link |
00:17:18.880
So in the discovery of the anti electron, the positron,
link |
00:17:22.480
that was predicted from quantum mechanics and relativity
link |
00:17:26.160
by a very clever theoretical physicist called Paul Dirac,
link |
00:17:30.320
who was probably the second brightest physicist
link |
00:17:33.240
of the 20th century, apart from Einstein,
link |
00:17:34.920
but isn't anywhere near as well known.
link |
00:17:36.720
So he predicted the existence of the anti electron
link |
00:17:39.240
from basically a combination of the theories
link |
00:17:41.880
of quantum mechanics and relativity.
link |
00:17:43.240
And it was discovered about a year after
link |
00:17:44.720
he made the prediction.
link |
00:17:46.000
What happens when an electron meets a positron?
link |
00:17:49.160
They annihilate each other.
link |
00:17:50.680
So when you bring a particle and its antiparticle together,
link |
00:17:54.400
they react, well, they don't react,
link |
00:17:56.440
they just wipe each other out and they turn,
link |
00:17:58.520
their mass is turned into energy,
link |
00:18:00.040
usually in the form of photons, so you get light produced.
link |
00:18:03.440
So when you have that kind of situation,
link |
00:18:06.920
why does the universe exist at all
link |
00:18:08.880
if there's matter in any matter?
link |
00:18:10.320
Oh God, now we're getting into the really big questions.
link |
00:18:12.080
So, do you wanna go there now?
link |
00:18:15.680
Let's, maybe let's go there later.
link |
00:18:19.000
Cause that, I mean, that is a very big question.
link |
00:18:20.600
Yeah, let's take it slow with the standard model.
link |
00:18:23.720
So, okay, so there's matter and antimatter in the 30s.
link |
00:18:28.240
So what else?
link |
00:18:29.520
So matter and antimatter,
link |
00:18:30.400
and then a load of new particles start turning up
link |
00:18:33.400
in these cosmic ray experiments, first of all.
link |
00:18:36.880
And they don't seem to be particles that make up atoms.
link |
00:18:40.120
They're something else.
link |
00:18:41.080
They all mostly interact with a strong nuclear force.
link |
00:18:44.120
So they're a bit like protons and neutrons.
link |
00:18:46.480
And by, in the 1960s in America, particularly,
link |
00:18:50.280
but also in Europe and Russia,
link |
00:18:52.320
scientists started to build particle accelerators.
link |
00:18:54.160
So these are the forerunners of the LHC.
link |
00:18:55.800
So big ring shaped machines that were, you know,
link |
00:18:58.280
hundreds of meters long, which in those days was enormous.
link |
00:19:00.720
You never, you know, most physics up until that point
link |
00:19:02.760
had been done in labs, in universities, you know,
link |
00:19:04.840
with small bits of kit.
link |
00:19:06.240
So this is a big change.
link |
00:19:07.160
And when these accelerators are built,
link |
00:19:08.920
they start to find they can produce
link |
00:19:10.680
even more of these particles.
link |
00:19:12.160
So I don't know the exact numbers, but by around 1960,
link |
00:19:16.440
there are of order a hundred of these things
link |
00:19:19.320
that have been discovered.
link |
00:19:20.160
And physicists are kind of tearing their hair out
link |
00:19:22.720
because physics is all about simplification.
link |
00:19:25.040
And suddenly what was simple has become messy
link |
00:19:28.080
and complicated and everyone sort of wants
link |
00:19:29.720
to understand what's going on.
link |
00:19:31.640
As a quick kind of aside and probably really dumb question,
link |
00:19:34.600
but how is it possible to take something like a,
link |
00:19:38.720
like a photon or electron and be able to control it enough,
link |
00:19:44.000
like to be able to do a controlled experiment
link |
00:19:49.000
where you collide it against something else?
link |
00:19:51.480
Yeah.
link |
00:19:52.320
Is that, is that, that seems like an exceptionally difficult
link |
00:19:55.920
engineering challenge because you mentioned vacuum too.
link |
00:19:59.520
So you basically want to remove every other distraction
link |
00:20:03.200
and really focus on this collision.
link |
00:20:04.760
How difficult of an engineering challenge is that?
link |
00:20:06.840
Just to get a sense.
link |
00:20:07.840
And it is very hard.
link |
00:20:09.680
I mean, in the early days,
link |
00:20:10.920
particularly when the first accelerators are being built
link |
00:20:12.960
in like 1932, Ernest Lawrence builds the first,
link |
00:20:17.880
what we call a cyclotron,
link |
00:20:18.880
which is like a little accelerator, this big or so.
link |
00:20:21.760
There's another one.
link |
00:20:22.600
Is it really that big?
link |
00:20:23.420
There's a tiny little thing.
link |
00:20:24.260
Yeah.
link |
00:20:25.100
So most of the first accelerators
link |
00:20:27.840
were what we call fixed target experiments.
link |
00:20:31.000
So you had a ring, you accelerate particles around the ring
link |
00:20:34.100
and then you fire them out the side into some target.
link |
00:20:37.480
So that makes the kind of,
link |
00:20:39.480
the colliding bit is relatively straightforward
link |
00:20:41.320
because you just fire it,
link |
00:20:42.360
whatever it is you want to fire it at.
link |
00:20:43.660
The hard bit is the steering the beams
link |
00:20:46.200
with the magnetic fields, getting, you know,
link |
00:20:47.760
strong enough electric fields to accelerate them,
link |
00:20:49.560
all that kind of stuff.
link |
00:20:50.400
The first colliders where you have two beams
link |
00:20:53.760
colliding head on, that comes later.
link |
00:20:56.680
And I don't think it's done until maybe the 1980s.
link |
00:21:01.920
I'm not entirely sure, but it's a much harder problem.
link |
00:21:05.360
That's crazy.
link |
00:21:06.200
Cause you have to like perfectly get them to hit each other.
link |
00:21:09.880
I mean, we're talking about, I mean, what scale it takes,
link |
00:21:13.120
what's the, I mean, the temporal thing is a giant mess,
link |
00:21:18.160
but the spatially, like the size is tiny.
link |
00:21:23.160
Well, to give you a sense of the LHC beams,
link |
00:21:26.060
the cross sectional diameter is I think around a dozen
link |
00:21:31.620
or so microns.
link |
00:21:32.820
So, you know, 10 millionths of a meter.
link |
00:21:37.060
And a beam, sorry, just to clarify,
link |
00:21:39.900
a beam contains how many,
link |
00:21:41.340
is it the bunches that you mentioned?
link |
00:21:43.060
Is it multiple particles or is it just one particle?
link |
00:21:45.060
Oh no, no.
link |
00:21:45.900
The bunches contains say a hundred billion protons each.
link |
00:21:48.920
So a bunch is, it's not really bunch shaped.
link |
00:21:51.020
They're actually quite long.
link |
00:21:51.900
They're like 30 centimeters long,
link |
00:21:53.660
but thinner than a human hair.
link |
00:21:54.860
So like very, very narrow, long sort of objects.
link |
00:21:58.420
Those are the things.
link |
00:21:59.260
So what happens in the LHC is you steer the beams
link |
00:22:02.260
so that they cross in the middle of the detector.
link |
00:22:06.080
So they basically have these swarms of protons
link |
00:22:08.540
that are flying through each other.
link |
00:22:10.160
And most of the, you have to have a hundred billion
link |
00:22:12.180
coming one way, a hundred billion another way,
link |
00:22:14.500
maybe 10 of them will hit each other.
link |
00:22:17.100
Oh, okay.
link |
00:22:17.940
So this, okay, that makes a lot more sense.
link |
00:22:19.400
So that's nice.
link |
00:22:20.240
But you're trying to use sort of,
link |
00:22:21.980
it's like probabilistically, you're not.
link |
00:22:24.560
You can't make a single particle collide
link |
00:22:26.100
with a single other particle.
link |
00:22:26.940
That's not an efficient way to do it.
link |
00:22:28.140
You'd be waiting a very long time to get anything.
link |
00:22:30.980
So you're basically, right.
link |
00:22:34.020
You're relying on probability to be that some fraction
link |
00:22:37.460
of them are gonna collide.
link |
00:22:38.780
And then you know which,
link |
00:22:40.820
because it's a swarm of the same kind of particle.
link |
00:22:44.340
So it doesn't matter which ones hit each other exactly.
link |
00:22:46.420
I mean, that's not to say it's not hard.
link |
00:22:48.240
You've got to, one of the challenges
link |
00:22:50.420
to make the collisions work is you have to squash
link |
00:22:52.880
these beams to very, very,
link |
00:22:54.580
basically the narrower they are the better
link |
00:22:56.020
cause the higher chances of them colliding.
link |
00:22:58.780
If you think about two flocks of birds
link |
00:23:00.380
flying through each other,
link |
00:23:01.580
the birds are all far apart in the flocks.
link |
00:23:03.660
There's not much chance that they'll collide.
link |
00:23:04.980
If they're all flying densely together,
link |
00:23:06.420
then they're much more likely to collide with each other.
link |
00:23:08.360
So that's the sort of problem.
link |
00:23:10.060
And it's tuning those magnetic fields,
link |
00:23:12.060
getting the magnetic fields powerful enough
link |
00:23:13.380
that you squash the beams and focus them
link |
00:23:15.220
so that you get enough collisions.
link |
00:23:16.900
That's super cool.
link |
00:23:17.900
Do you know how much software is involved here?
link |
00:23:20.360
I mean, it's sort of,
link |
00:23:21.200
I come from the software world and it's fascinating.
link |
00:23:24.780
This seems like software is buggy and messy.
link |
00:23:28.060
And so like, you almost don't want to rely
link |
00:23:30.980
on software too much.
link |
00:23:31.900
Like if you do, it has to be like low level,
link |
00:23:33.900
like Fortran style programming.
link |
00:23:36.340
Do you know how much software
link |
00:23:37.540
is in a large Hadron Collider?
link |
00:23:39.500
I mean, it depends at which level a lot.
link |
00:23:41.580
I mean, the whole thing is obviously computer controlled.
link |
00:23:43.640
So, I mean, I don't know a huge amount
link |
00:23:45.460
about how the software for the actual accelerator works,
link |
00:23:49.340
but I've been in the control center.
link |
00:23:51.340
So at CERN, there's this big control room,
link |
00:23:53.280
which is like a bit like a NASA mission control
link |
00:23:55.480
with big banks of desks where the engineers sit
link |
00:23:57.760
and they monitor the LHC.
link |
00:23:59.180
Cause you obviously can't be in the tunnel
link |
00:24:00.860
when it's running.
link |
00:24:01.680
So everything's remote.
link |
00:24:03.460
I mean, one sort of anecdote about the software side,
link |
00:24:07.460
in 2008, when the LHC first switched on,
link |
00:24:10.460
they had this big launch event
link |
00:24:11.620
and then big press conference party
link |
00:24:14.940
to inaugurate the machine.
link |
00:24:16.260
And about 10 days after that,
link |
00:24:18.300
they were doing some tests
link |
00:24:19.580
and this dramatic event happened
link |
00:24:22.100
where a huge explosion basically took place
link |
00:24:24.180
in the tunnel that destroyed or damaged, badly damaged
link |
00:24:26.880
about half a kilometer of the machine.
link |
00:24:29.880
But the stories, the engineers
link |
00:24:31.540
are in the control room that day.
link |
00:24:33.620
One guy told me this story about,
link |
00:24:35.300
basically all these screens they have in the control room
link |
00:24:37.700
started going red.
link |
00:24:38.540
So these alarms like kind of in software going off
link |
00:24:42.300
and then they assume that there's something wrong
link |
00:24:43.500
with the software, cause there's no way
link |
00:24:45.500
something this catastrophic could have happened.
link |
00:24:48.700
But I mean, when I worked on, when I was a PhD student,
link |
00:24:52.300
one of my jobs was to help to maintain the software
link |
00:24:56.060
that's used to control the detector that we work on.
link |
00:24:59.140
And that was, it's relatively robust,
link |
00:25:01.180
not such, you don't want it to be too fancy.
link |
00:25:02.940
You don't want it to sort of fall over too easily.
link |
00:25:04.620
The more clever stuff comes
link |
00:25:07.040
when you're talking about analyzing the data
link |
00:25:08.500
and that's where the sort of, you know.
link |
00:25:10.540
Are we jumping around too much?
link |
00:25:11.740
Do we finish with a standard model?
link |
00:25:13.160
We didn't, no.
link |
00:25:14.000
We didn't, so have we even started talking about quarks?
link |
00:25:17.020
We haven't talked to them yet.
link |
00:25:17.860
No, we got to the messy zoo of particles.
link |
00:25:20.360
Let me, let's go back there if it's okay.
link |
00:25:22.980
Okay, that's fine.
link |
00:25:23.820
Can you take us to the rest of the history of physics
link |
00:25:26.540
in the 20th century?
link |
00:25:27.700
Okay, sure.
link |
00:25:29.020
Okay, so circa 1960, you have this,
link |
00:25:32.000
you have these a hundred or so particles.
link |
00:25:33.680
It's a bit like the periodic table all over again.
link |
00:25:35.540
So you've got like having a hundred elements,
link |
00:25:37.860
it's sort of a bit like that.
link |
00:25:39.260
And people start to try to impose some order.
link |
00:25:41.500
So Murray Gellman, he's a theoretical physicist,
link |
00:25:46.140
American from New York.
link |
00:25:47.700
He realizes that there are these symmetries
link |
00:25:50.500
in these particles that if you arrange them in certain ways,
link |
00:25:53.340
they relate to each other.
link |
00:25:54.380
And he uses these symmetry principles
link |
00:25:56.060
to predict the existence of particles
link |
00:25:58.260
that haven't been discovered,
link |
00:25:59.220
which are then discovered in accelerators.
link |
00:26:01.060
So this starts to suggest
link |
00:26:02.480
there's not just random collections of crap.
link |
00:26:04.500
There's like, you know, actually some order
link |
00:26:06.460
to this underlying it.
link |
00:26:08.740
A little bit later in 1960, again, around the 1960s,
link |
00:26:14.260
he proposes along with another physicist called George Zweig
link |
00:26:17.860
that these symmetries arise because
link |
00:26:21.060
just like the patterns in the periodic table arise
link |
00:26:23.380
because atoms are made of electrons and protons,
link |
00:26:26.420
that these patterns are due to the fact
link |
00:26:28.100
that these particles are made of smaller things.
link |
00:26:30.260
And they are called quarks.
link |
00:26:31.900
So these are the particles they're predicted from theory.
link |
00:26:34.500
For a long time, no one really believes they're real.
link |
00:26:36.700
A lot of people think that they're a kind of theoretical
link |
00:26:39.180
convenience that happened to fit the data,
link |
00:26:41.480
but there's no evidence.
link |
00:26:42.580
No one's ever seen a quark in any experiment.
link |
00:26:45.460
And lots of experiments are done to try to find quarks,
link |
00:26:48.580
to try to knock a quark out of a...
link |
00:26:50.460
So the idea, if protons and neutrons are made of quarks,
link |
00:26:52.860
you should be able to knock a quark out and see the quark.
link |
00:26:55.140
That never happens.
link |
00:26:56.020
And we still have never actually managed to do that.
link |
00:26:58.140
Wait, really?
link |
00:26:59.260
No.
link |
00:27:00.100
So the way that it's done in the end
link |
00:27:02.260
is this machine that's built in California
link |
00:27:04.620
at the Stanford Lab, Stanford Linear Accelerator,
link |
00:27:08.860
which is essentially a gigantic,
link |
00:27:10.540
three kilometer long electron gun.
link |
00:27:12.460
It fires electrons, almost the speed of light, at protons.
link |
00:27:16.260
And when you do these experiments,
link |
00:27:17.860
what you find is at very high energy,
link |
00:27:20.100
the electrons bounce off small, hard objects
link |
00:27:24.000
inside the proton.
link |
00:27:25.420
So it's a bit like taking an X ray of the proton.
link |
00:27:28.100
You're firing these very light, high energy particles,
link |
00:27:31.580
and they're pinging off little things inside the proton
link |
00:27:34.260
that are like ball bearings, if you like.
link |
00:27:36.260
So you actually, that way,
link |
00:27:38.220
they resolve that there are three things
link |
00:27:41.020
inside the proton, which are quarks,
link |
00:27:42.820
the quarks that Gellman and Zweig had predicted.
link |
00:27:45.480
So that's really the evidence that convinces people
link |
00:27:47.900
that these things are real.
link |
00:27:49.400
The fact that we've never seen one
link |
00:27:50.820
in an experiment directly,
link |
00:27:51.980
they're always stuck inside other particles.
link |
00:27:56.260
And the reason for that is essentially
link |
00:27:58.180
to do with a strong force.
link |
00:27:59.100
The strong force is the force that holds quarks together.
link |
00:28:01.700
And it's so strong that it's impossible
link |
00:28:04.020
to actually liberate a quark.
link |
00:28:06.460
So if you try and pull a quark out of a proton,
link |
00:28:08.260
what actually ends up happening
link |
00:28:09.700
is that you kind of create this spring like bond
link |
00:28:14.260
in the strong force.
link |
00:28:15.100
You imagine two quarks that are held together
link |
00:28:16.780
by a very powerful spring.
link |
00:28:18.540
You pull and pull and pull,
link |
00:28:19.940
more and more energy gets stored in that bond,
link |
00:28:22.280
like stretching a spring,
link |
00:28:23.420
and eventually the tension gets so great,
link |
00:28:25.340
the spring snaps, and the energy in that bond
link |
00:28:28.700
gets turned into two new quarks
link |
00:28:30.660
that go on the broken ends.
link |
00:28:32.420
So you started with two quarks,
link |
00:28:33.260
you end up with four quarks.
link |
00:28:34.660
So you never actually get to take a quark out.
link |
00:28:37.180
You just end up making loads more quarks in the process.
link |
00:28:39.860
So how do we, again, forgive the dumb question,
link |
00:28:42.900
how do we know quarks are real then?
link |
00:28:44.880
Well, A, from these experiments where we can scatter,
link |
00:28:48.100
you fire electrons into the protons.
link |
00:28:49.700
They can burrow into the proton and knock off,
link |
00:28:52.620
and they can bounce off these quarks.
link |
00:28:55.140
So you can see from the angles,
link |
00:28:56.460
the electrons come out.
link |
00:28:58.100
I see, you can infer.
link |
00:28:59.120
You can infer that these things are there.
link |
00:29:02.060
The quark model can also be used.
link |
00:29:03.620
It has a lot of successes that you can use it
link |
00:29:05.340
to predict the existence of new particles
link |
00:29:07.500
that hadn't been seen.
link |
00:29:08.700
So, and it basically, there's lots of data
link |
00:29:10.780
basically showing from, you know,
link |
00:29:12.340
when we fire protons at each other at the LHC,
link |
00:29:16.420
a lot of quarks get knocked all over the place.
link |
00:29:18.820
And every time they try and escape from,
link |
00:29:20.540
say, one of their protons,
link |
00:29:21.580
they make a whole jet of quarks that go flying off,
link |
00:29:25.580
bound up in other sorts of particles made of quarks.
link |
00:29:28.560
So all the sort of the theoretical predictions
link |
00:29:30.740
from the basic theory of the strong force and the quarks
link |
00:29:33.740
all agrees with what we are seeing in experiments.
link |
00:29:35.380
We've just never seen an actual quark on its own
link |
00:29:38.020
because unfortunately it's impossible
link |
00:29:39.280
to get them out on their own.
link |
00:29:41.140
So quarks, these crazy smaller things
link |
00:29:45.120
that are hard to imagine are real.
link |
00:29:47.160
So what else?
link |
00:29:48.140
What else is part of the story here?
link |
00:29:49.780
So the other thing that's going on at the time,
link |
00:29:52.100
around the 60s, is an attempt to understand the forces
link |
00:29:57.380
that make these particles interact with each other.
link |
00:30:00.220
So you have the electromagnetic force,
link |
00:30:01.780
which is the force that was sort of discovered
link |
00:30:03.900
to some extent in this room, or at least in this building.
link |
00:30:07.140
So the first, what we call quantum field theory
link |
00:30:10.020
of the electromagnetic force is developed
link |
00:30:13.380
in the 1940s and 50s by Feynman,
link |
00:30:17.660
Richard Feynman amongst other people,
link |
00:30:19.740
Julian Schrodinger, Tom Onaga,
link |
00:30:22.020
who come up with the first,
link |
00:30:23.060
what we call a quantum field theory
link |
00:30:24.420
of the electromagnetic force.
link |
00:30:25.740
And this is where this description of,
link |
00:30:27.340
which I gave you at the beginning,
link |
00:30:28.360
that particles are ripples in fields.
link |
00:30:30.820
Well, in this theory, the photon, the particle of light
link |
00:30:33.900
is described as a ripple in this quantum field
link |
00:30:36.340
called the electromagnetic field.
link |
00:30:38.720
And the attempt then is made to try,
link |
00:30:40.240
well, can we come up with a quantum field theory
link |
00:30:42.260
of the other forces, of the strong force and the weak,
link |
00:30:45.140
the third force, which we haven't discussed,
link |
00:30:47.140
which is the weak force, which is a nuclear force.
link |
00:30:50.740
We don't really experience it in our everyday lives,
link |
00:30:52.640
but it's responsible for radioactive decay.
link |
00:30:54.960
It's the force that allows, you know,
link |
00:30:56.980
on a radioactive atom to turn
link |
00:30:59.140
into a different element, for example.
link |
00:31:01.060
And I don't know if you've explicitly mentioned,
link |
00:31:03.420
but so there's technically four forces.
link |
00:31:06.100
Yes.
link |
00:31:06.980
I guess three of them would be in the standard model,
link |
00:31:09.900
like the weak, the strong, and the electromagnetic,
link |
00:31:13.460
and then there's gravity.
link |
00:31:14.540
And there's gravity, which we don't worry about that,
link |
00:31:16.220
because it's too hard.
link |
00:31:17.040
It's too hard.
link |
00:31:17.880
Well, no, maybe we bring that up at the end, but yeah.
link |
00:31:19.940
Gravity, so far, we don't have a quantum theory of,
link |
00:31:22.340
and if you can solve that problem,
link |
00:31:23.580
you'll win a Nobel Prize.
link |
00:31:25.140
Well, we're gonna have to bring up
link |
00:31:26.340
the graviton at some point, I'm gonna ask you,
link |
00:31:28.140
but let's leave that to the side for now.
link |
00:31:31.160
So those three, okay, Feynman, electromagnetic force,
link |
00:31:36.500
the quantum field, and where does the weak force come in?
link |
00:31:41.920
So yeah, well, first of all,
link |
00:31:43.580
I mean, the strong force is the easiest.
link |
00:31:44.780
The strong force is a little bit
link |
00:31:46.460
like the electromagnetic force.
link |
00:31:47.600
It's a force that binds things together.
link |
00:31:49.140
So that's the force that holds quarks together
link |
00:31:51.060
inside the proton, for example.
link |
00:31:52.860
So a quantum field theory of that force
link |
00:31:55.960
is discovered in the, I think it's in the 60s,
link |
00:31:59.820
and it predicts the existence
link |
00:32:01.460
of new force particles called gluons.
link |
00:32:04.500
So gluons are a bit like the photon.
link |
00:32:06.940
The photon is the particle of electromagnetism.
link |
00:32:09.500
Gluons are the particles of the strong force.
link |
00:32:13.540
So just like there's an electromagnetic field,
link |
00:32:15.860
there's something called a gluon field,
link |
00:32:17.540
which is also all around us.
link |
00:32:19.500
So some of these particles, I guess,
link |
00:32:21.780
are the force carriers or whatever.
link |
00:32:23.660
They carry the force.
link |
00:32:24.500
It depends how you want to think about it.
link |
00:32:25.980
I mean, really the field, the strong force field,
link |
00:32:28.460
the gluon field is the thing that binds the quarks together.
link |
00:32:32.880
The gluons are the little ripples in that field.
link |
00:32:35.460
So that like, in the same way that the photon is a ripple
link |
00:32:37.740
in the electromagnetic field.
link |
00:32:39.900
But the thing that really does the binding is the field.
link |
00:32:43.620
I mean, you may have heard people talk about things
link |
00:32:45.680
like you've heard the phrase virtual particle.
link |
00:32:49.860
So sometimes in some, if you hear people describing
link |
00:32:52.460
how forces are exchanged between particles,
link |
00:32:54.900
they quite often talk about the idea
link |
00:32:56.220
that if you have an electron and another electron, say,
link |
00:32:59.180
and they're repelling each other
link |
00:33:00.640
through the electromagnetic force,
link |
00:33:03.060
you can think of that as if they're exchanging photons.
link |
00:33:05.820
So they're kind of firing photons
link |
00:33:07.060
backwards and forwards between each other.
link |
00:33:08.660
And that causes them to repel.
link |
00:33:11.060
That photon is then a virtual particle.
link |
00:33:13.060
Yes, that's what we call a virtual particle.
link |
00:33:14.460
In other words, it's not a real thing,
link |
00:33:15.580
it doesn't actually exist.
link |
00:33:16.820
So it's an artifact of the way theorists do calculations.
link |
00:33:19.900
So when they do calculations in quantum field theory,
link |
00:33:22.140
rather than, no one's discovered a way
link |
00:33:24.460
of just treating the whole field.
link |
00:33:25.780
You have to break the field down into simpler things.
link |
00:33:28.200
So you can basically treat the field
link |
00:33:30.200
as if it's made up of lots of these virtual photons,
link |
00:33:33.540
but there's no experiment that you can do
link |
00:33:35.660
that can detect these particles being exchanged.
link |
00:33:38.420
What's really happening in reality
link |
00:33:40.460
is that the electromagnetic field is warped
link |
00:33:43.280
by the charge of the electron and that causes the force.
link |
00:33:46.240
But the way we do calculations involves particles.
link |
00:33:49.300
So it's a bit confusing,
link |
00:33:50.840
but it's really a mathematical technique.
link |
00:33:53.300
It's not something that corresponds to reality.
link |
00:33:55.740
I mean, that's part, I guess, of the Feynman diagrams.
link |
00:33:58.260
Yes.
link |
00:33:59.100
Is this these virtual particles, okay.
link |
00:34:00.100
That's right, yeah.
link |
00:34:01.500
Some of these have mass, some of them don't.
link |
00:34:06.380
What does that even mean, not to have mass?
link |
00:34:09.060
And maybe you can say which one of them have mass
link |
00:34:11.900
and which don't.
link |
00:34:12.860
Okay, so.
link |
00:34:14.140
And why is mass important or relevant
link |
00:34:17.020
in this field view of the universe?
link |
00:34:22.020
Well, there are actually only two particles
link |
00:34:23.700
in the standard model that don't have mass,
link |
00:34:25.500
which are the photon and the gluons.
link |
00:34:28.480
So they are massless particles,
link |
00:34:30.300
but the electron, the quarks,
link |
00:34:32.960
and there are a bunch of other particles
link |
00:34:34.140
I haven't discussed.
link |
00:34:34.960
There's something called a muon and a tau,
link |
00:34:36.380
which are basically heavy versions of the electron
link |
00:34:39.280
that are unstable.
link |
00:34:40.120
You can make them in accelerators,
link |
00:34:41.380
but they don't form atoms or anything.
link |
00:34:44.200
They don't exist for long enough.
link |
00:34:45.600
But all the matter particles, there are 12 of them,
link |
00:34:48.700
six quarks and six, what we call leptons,
link |
00:34:51.940
which includes the electron and its two heavy versions
link |
00:34:54.460
and three neutrinos, all of them have mass.
link |
00:34:57.380
And so do, this is the critical bit.
link |
00:34:59.500
So the weak force, which is the third of these
link |
00:35:02.860
quantum forces, which is one of the hardest to understand,
link |
00:35:07.540
the force particles of that force have very large masses.
link |
00:35:13.860
And there are three of them.
link |
00:35:14.900
They're called the W plus, the W minus, and the Z boson.
link |
00:35:19.540
And they have masses of between 80 and 90 times
link |
00:35:23.000
that of the protons.
link |
00:35:24.580
They're very heavy.
link |
00:35:25.660
Wow.
link |
00:35:26.500
They're very heavy things.
link |
00:35:27.320
So they're what, the heaviest, I guess?
link |
00:35:29.440
They're not the heaviest.
link |
00:35:30.280
The heaviest particle is the top quark,
link |
00:35:32.920
which has a mass of about 175 ish protons.
link |
00:35:38.460
So that's really massive.
link |
00:35:39.700
And we don't know why it's so massive,
link |
00:35:41.680
but coming back to the weak force,
link |
00:35:43.160
so the problem in the 60s and 70s was that
link |
00:35:47.380
the reason that the electromagnetic force
link |
00:35:50.100
is a force that we can experience in our everyday lives.
link |
00:35:51.900
So if we have a magnet and a piece of metal,
link |
00:35:53.260
you can hold it, you know, a meter apart
link |
00:35:55.420
if it's powerful enough and you'll feel a force.
link |
00:35:57.040
Whereas the weak force only becomes apparent
link |
00:36:00.380
when you basically have two particles touching
link |
00:36:03.180
at the scale of a nucleus.
link |
00:36:05.340
So we just get to very short distances
link |
00:36:06.980
before this force becomes manifest.
link |
00:36:09.620
It's not, we don't get weak forces going on in this room.
link |
00:36:12.260
We don't notice them.
link |
00:36:14.060
And the reason for that is that the particle,
link |
00:36:15.860
well, the field that transmits the weak force,
link |
00:36:20.140
the particle that's associated with that field
link |
00:36:22.300
has a very large mass,
link |
00:36:23.380
which means that the field dies off very quickly.
link |
00:36:26.240
So as you, whereas an electric charge,
link |
00:36:28.360
if you were to look at the shape of the electromagnetic field,
link |
00:36:30.640
it would fall off with this,
link |
00:36:32.140
you have this thing called the inverse square law,
link |
00:36:33.780
which is the idea that the force halves
link |
00:36:36.220
every time you double the distance.
link |
00:36:38.740
No, sorry, it doesn't half.
link |
00:36:39.700
It quarters every time you double the distance
link |
00:36:42.580
between say the two particles.
link |
00:36:44.220
Whereas the weak force kind of,
link |
00:36:45.780
you move a little bit away from the nucleus
link |
00:36:47.300
and just disappears.
link |
00:36:49.400
The reason for that is because these fields,
link |
00:36:51.980
the particles that go with them have a very large mass.
link |
00:36:55.420
But the problem that theorists faced in the 60s
link |
00:36:59.860
was that if you tried to introduce massive force fields,
link |
00:37:04.300
the theory gave you nonsensical answers.
link |
00:37:06.540
So you'd end up with infinite results
link |
00:37:08.700
for a lot of the calculations you tried to do.
link |
00:37:11.140
So the basically, it seemed that quantum field theory
link |
00:37:13.660
was incompatible with having massive particles,
link |
00:37:17.320
not just the force particles actually,
link |
00:37:18.700
but even the electron was a problem.
link |
00:37:21.900
So this is where the Higgs
link |
00:37:23.740
that we sort of alluded to comes in.
link |
00:37:25.640
And the solution was to say, okay, well,
link |
00:37:28.400
actually all the particles in the Standard Model are mass.
link |
00:37:30.460
They have no mass.
link |
00:37:31.540
So the quarks, the electron, they don't have a mass.
link |
00:37:33.340
Neither do these weak particles.
link |
00:37:34.820
They don't have mass either.
link |
00:37:36.740
What happens is they actually acquire mass
link |
00:37:38.500
through another process.
link |
00:37:40.420
They get it from somewhere else.
link |
00:37:41.660
They don't actually have it intrinsically.
link |
00:37:43.780
So this idea that was introduced by,
link |
00:37:46.500
well, Peter Higgs is the most famous,
link |
00:37:47.740
but actually there are about six people
link |
00:37:49.380
that came up with the idea more or less at the same time,
link |
00:37:52.080
is that you introduce a new quantum field,
link |
00:37:55.180
which is another one of these invisible things
link |
00:37:56.880
that's everywhere.
link |
00:37:58.100
And it's through the interaction with this field
link |
00:38:01.500
that particles get mass.
link |
00:38:02.660
So you can think of say an electron in the Higgs field,
link |
00:38:07.380
the Higgs field kind of bunches around the electron.
link |
00:38:10.900
It's sort of drawn towards the electron.
link |
00:38:12.900
And that energy that's stored in that field
link |
00:38:15.580
around the electron is what we see
link |
00:38:17.720
as the mass of the electron.
link |
00:38:19.320
But if you could somehow turn off the Higgs field,
link |
00:38:21.740
then all the particles in nature would become massless
link |
00:38:23.880
and fly around at the speed of light.
link |
00:38:26.540
So this idea of the Higgs field allowed other people,
link |
00:38:32.540
other theorists to come up with a, well,
link |
00:38:36.160
it was another, basically a unified theory
link |
00:38:39.500
of the electromagnetic force and the weak force.
link |
00:38:41.580
So once you bring in the Higgs field,
link |
00:38:43.060
you can combine two of the forces into one.
link |
00:38:45.620
So it turns out the electromagnetic force
link |
00:38:47.900
and the weak force are just two aspects
link |
00:38:49.660
of the same fundamental force.
link |
00:38:52.420
And at the LHC, we go to high enough energies
link |
00:38:54.760
that you see these two forces unifying effectively.
link |
00:38:59.460
So first of all, it started as a theoretical notion,
link |
00:39:04.260
like this is some, and then, I mean,
link |
00:39:07.540
wasn't the Higgs called the God particle at some point?
link |
00:39:10.660
It was by a guy trying to sell popular science books, yeah.
link |
00:39:13.660
Yeah, but I mean, I remember because when I was hearing it,
link |
00:39:17.880
I thought it would, I mean, that would solve a lot of,
link |
00:39:22.060
that unify a lot of our ideas of physics was my notion.
link |
00:39:26.340
But maybe you can speak to that.
link |
00:39:29.020
Is it as big of a leap as a God particle
link |
00:39:32.540
or is it a Jesus particle, which, you know,
link |
00:39:37.340
what's the big contribution of Higgs
link |
00:39:39.020
in terms of this unification power?
link |
00:39:40.780
Yeah, I mean, to understand that,
link |
00:39:42.940
it maybe helps know the history a little bit.
link |
00:39:45.060
So when the, what we call electroweak theory
link |
00:39:47.740
was put together, which is where you unify electromagnetism
link |
00:39:50.580
with the weak force and Higgs is involved in all of that.
link |
00:39:53.280
So that theory, which was written in the mid 70s,
link |
00:39:55.420
predicted the existence of four new particles,
link |
00:39:59.380
the W plus boson, the W minus boson,
link |
00:40:01.780
the Z boson and the Higgs boson.
link |
00:40:03.500
So there were these four particles
link |
00:40:04.780
that came with the theory,
link |
00:40:06.020
that were predicted by the theory.
link |
00:40:07.500
In 1983, 84, the W's and the Z particles
link |
00:40:11.620
were discovered at an accelerator at CERN
link |
00:40:14.320
called the super proton synchrotron,
link |
00:40:15.980
which was a seven kilometer particle collider.
link |
00:40:19.240
So three of the bits of this theory had already been found.
link |
00:40:22.820
So people were pretty confident from the 80s
link |
00:40:25.560
that the Higgs must exist
link |
00:40:27.060
because it was a part of this family of particles
link |
00:40:30.800
that this theoretical structure only works
link |
00:40:33.020
if the Higgs is there.
link |
00:40:34.460
So what then happens,
link |
00:40:36.540
and so you've got this question about
link |
00:40:37.380
why is the LHC the size it is?
link |
00:40:39.420
Well, actually the tunnel that the LHC is in
link |
00:40:41.500
was not built for the LHC.
link |
00:40:42.780
It was built for a previous accelerator
link |
00:40:45.140
called the large electron positron collider.
link |
00:40:48.740
So that began operation in the late 80s, early 90s.
link |
00:40:53.800
They basically, that's when they dug
link |
00:40:55.220
the 27 kilometer tunnel.
link |
00:40:56.420
They put this accelerator into it,
link |
00:40:58.020
the collider that fires electrons
link |
00:40:59.860
and anti electrons at each other, electrons and positrons.
link |
00:41:02.660
So the purpose of that machine was,
link |
00:41:05.180
well, it was actually to look for the Higgs.
link |
00:41:06.700
That was one of the things it was trying to do.
link |
00:41:08.700
It didn't have enough energy to do it in the end.
link |
00:41:11.380
But the main thing it achieved was it studied
link |
00:41:13.820
the W and the Z particles at very high precision.
link |
00:41:17.540
So it made loads of these things.
link |
00:41:19.300
Previously, you can only make a few of them
link |
00:41:20.540
at the previous accelerator.
link |
00:41:21.460
So you could study these really, really precisely.
link |
00:41:24.500
And by studying their properties,
link |
00:41:25.680
you could really test this electroweak theory
link |
00:41:28.220
that had been invented in the 70s
link |
00:41:29.820
and really make sure that it worked.
link |
00:41:31.260
So actually by 1999, when this machine turned off,
link |
00:41:36.380
people knew, well, okay, you never know
link |
00:41:39.500
until you find the thing.
link |
00:41:41.420
But people were really confident
link |
00:41:43.000
this electroweak theory was right.
link |
00:41:44.800
And that the Higgs almost,
link |
00:41:46.820
the Higgs or something very like the Higgs had to exist
link |
00:41:49.860
because otherwise the whole thing doesn't work.
link |
00:41:52.220
It'd be really weird if you could discover
link |
00:41:54.000
and these particles, they all behave exactly
link |
00:41:55.900
as your theory tells you they should.
link |
00:41:57.320
But somehow this key piece of the picture is not there.
link |
00:42:00.900
So in a way, it depends how you look at it.
link |
00:42:03.920
The discovery of the Higgs on its own
link |
00:42:07.020
is obviously a huge achievement in many,
link |
00:42:09.980
both experimentally and theoretically.
link |
00:42:12.300
On the other hand, it's like having a jigsaw puzzle
link |
00:42:15.260
where every piece has been filled in.
link |
00:42:17.100
You have this beautiful image, there's one gap
link |
00:42:19.020
and you kind of know that piece must be there somewhere.
link |
00:42:22.860
So the discovery in itself, although it's important,
link |
00:42:29.020
is not so interesting.
link |
00:42:30.420
It's like a confirmation of the obvious at that point.
link |
00:42:34.340
But what makes it interesting
link |
00:42:36.020
is not that it just completes the standard model,
link |
00:42:38.080
which is a theory that we've known
link |
00:42:39.980
had the basic layout offs for 40 years or more now.
link |
00:42:44.780
It's that the Higgs actually is a unique particle.
link |
00:42:48.420
It's very different to any of the other particles
link |
00:42:50.540
in the standard model.
link |
00:42:51.860
And it's a theoretically very troublesome particle.
link |
00:42:55.260
There are a lot of nasty things to do with the Higgs,
link |
00:42:59.240
but also opportunities.
link |
00:43:00.860
So that we basically, we don't really understand
link |
00:43:02.580
how such an object can exist in the form that it does.
link |
00:43:06.260
So there are lots of reasons for thinking
link |
00:43:08.500
that the Higgs must come with a bunch of other particles
link |
00:43:12.540
or that it's perhaps made of other things.
link |
00:43:15.020
So it's not a fundamental particle,
link |
00:43:16.460
that it's made of smaller things.
link |
00:43:17.940
I can talk about that if you like a bit.
link |
00:43:19.580
That's still a notion, so the Higgs
link |
00:43:23.180
might not be a fundamental particle,
link |
00:43:24.820
that there might be some, it might, oh man.
link |
00:43:27.180
So that is an idea, it's not been demonstrated to be true.
link |
00:43:31.080
But I mean, all of these ideas basically come
link |
00:43:33.820
from the fact that this is a problem
link |
00:43:37.940
that motivated a lot of development in physics
link |
00:43:40.100
in the last 30 years or so.
link |
00:43:42.380
And it's this basic fact that the Higgs field,
link |
00:43:44.780
which is this field that's everywhere in the universe,
link |
00:43:47.260
this is the thing that gives mass to the particles.
link |
00:43:49.060
And the Higgs field is different from all the other fields
link |
00:43:51.340
in that, let's say you take the electromagnetic field,
link |
00:43:54.420
which is, if we actually were to measure
link |
00:43:56.080
the electromagnetic field in this room,
link |
00:43:57.420
we would measure all kinds of stuff going on
link |
00:43:58.900
because there's light, there's gonna be microwaves
link |
00:44:00.940
and radio waves and stuff.
link |
00:44:02.100
But let's say we could go to a really, really remote part
link |
00:44:04.940
of empty space and shield it and put a big box around it
link |
00:44:07.660
and then measure the electromagnetic field in that box.
link |
00:44:10.060
The field would be almost zero,
link |
00:44:12.180
apart from some little quantum fluctuations,
link |
00:44:14.780
but basically it goes to naught.
link |
00:44:16.980
The Higgs field has a value everywhere.
link |
00:44:19.140
So it's a bit like the whole,
link |
00:44:20.700
it's like the entire space has got this energy
link |
00:44:23.440
stored in the Higgs field, which is not zero,
link |
00:44:25.420
it's finite, it's a bit like having the temperature
link |
00:44:28.860
of space raised to some background temperature.
link |
00:44:33.900
And it's that energy that gives mass to the particles.
link |
00:44:36.900
So the reason that electrons and quarks have mass
link |
00:44:40.460
is through the interaction with this energy
link |
00:44:42.440
that's stored in the Higgs field.
link |
00:44:44.820
Now, it turns out that the precise value this energy has
link |
00:44:50.620
has to be very carefully tuned if you want a universe
link |
00:44:55.700
where interesting stuff can happen.
link |
00:44:58.140
So if you push the Higgs field down,
link |
00:45:00.660
it has a tendency to collapse to,
link |
00:45:03.100
well, there's a tendency,
link |
00:45:04.020
if you do your sort of naive calculations,
link |
00:45:05.620
there are basically two possible likely configurations
link |
00:45:08.260
for the Higgs field, which is either it's zero everywhere,
link |
00:45:11.320
in which case you have a universe
link |
00:45:12.480
which is just particles with no mass that can't form atoms
link |
00:45:15.860
and just fly about at the speed of light,
link |
00:45:18.060
or it explodes to an enormous value,
link |
00:45:20.700
what we call the Planck scale,
link |
00:45:21.820
which is the scale of quantum gravity.
link |
00:45:24.140
And at that point, if the Higgs field was that strong,
link |
00:45:27.060
even an electron would become so massive
link |
00:45:28.900
that it would collapse into a black hole.
link |
00:45:31.200
And then you have a universe made of black holes
link |
00:45:33.100
and nothing like us.
link |
00:45:34.940
So it seems that the strength of the Higgs field
link |
00:45:37.640
is to achieve the value that we see
link |
00:45:40.180
requires what we call fine tuning of the laws of physics.
link |
00:45:42.900
You have to fiddle around with the other fields
link |
00:45:45.340
in the Standard Model and their properties
link |
00:45:47.340
to just get it to this right sort of Goldilocks value
link |
00:45:50.780
that allows atoms to exist.
link |
00:45:53.100
This is deeply fishy.
link |
00:45:54.580
People really dislike this.
link |
00:45:57.380
Well, yeah, I guess, so what would be,
link |
00:45:59.420
so two explanations.
link |
00:46:00.840
One, there's a god that designed this perfectly,
link |
00:46:03.060
and two is there's an infinite number
link |
00:46:05.580
of alternate universes,
link |
00:46:07.020
and we just happen to be in the one in which life
link |
00:46:10.300
is possible, complexity.
link |
00:46:12.380
So when you say, I mean, life, any kind of complexity,
link |
00:46:15.540
that's not either complete chaos or black holes.
link |
00:46:21.500
I mean, how does that make you feel?
link |
00:46:22.760
What do you make of that?
link |
00:46:23.600
That's such a fascinating notion
link |
00:46:25.260
that this perfectly tuned field
link |
00:46:28.340
that's the same everywhere is there.
link |
00:46:31.120
What do you make of that?
link |
00:46:33.140
Yeah, what do you make of that?
link |
00:46:34.200
I mean, yeah, so you laid out
link |
00:46:35.300
two of the possible explanations.
link |
00:46:36.660
Really?
link |
00:46:37.500
Some, well, yeah, I mean, well,
link |
00:46:38.820
someone, some cosmic creator went,
link |
00:46:41.060
yeah, let's fix that to be at the right level.
link |
00:46:43.140
That's one possibility, I guess.
link |
00:46:44.420
It's not a scientifically testable one,
link |
00:46:45.900
but theoretically, I guess, it's possible.
link |
00:46:48.740
Sorry to interrupt, but there could also be
link |
00:46:50.860
not a designer, but couldn't there be just,
link |
00:46:54.540
I guess I'm not sure what that would be,
link |
00:46:55.980
but some kind of force that,
link |
00:46:58.240
that some kind of mechanism
link |
00:47:03.240
by which this kind of field is enforced
link |
00:47:09.840
in order to create complexity,
link |
00:47:11.920
basically forces that pull the universe
link |
00:47:16.280
towards an interesting complexity.
link |
00:47:19.800
I mean, yeah, I mean, there are people
link |
00:47:21.360
who have those ideas.
link |
00:47:22.280
I don't really subscribe to them.
link |
00:47:23.600
As I'm saying, it sounds really stupid.
link |
00:47:25.520
No, I mean, there are definitely people
link |
00:47:27.120
that make those kind of arguments.
link |
00:47:29.400
There's ideas that, I think it's Lee Smolin's idea,
link |
00:47:33.040
or one, I think, that universes are born inside black holes.
link |
00:47:38.120
And so, universes, they basically have
link |
00:47:40.280
like Darwinian evolution of the universe,
link |
00:47:42.480
where universes give birth to other universes.
link |
00:47:44.800
And if universes where black holes can form
link |
00:47:46.720
are more likely to give birth to more universes,
link |
00:47:48.760
so you end up with universes which have similar laws.
link |
00:47:51.260
I mean, I don't know, whatever.
link |
00:47:52.600
Well, I talked to Lee recently on this podcast,
link |
00:47:57.080
and he's a reminder to me that the physics community
link |
00:48:02.360
has like so many interesting characters in it.
link |
00:48:05.600
It's fascinating.
link |
00:48:06.960
Anyway, sorry, so.
link |
00:48:08.040
I mean, as an experimentalist, I tend to sort of think,
link |
00:48:10.120
these are interesting ideas, but they're not really testable,
link |
00:48:12.760
so I tend not to think about them very much.
link |
00:48:14.720
So, I mean, going back to the science of this,
link |
00:48:17.600
there is an explanation.
link |
00:48:19.120
There is a possible solution to this problem of the Higgs,
link |
00:48:21.240
which doesn't involve multiverses or creators fiddling about
link |
00:48:25.200
with the laws of physics.
link |
00:48:26.560
If the most popular solution
link |
00:48:28.400
was something called supersymmetry,
link |
00:48:30.440
which is a theory which involves a new type of symmetry
link |
00:48:34.800
of the universe.
link |
00:48:35.720
In fact, it's one of the last types of symmetries
link |
00:48:37.680
that it's possible to have
link |
00:48:38.560
that we haven't already seen in nature,
link |
00:48:40.400
which is a symmetry between force particles
link |
00:48:43.600
and matter particles.
link |
00:48:44.760
So what we call fermions, which are the matter particles
link |
00:48:47.880
and bosons, which are force particles.
link |
00:48:49.920
And if you have supersymmetry, then there is a super partner
link |
00:48:52.600
for every particle in the standard model.
link |
00:48:55.920
And without going into the details,
link |
00:48:57.520
the effect of this basically is that you have
link |
00:48:59.320
a whole bunch of other fields,
link |
00:49:01.320
and these fields cancel out the effect
link |
00:49:04.240
of the standard model fields,
link |
00:49:05.680
and they stabilize the Higgs field at a nice sensible value.
link |
00:49:09.000
So in supersymmetry, you naturally,
link |
00:49:11.360
without any tinkering about with the constants of nature
link |
00:49:14.280
or anything, you get a Higgs field with a nice value,
link |
00:49:17.360
which is the one we see.
link |
00:49:18.960
So this is one of the,
link |
00:49:20.200
and supersymmetry's also got lots of other things
link |
00:49:22.000
going for it.
link |
00:49:22.840
It predicts the existence of a dark matter particle,
link |
00:49:25.360
which would be great.
link |
00:49:27.000
It potentially suggests that the strong force
link |
00:49:30.120
and the electroweak force unify at high energy.
link |
00:49:32.760
So lots of reasons people thought this was a productive idea.
link |
00:49:35.360
And when the LHC was, just before it was turned on,
link |
00:49:37.800
there was a lot of hype, I guess,
link |
00:49:39.600
a lot of an expectation that we would discover
link |
00:49:42.440
these super partners because,
link |
00:49:44.280
and particularly the main reason was
link |
00:49:46.080
that if supersymmetry stabilizes the Higgs field
link |
00:49:50.240
at this nice Goldilocks value,
link |
00:49:52.960
these super particles should have a mass
link |
00:49:55.760
around the energy that we're probing at the LHC,
link |
00:49:58.520
around the energy of the Higgs.
link |
00:49:59.920
So it was kind of thought, you discover the Higgs,
link |
00:50:01.520
you probably discover super partners as well.
link |
00:50:03.600
So once you start creating ripples in this Higgs field,
link |
00:50:06.200
you should be able to see these kinds of,
link |
00:50:08.680
you should be, yeah.
link |
00:50:09.520
So the super fields would be there.
link |
00:50:11.000
When I, at the very beginning I said,
link |
00:50:12.320
we're probing the vacuum.
link |
00:50:13.720
What I mean is really that, you know,
link |
00:50:15.200
okay, let's say these super fields exist.
link |
00:50:16.680
The vacuum contains super fields.
link |
00:50:18.200
They're there, these supersymmetric fields.
link |
00:50:20.160
If we hit them hard enough, we can make them vibrate.
link |
00:50:22.640
We see super particles come flying out.
link |
00:50:24.840
That's the sort of, that's the idea.
link |
00:50:26.320
That's the whole, okay.
link |
00:50:27.160
That's the whole point.
link |
00:50:29.600
But we haven't.
link |
00:50:30.680
But we haven't.
link |
00:50:31.520
So, so far at least, I mean,
link |
00:50:33.240
we've had now a decade of data taking at the LHC.
link |
00:50:38.920
No signs of super partners have,
link |
00:50:41.760
supersymmetric particles have been found.
link |
00:50:43.360
In fact, no signs of any physics, any new particles
link |
00:50:46.000
beyond the Standard Model have been found.
link |
00:50:47.520
So supersymmetry is not the only thing that can do this.
link |
00:50:49.520
There are other theories that involve
link |
00:50:51.440
additional dimensions of space
link |
00:50:53.160
or potentially involve the Higgs boson
link |
00:50:55.680
being made of smaller things,
link |
00:50:56.920
being made of other particles.
link |
00:50:58.360
Yeah, that's an interesting, you know,
link |
00:50:59.480
I haven't heard that before.
link |
00:51:00.560
That's really, that's an interesting,
link |
00:51:02.320
but can you maybe linger on that?
link |
00:51:03.640
Like what, what could be,
link |
00:51:06.400
what could the Higgs particle be made of?
link |
00:51:08.880
Well, so the oldest, I think the original ideas about this
link |
00:51:11.560
was these theories called technicolor,
link |
00:51:14.080
which were basically like an analogy with the strong force.
link |
00:51:17.320
So the idea was the Higgs boson was a bound state
link |
00:51:21.440
of two very strongly interacting particles
link |
00:51:24.480
that were a bit like quarks.
link |
00:51:25.560
So like quarks, but I guess higher energy things
link |
00:51:29.200
with a super strong force.
link |
00:51:30.440
So not the strong force, but a new force
link |
00:51:31.880
that was very strong.
link |
00:51:33.000
And the Higgs was a bound state of these, these objects.
link |
00:51:36.480
And the Higgs would in principle, if that was right,
link |
00:51:38.440
would be the first in a series of technicolor particles.
link |
00:51:42.400
Technicolor, I think not being a theorist,
link |
00:51:45.560
but it's not, it's basically not done very well,
link |
00:51:48.120
particularly since the LHC found the Higgs,
link |
00:51:49.600
that kind of, it rules out, you know,
link |
00:51:52.360
a lot of these technicolor theories,
link |
00:51:53.440
but there are other things that are a bit like technicolor.
link |
00:51:55.440
So there's a theory called partial composite,
link |
00:52:00.560
which is an idea that some of my colleagues
link |
00:52:02.560
at Cambridge have worked on,
link |
00:52:04.360
which is a similar sort of idea that the Higgs
link |
00:52:06.840
is a bound state of some strongly interacting particles,
link |
00:52:10.440
and that the standard model particles themselves,
link |
00:52:13.000
the more exotic ones like the top quark
link |
00:52:16.000
are also sort of mixtures of these composite particles.
link |
00:52:20.480
So it's a kind of an extension to the standard model,
link |
00:52:23.320
which explains this problem
link |
00:52:25.280
with the Higgs bosons, Goldilocks value,
link |
00:52:28.560
but also helps us understand we have,
link |
00:52:31.160
we're in a situation now, again,
link |
00:52:32.840
a bit like the periodic table,
link |
00:52:34.480
where we have six quarks, six leptons in this kind of,
link |
00:52:38.640
you can arrange in this nice table
link |
00:52:40.000
and you can see these columns where the patterns repeat
link |
00:52:42.480
and you go, okay, maybe there's something deeper
link |
00:52:46.160
going on here, you know,
link |
00:52:47.640
and so this would potentially be something,
link |
00:52:49.640
this partial composite theory could explain,
link |
00:52:52.880
a sort of enlarge this picture
link |
00:52:54.360
that allows us to see the whole symmetrical pattern
link |
00:52:56.480
and understand what the ingredients, why do we have,
link |
00:52:59.120
so one of the big questions in particle physics is,
link |
00:53:02.160
why are there three copies of the matter particles?
link |
00:53:06.240
So in what we call the first generation,
link |
00:53:07.920
which is what we're made of,
link |
00:53:08.920
there's the electron, the electron neutrino,
link |
00:53:11.760
the up quark and the down quark,
link |
00:53:13.160
they're the most common matter particles in the universe,
link |
00:53:15.640
but then there are copies of these four particles
link |
00:53:18.800
in the second and the third generations,
link |
00:53:20.360
so things like nuons and top quarks and other stuff,
link |
00:53:23.120
we don't know why, we see these patterns,
link |
00:53:25.240
we have no idea where it comes from,
link |
00:53:26.440
so that's another big question, you know,
link |
00:53:28.880
can we find out the deeper order that explains
link |
00:53:32.920
this particular periodic table of particles that we see?
link |
00:53:36.440
Is it possible that the deeper order includes
link |
00:53:40.240
like almost a single entity,
link |
00:53:42.400
so like something that I guess like string theory
link |
00:53:44.960
dreams about, is this essentially the dream,
link |
00:53:50.240
is to discover something simple, beautiful and unifying?
link |
00:53:54.120
Yeah, I mean, that is the dream,
link |
00:53:55.640
and I think for some people, for a lot of people,
link |
00:53:59.480
it still is the dream,
link |
00:54:00.400
so there's a great book by Steven Weinberg,
link |
00:54:03.800
who is one of the theoretical physicists
link |
00:54:05.760
who was instrumental in building the Standard Model,
link |
00:54:08.360
so he came up with some others with the electroweak theory,
link |
00:54:12.000
the theory that unified electromagnetism and the weak force,
link |
00:54:14.560
and he wrote this book,
link |
00:54:15.680
I think it was towards the end of the 80s, early 90s,
link |
00:54:18.080
called Dreams of a Final Theory,
link |
00:54:20.000
which is a very lovely, quite short book
link |
00:54:22.920
about this idea of a final unifying theory
link |
00:54:26.200
that brings everything together,
link |
00:54:27.560
and I think you get a sense reading his book
link |
00:54:29.440
written at the end of the 80s, early 90s,
link |
00:54:31.760
that there was this feeling that such a theory was coming,
link |
00:54:37.760
and that was the time when string theory
link |
00:54:39.200
was very exciting, so string theory,
link |
00:54:41.960
there's been this thing called the superstring revolution,
link |
00:54:44.080
and theoretical physicists were very excited,
link |
00:54:46.080
they discovered these theoretical objects,
link |
00:54:47.960
these little vibrating loops of string
link |
00:54:49.440
that in principle not only was a quantum theory of gravity
link |
00:54:52.440
but could explain all the particles in the Standard Model
link |
00:54:54.840
and bring it all together,
link |
00:54:55.760
and as you say, you have one object, the string,
link |
00:54:59.520
and you can pluck it, and the way it vibrates
link |
00:55:02.560
gives you these different notes,
link |
00:55:03.840
each of which is a different particle,
link |
00:55:05.960
so it's a very lovely idea,
link |
00:55:08.160
but the problem is that, well, there's a few,
link |
00:55:11.920
people discover that mathematics is very difficult,
link |
00:55:14.680
so people have spent three decades or more
link |
00:55:17.640
trying to understand string theory,
link |
00:55:19.120
and I think if you spoke to most string theorists,
link |
00:55:21.520
they would probably freely admit
link |
00:55:22.640
that no one really knows what string theory is yet,
link |
00:55:24.920
I mean, there's been a lot of work,
link |
00:55:26.000
but it's not really understood,
link |
00:55:27.320
and the other problem is that string theory
link |
00:55:31.240
mostly makes predictions about physics
link |
00:55:34.040
that occurs at energies far beyond
link |
00:55:36.560
what we will ever be able to probe in the laboratory.
link |
00:55:40.600
Yeah, probably ever.
link |
00:55:42.200
By the way, so sorry to take a million tangents,
link |
00:55:44.840
but is there room for complete innovation
link |
00:55:48.080
of how to build a particle collider
link |
00:55:50.240
that could give us an order of magnitude increase
link |
00:55:52.720
in the kind of energies,
link |
00:55:55.200
or do we need to keep just increasing the size of things?
link |
00:55:58.520
I mean, maybe, yeah, I mean, there are ideas,
link |
00:56:00.920
to give you a sense of the gulf that has to be bridged.
link |
00:56:03.920
So the LHC collides particles at an energy
link |
00:56:09.320
of what we call 14 tera electron volts,
link |
00:56:13.440
so that's basically the equivalent
link |
00:56:15.040
if you've accelerated a proton through 14 trillion volts.
link |
00:56:19.200
That gets us to the energies
link |
00:56:20.520
where the Higgs and these weak particles live.
link |
00:56:23.240
They're very massive.
link |
00:56:24.480
The scale where strings become manifest
link |
00:56:27.760
is something called the Planck scale,
link |
00:56:29.320
which I think is of the order 10 to the,
link |
00:56:31.960
hang on, get this right,
link |
00:56:33.720
it's 10 to the 18 giga electron volts,
link |
00:56:35.840
so about 10 to the 15 tera electron volts.
link |
00:56:41.000
So you're talking trillions of times more energy.
link |
00:56:44.760
Yeah, 10 to the 15th or 10 to the 14th larger, I don't even.
link |
00:56:49.760
It's of that order.
link |
00:56:50.840
It's a very big number.
link |
00:56:52.680
So we're not talking just an order
link |
00:56:54.400
of magnitude increase in energy,
link |
00:56:55.600
we're talking 14 orders of magnitude energy increase.
link |
00:56:58.600
So to give you a sense of what that would look like,
link |
00:57:01.160
were you to build a particle accelerator
link |
00:57:03.000
with today's technology.
link |
00:57:04.760
Bigger or smaller than our solar system?
link |
00:57:07.960
The size of the galaxy.
link |
00:57:09.120
The galaxy.
link |
00:57:10.040
So you'd need to put a particle accelerator
link |
00:57:11.480
that circled the Milky Way to get to the energies
link |
00:57:14.560
where you would see strings if they exist.
link |
00:57:17.600
So that is a fundamental problem,
link |
00:57:20.400
which is that most of the predictions
link |
00:57:22.600
of these unified theories, quantum theories of gravity,
link |
00:57:26.040
only make statements that are testable at energies
link |
00:57:29.200
that we will not be able to probe,
link |
00:57:32.200
and barring some unbelievable,
link |
00:57:35.200
completely unexpected technological
link |
00:57:37.160
or scientific breakthrough,
link |
00:57:38.080
which is almost impossible to imagine.
link |
00:57:40.000
You never say never, but it seems very unlikely.
link |
00:57:42.800
Yeah, I can just see the news story.
link |
00:57:45.120
Elon Musk decides to build a particle collider
link |
00:57:48.840
the size of our galaxy.
link |
00:57:51.080
We'd have to get together
link |
00:57:51.920
with all our galactic neighbors to pay for it, I think.
link |
00:57:55.120
What is the exciting possibilities
link |
00:57:56.720
of the Large Hadron Collider?
link |
00:57:58.960
What is there to be discovered
link |
00:58:00.640
in this order of magnitude of scale?
link |
00:58:04.160
Is there other bigger efforts on the horizon in this space?
link |
00:58:09.800
What are the open problems, the exciting possibilities?
link |
00:58:12.720
You mentioned supersymmetry.
link |
00:58:14.560
Yeah, so, well, there are lots of new ideas.
link |
00:58:17.600
Well, there are lots of problems that we're facing.
link |
00:58:18.920
So there's a problem with the Higgs field,
link |
00:58:20.160
which supersymmetry was supposed to solve.
link |
00:58:23.320
There's the fact that 95% of the universe
link |
00:58:25.720
we know from cosmology, astrophysics, is invisible,
link |
00:58:29.360
that it's made of dark matter and dark energy,
link |
00:58:31.840
which are really just words
link |
00:58:33.520
for things that we don't know what they are.
link |
00:58:35.360
It's what Donald Rumsfeld called a known unknown.
link |
00:58:37.920
So we know we don't know what they are.
link |
00:58:39.880
Well, that's better than unknown unknown.
link |
00:58:42.480
Yeah, well, there may be some unknown unknowns,
link |
00:58:43.800
but by definition we don't know what those are, so, yeah.
link |
00:58:47.360
But the hope is a particle accelerator
link |
00:58:52.480
could help us make sense of dark energy, dark matter.
link |
00:58:55.560
There's still, there's some hope for that?
link |
00:58:57.680
There's hope for that, yeah.
link |
00:58:58.760
So one of the hopes is the LHC could produce
link |
00:59:01.400
a dark matter particle in its collisions.
link |
00:59:03.800
And it may be that the LHC
link |
00:59:08.360
will still discover new particles,
link |
00:59:09.920
that it might still, supersymmetry could still be there.
link |
00:59:11.920
It's just maybe more difficult to find
link |
00:59:14.320
than we thought originally.
link |
00:59:15.640
And dark matter particles might be being produced,
link |
00:59:18.520
but we're just not looking in the right part of the data
link |
00:59:20.600
for them, that's possible.
link |
00:59:22.120
It might be that we need more data,
link |
00:59:23.320
that these processes are very rare
link |
00:59:24.800
and we need to collect lots and lots of data
link |
00:59:26.600
before we see them.
link |
00:59:27.600
But I think a lot of people would say now
link |
00:59:29.880
that the chances of the LHC
link |
00:59:33.720
directly discovering new particles
link |
00:59:36.000
in the near future is quite slim.
link |
00:59:37.760
It may be that we need a decade more data
link |
00:59:40.800
before we can see something, or we may not see anything.
link |
00:59:43.920
That's the, that's where we are.
link |
00:59:45.480
So, I mean, the physics, the experiments that I work on,
link |
00:59:48.960
so I work on a detector called LHCb,
link |
00:59:50.760
which is one of these four big detectors
link |
00:59:52.760
that are spaced around the ring.
link |
00:59:54.400
And we do slightly different stuff to the big guys.
link |
00:59:57.520
There's two big experiments called Atlas and CMS,
link |
01:00:00.600
3000 physicists and scientists
link |
01:00:02.720
and computer scientists on them each.
link |
01:00:04.760
They are the ones that discovered the Higgs
link |
01:00:06.080
and they look for supersymmetry and dark matter and so on.
link |
01:00:08.560
What we look at are standard model particles
link |
01:00:11.200
called bequarks, which depending on your preferences,
link |
01:00:14.880
either bottom or beauty,
link |
01:00:16.600
we tend to say beauty because it sounds sexier.
link |
01:00:18.800
Yeah, for sure.
link |
01:00:20.440
But these particles are interesting
link |
01:00:22.680
because they have, we can make lots of them.
link |
01:00:25.840
We make billions or hundreds of billions of these things.
link |
01:00:28.880
You can therefore measure their properties very precisely.
link |
01:00:31.560
So you can make these really lovely precision measurements.
link |
01:00:34.400
And what we are doing really is a sort of complimentary thing
link |
01:00:39.400
to the other big experiments, which is they,
link |
01:00:41.920
if you think of the sort of analogy they often use is,
link |
01:00:44.120
if you imagine you're looking in, you're in the jungle
link |
01:00:45.800
and you're looking for an elephant, say,
link |
01:00:48.680
and you are a hunter and you're kind of like,
link |
01:00:52.040
let's say there's the relevance, very rare.
link |
01:00:53.520
You don't know where in the jungle, the jungle's big.
link |
01:00:55.440
So there's two ways you go about this.
link |
01:00:56.760
Either you can go wandering around the jungle
link |
01:00:58.720
and try and find the elephant.
link |
01:01:00.160
The problem is if the elephant,
link |
01:01:01.320
if there's only one elephant and the jungle's big,
link |
01:01:02.720
the chances of running into it are very small.
link |
01:01:04.760
Or you could look on the ground
link |
01:01:07.200
and see if you see footprints left by the elephant.
link |
01:01:09.200
And if the elephant's moving around, you've got a chance,
link |
01:01:11.480
that you're better chance maybe
link |
01:01:12.320
of seeing the elephant's footprints.
link |
01:01:13.880
If you see the footprints, you go, okay, there's an elephant.
link |
01:01:16.080
I maybe don't know what kind of elephant it is,
link |
01:01:18.320
but I got a sense there's something out there.
link |
01:01:20.000
So that's sort of what we do.
link |
01:01:21.600
We are the footprint people.
link |
01:01:23.040
We are, we're looking for the footprints,
link |
01:01:25.800
the impressions that quantum fields
link |
01:01:28.800
that we haven't managed to directly create the particle of,
link |
01:01:32.600
the effects these quantum fields have
link |
01:01:33.960
on the ordinary standard model fields
link |
01:01:35.560
that we already know about.
link |
01:01:36.480
So these B particles, the way they behave
link |
01:01:39.760
can be influenced by the presence of say,
link |
01:01:41.720
super fields or dark matter fields or whatever you like.
link |
01:01:45.200
And the way they decay and behave can be altered slightly
link |
01:01:48.640
from what our theory tells us they ought to behave.
link |
01:01:52.480
And it's easier to collect huge amounts of data
link |
01:01:54.600
on B quarks.
link |
01:01:56.600
We get billions and billions of these things.
link |
01:01:58.440
You can make very precise measurements.
link |
01:02:00.280
And the only place really at the LHC
link |
01:02:03.200
or really in high energy physics at the moment
link |
01:02:05.200
where there's fairly compelling evidence
link |
01:02:08.920
that there might be something beyond the standard model
link |
01:02:10.960
is in these B, these beauty quarks decays.
link |
01:02:15.320
Just to clarify, which is the difference
link |
01:02:18.640
between the different, the four experiments,
link |
01:02:20.320
for example, that you mentioned,
link |
01:02:21.600
is it the kind of particles that are being collided?
link |
01:02:24.760
Is it the energies which they're collided?
link |
01:02:27.160
What's the fundamental difference
link |
01:02:28.960
between the different experiments?
link |
01:02:30.440
The collisions are the same.
link |
01:02:32.280
What's different is the design of the detectors.
link |
01:02:34.480
So Atlas and CMS are called,
link |
01:02:37.040
they're called what are called general purpose detectors.
link |
01:02:39.760
And they are basically barrel shaped machines
link |
01:02:42.360
and the collisions happen in the middle of the barrel
link |
01:02:44.440
and the barrel captures all the particles
link |
01:02:46.600
that go flying out in every direction.
link |
01:02:48.040
So in a sphere effectively that can fly out
link |
01:02:49.840
and it can record all of those particles.
link |
01:02:51.840
And what's the, sorry to be interrupting,
link |
01:02:54.720
but what's the mechanism of the recording?
link |
01:02:57.440
Oh, so these detectors, if you've seen pictures of them,
link |
01:02:59.520
they're huge, like Atlas is 25 meters high
link |
01:03:03.080
and 45 meters long, they're vast machines,
link |
01:03:07.760
instruments, I guess you should call them really.
link |
01:03:09.600
They are, they're kind of like onions.
link |
01:03:11.760
So they have layers, concentric layers of detectors,
link |
01:03:15.360
different sorts of detectors.
link |
01:03:16.480
So close into the beam pipe,
link |
01:03:18.160
you have what are called usually made of silicon,
link |
01:03:20.600
they're tracking detectors.
link |
01:03:21.720
So they're little made of strips of silicon
link |
01:03:23.600
or pixels of silicon.
link |
01:03:24.960
And when a particle goes through the silicon,
link |
01:03:26.800
it gives a little electrical signal
link |
01:03:28.520
and you get these dots, electrical dots
link |
01:03:30.280
through your detector, which allows you
link |
01:03:31.440
to reconstruct the trajectory of the particle.
link |
01:03:34.120
So that's the middle
link |
01:03:34.960
and then the outsides of these detectors,
link |
01:03:36.280
you have things called calorimeters,
link |
01:03:37.720
which measure the energies of the particles
link |
01:03:39.600
and the very edge you have things called muon chambers,
link |
01:03:42.640
which basically these muon particles,
link |
01:03:44.680
which are the heavy version of the electron,
link |
01:03:46.720
they're like high velocity bullets
link |
01:03:48.440
and they can get right to the edge of the detectors.
link |
01:03:50.120
If you see something at the edge, that's a muon.
link |
01:03:52.480
So that's broadly how they work.
link |
01:03:54.000
And all of that is being recorded.
link |
01:03:55.720
That's all being fed out to, you know, computers.
link |
01:03:58.280
Data must be awesome, okay.
link |
01:04:00.800
So LHCb is different.
link |
01:04:02.000
So we, because we're looking for these be quarks,
link |
01:04:04.680
be quarks tend to be produced along the beam line.
link |
01:04:07.960
So in a collision, the be quark tend to fly
link |
01:04:10.640
sort of close to the beam pipe.
link |
01:04:12.840
So we built a detector that sort of pyramid cone shaped
link |
01:04:15.520
basically, that just looks in one direction.
link |
01:04:18.120
So we ignore, if you have your collision,
link |
01:04:20.280
stuff goes everywhere.
link |
01:04:21.120
We ignore all the stuff over here and going off sideways.
link |
01:04:23.400
We're just looking in this little region
link |
01:04:26.240
close to the beam pipe
link |
01:04:27.080
where most of these be quarks are made.
link |
01:04:28.720
So is there a different aspect of the sensors involved
link |
01:04:34.160
in the collection of the be quark trajectories?
link |
01:04:37.600
There are some differences.
link |
01:04:38.720
So one of the differences is that,
link |
01:04:40.840
one of the ways you know you've seen a be quark
link |
01:04:42.600
is that be quarks are actually quite long lived
link |
01:04:44.880
by particle standards.
link |
01:04:45.920
So they live for 1.5 trillionths of a second,
link |
01:04:49.120
which is if you're a fundamental particle
link |
01:04:50.600
is a very long time.
link |
01:04:51.640
Cause the Higgs boson, I think lives for about
link |
01:04:54.600
a trillionth of a trillionth of a second,
link |
01:04:57.240
or maybe even less than that.
link |
01:04:58.400
So these are quite long lived things
link |
01:05:00.760
and they will actually fly a little distance
link |
01:05:02.600
before they decay.
link |
01:05:03.440
So they will fly a few centimeters maybe if you're lucky,
link |
01:05:06.280
then they'll decay into other stuff.
link |
01:05:07.920
So what we need to do in the middle of the detector,
link |
01:05:10.360
you wanna be able to see,
link |
01:05:12.160
you have your place where the protons crash into each other
link |
01:05:14.560
and that produces loads of particles that come flying out.
link |
01:05:16.880
So you have loads of lines, loads of tracks
link |
01:05:18.960
that point back to that proton collision.
link |
01:05:21.320
And then you're looking for a couple of other tracks,
link |
01:05:23.400
maybe two or three that point back to a different place
link |
01:05:25.880
that's maybe a few centimeters away
link |
01:05:27.360
from the proton collision.
link |
01:05:28.400
And that's the sign that a little B particle has flown
link |
01:05:31.560
a few centimeters and decayed somewhere else.
link |
01:05:33.240
So we need to be able to very accurately resolve
link |
01:05:36.760
the proton collision from the B particle decay.
link |
01:05:39.480
So the middle of our detector is very sensitive
link |
01:05:42.360
and it gets very close to the collision.
link |
01:05:44.160
So you have this really beautiful delicate
link |
01:05:46.520
silicon detector that sits,
link |
01:05:48.360
I think it's seven millimeters from the beam.
link |
01:05:52.360
And the LHC beam has as much energy
link |
01:05:53.920
as a jumbo jet at takeoff.
link |
01:05:55.200
So it's enough to melt a ton of copper.
link |
01:05:57.360
So you have this furiously powerful thing sitting next
link |
01:05:59.840
to this tiny delicate silicon sensor.
link |
01:06:03.360
So those aspects of our detector that are specialized
link |
01:06:07.120
to measure these particular B quarks
link |
01:06:09.840
that we're interested in.
link |
01:06:10.880
And is there, I mean, I remember seeing somewhere
link |
01:06:12.960
that there's some mention of matter and antimatter
link |
01:06:15.360
connected to the B, these beautiful quarks.
link |
01:06:18.280
Is that, what's the connection?
link |
01:06:23.600
Yeah, what's the connection there?
link |
01:06:25.880
Yeah, so there is a connection, which is that
link |
01:06:29.600
when you produce these B particles,
link |
01:06:31.880
these particles, because you don't see the B quark,
link |
01:06:33.760
you see the thing that B quark is inside.
link |
01:06:35.400
So they're bound up inside what we call beauty particles,
link |
01:06:37.960
where the B quark is joined together with another quark
link |
01:06:40.640
or two, maybe two other quarks, depending on what it is.
link |
01:06:43.400
They're a particular set of these B particles
link |
01:06:46.160
that exhibit this property called oscillation.
link |
01:06:49.480
So if you make a, for the sake of argument,
link |
01:06:52.280
a matter version of one of these B particles,
link |
01:06:55.440
as it travels, because of the magic of quantum mechanics,
link |
01:06:58.840
it oscillates backwards and forwards
link |
01:07:01.040
between its matter and antimatter versions.
link |
01:07:03.880
So it does this weird flipping about backwards and forwards.
link |
01:07:06.720
And what we can use this for is a laboratory
link |
01:07:09.160
for testing the symmetry between matter and antimatter.
link |
01:07:12.880
So if the symmetry between antimatter is precise,
link |
01:07:15.680
it's exact, then we should see these B particles decaying
link |
01:07:20.040
as often as matter, as they do as antimatter,
link |
01:07:21.840
because this oscillation should be even.
link |
01:07:23.360
It should spend as much time in each state.
link |
01:07:26.000
But what we actually see is that one of the states,
link |
01:07:29.000
it spends more time and it's more likely to decay
link |
01:07:31.720
in one state than the other.
link |
01:07:32.800
So this gives us a way of testing this fundamental symmetry
link |
01:07:36.960
between matter and antimatter.
link |
01:07:39.160
So what can you, sort of returning to the question
link |
01:07:42.400
before about this fundamental symmetry,
link |
01:07:44.480
it seems like if there's perfect symmetry
link |
01:07:46.520
between matter and antimatter,
link |
01:07:50.560
if we have the equal amount of each in our universe,
link |
01:07:54.600
it would just destroy itself.
link |
01:07:57.000
And just like you mentioned,
link |
01:07:58.760
we seem to live in a very unlikely universe
link |
01:08:00.920
where it doesn't destroy itself.
link |
01:08:03.520
So do you have some intuition about why that is?
link |
01:08:07.280
I mean, well, I'm not a theorist.
link |
01:08:10.160
I don't have any particular ideas myself.
link |
01:08:11.680
I mean, I sort of do measurements
link |
01:08:13.120
to try and test these things,
link |
01:08:14.200
but I mean, so the terms of the basic problem
link |
01:08:16.000
is that in the Big Bang,
link |
01:08:17.800
if you use the standard model to figure out
link |
01:08:19.240
what ought to have happened,
link |
01:08:20.120
you should have got equal amounts of matter
link |
01:08:21.640
and antimatter made,
link |
01:08:22.480
because whenever you make a particle
link |
01:08:23.880
in our collisions, for example,
link |
01:08:25.440
when we collide stuff together,
link |
01:08:26.800
you make a particle, you make an antiparticle.
link |
01:08:28.440
They always come together.
link |
01:08:29.480
They always annihilate together.
link |
01:08:30.920
So there's no way of making more matter than antimatter
link |
01:08:33.440
that we've discovered so far.
link |
01:08:35.040
So that means in the Big Bang,
link |
01:08:36.080
you get equal amounts of matter and antimatter.
link |
01:08:38.200
As the universe expands and cools down during the Big Bang,
link |
01:08:41.720
not very long after the Big Bang,
link |
01:08:43.240
I think a few seconds after the Big Bang,
link |
01:08:45.040
you have this event called the Great Annihilation,
link |
01:08:47.280
which is where all the particles and antiparticles
link |
01:08:49.840
smack into each other, annihilate, turn into light mostly,
link |
01:08:53.520
and you end up with a universe later on.
link |
01:08:55.000
If that was what happened,
link |
01:08:55.960
then the universe we live in today would be black and empty,
link |
01:08:58.800
apart from some photons, that would be it.
link |
01:09:01.600
So there is stuff in the universe.
link |
01:09:03.560
It appears to be just made of matter.
link |
01:09:04.960
So there's this big mystery as to how did this happen?
link |
01:09:08.200
And there are various ideas,
link |
01:09:09.720
which all involve sort of physics going on
link |
01:09:13.520
in the first trillionth of a second or so of the Big Bang.
link |
01:09:17.040
So it could be that one possibility
link |
01:09:20.080
is that the Higgs field is somehow implicated in this,
link |
01:09:22.600
that there was this event that took place
link |
01:09:25.360
in the early universe where the Higgs field
link |
01:09:27.680
basically switched on, it acquired its modern value.
link |
01:09:31.400
And when that happened,
link |
01:09:33.480
this caused all the particles to acquire mass
link |
01:09:35.600
and the universe basically went through a phase transition
link |
01:09:37.880
where you had a hot plasma of massless particles.
link |
01:09:41.000
And then in that plasma,
link |
01:09:42.040
it's almost like a gas turning into droplets of water.
link |
01:09:44.760
You get kind of these little bubbles forming in the universe
link |
01:09:47.960
where the Higgs field has acquired its modern value,
link |
01:09:50.760
the particles have got mass.
link |
01:09:52.280
And this phase transition in some models
link |
01:09:55.200
can cause more matter than antimatter to be produced,
link |
01:09:57.960
depending on how matter bounces off these bubbles
link |
01:10:00.640
in the early universe.
link |
01:10:01.760
So that's one idea.
link |
01:10:02.760
There's other ideas to do with neutrinos,
link |
01:10:04.680
that there are exotic types of neutrinos
link |
01:10:06.360
that can decay in a biased way to just matter
link |
01:10:09.280
and not to antimatter.
link |
01:10:10.200
So, and people are trying to test these ideas.
link |
01:10:12.640
That's what we're trying to do at LHCb.
link |
01:10:14.280
There's neutrino experiments planned
link |
01:10:15.720
that are trying to do these sorts of things as well.
link |
01:10:17.560
So yeah, there are ideas, but at the moment,
link |
01:10:19.560
no clear evidence for which of these ideas might be right.
link |
01:10:22.920
So we're talking about some incredible ideas.
link |
01:10:25.520
By the way, never heard anyone be so eloquent
link |
01:10:28.320
about describing even just the standard model.
link |
01:10:31.680
So I'm in awe just listening.
link |
01:10:34.520
Oh, thank you.
link |
01:10:35.360
Yeah, just having fun enjoying it.
link |
01:10:38.080
So the, yes, the theoretical,
link |
01:10:40.280
the particle physics is fascinating here.
link |
01:10:42.520
To me, one of the most fascinating things
link |
01:10:44.680
about the Large Hadron Collider is the human side of it.
link |
01:10:47.880
That a bunch of sort of brilliant people
link |
01:10:51.520
that probably have egos got together
link |
01:10:54.360
and were collaborate together and countries,
link |
01:10:57.720
I guess, collaborate together for the funds
link |
01:11:00.000
and everything's just collaboration everywhere.
link |
01:11:03.000
Cause you may be, I don't know what the right question here
link |
01:11:07.440
to ask, but almost what's your intuition
link |
01:11:09.680
about how it was possible to make this happen
link |
01:11:11.840
and what are the lessons we should learn
link |
01:11:14.360
for the future of human civilization
link |
01:11:16.080
in terms of our scientific progress?
link |
01:11:17.840
Cause it seems like this is a great, great illustration
link |
01:11:21.600
of us working together to do something big.
link |
01:11:24.640
Yeah, I think it's possibly the best example.
link |
01:11:27.040
Maybe I can think of international collaboration
link |
01:11:30.280
that isn't for some unpleasant purpose, basically.
link |
01:11:33.400
You know, I mean, so when I started out in the field
link |
01:11:37.400
in 2008 as a new PhD student,
link |
01:11:39.720
the LHC was basically finished.
link |
01:11:41.480
So I didn't have to go around asking for money for it
link |
01:11:44.600
or trying to make the case.
link |
01:11:45.520
So I have huge admiration for the people who managed that.
link |
01:11:48.760
Cause this was a project that was first imagined
link |
01:11:51.160
in the 1970s, in the late 70s
link |
01:11:53.440
was when the first conversations about the LHC were mooted
link |
01:11:56.440
and it took two and a half decades of campaigning
link |
01:12:00.800
and fundraising and persuasion
link |
01:12:03.600
until they started breaking ground
link |
01:12:05.200
and building the thing in the early noughties in 2000.
link |
01:12:08.040
So, I mean, I think the reason just from a sort of,
link |
01:12:11.280
from the point of view of the sort of science,
link |
01:12:13.280
the scientists there,
link |
01:12:14.120
I think the reason it works ultimately
link |
01:12:16.680
is that everywhere, everyone there is there
link |
01:12:19.280
for the same reason, which is, well, in principle, at least
link |
01:12:23.680
they're there because they're interested in the world.
link |
01:12:25.520
They want to find out, you know,
link |
01:12:27.400
what are the basic ingredients of our universe?
link |
01:12:29.360
What are the laws of nature?
link |
01:12:31.040
And so everyone is pulling in the same direction.
link |
01:12:32.920
Now, of course, everyone has their own
link |
01:12:34.720
things they're interested in.
link |
01:12:35.680
Everyone has their own careers to consider.
link |
01:12:37.360
And, you know, I wouldn't pretend that
link |
01:12:38.800
there isn't also a lot of competition.
link |
01:12:40.760
So there's this funny thing in these experiments
link |
01:12:42.880
where your collaborators,
link |
01:12:43.960
your 800 collaborators in LHCb,
link |
01:12:46.120
but you're also competitors
link |
01:12:47.320
because your academics in your various universities
link |
01:12:49.920
and you want to be the one that gets the paper out
link |
01:12:51.520
on the most exciting, you know, new measurements.
link |
01:12:53.400
So there's this funny thing where you're kind of trying
link |
01:12:55.720
to stake out your territory while also collaborating
link |
01:12:58.440
and having to work together to make the experiments work.
link |
01:13:00.920
And it does work amazingly well,
link |
01:13:03.560
actually considering all of that.
link |
01:13:05.160
And I think there was actually,
link |
01:13:06.760
I think McKinsey or one of these big management
link |
01:13:08.680
consultancy firms went into CERN maybe a decade or so ago
link |
01:13:11.840
to try to understand how these organizations function.
link |
01:13:15.000
Did they figure it out?
link |
01:13:16.040
I don't think they could.
link |
01:13:16.960
I mean, I think one of the things that's interesting,
link |
01:13:18.800
one of the other interesting things
link |
01:13:19.800
about these experiments is, you know,
link |
01:13:21.080
they're big operations like say Atlas has 3000 people.
link |
01:13:24.960
Now there was a person nominally
link |
01:13:26.320
who was the head of Atlas, they're called the spokesperson.
link |
01:13:29.680
And the spokesperson is elected by,
link |
01:13:32.360
usually by the collaboration,
link |
01:13:34.240
but they have no actual power really.
link |
01:13:36.400
I mean, they can't fire anyone.
link |
01:13:38.560
They're not anyone's boss.
link |
01:13:39.720
So, you know, my boss is a professor at Cambridge,
link |
01:13:43.360
not the head of my experiments.
link |
01:13:45.120
The head of my experiment can't tell me what to do really.
link |
01:13:47.520
And there's all these independent academics
link |
01:13:50.200
who are their own bosses who, you know,
link |
01:13:52.400
so that somehow it, nonetheless,
link |
01:13:54.600
by kind of consensus and discussion and lots of meetings,
link |
01:13:58.520
these things do happen and it does get done, but.
link |
01:14:01.640
It's like the queen here in the UK is the spokesperson.
link |
01:14:04.960
I guess so.
link |
01:14:05.800
No actual power. Except we don't elect her, no.
link |
01:14:07.560
No, we don't elect her.
link |
01:14:08.880
But everybody seems to love her.
link |
01:14:10.480
I don't know, from my outside perspective.
link |
01:14:16.240
But yeah, giant egos, brilliant people.
link |
01:14:19.840
And moving forward, do you think there's.
link |
01:14:22.920
Actually, I would pick up one thing you said just there,
link |
01:14:24.800
just the brilliant people thing.
link |
01:14:25.840
Cause I'm not saying that people aren't great.
link |
01:14:28.240
But I think there is this sort of impression
link |
01:14:30.600
that physicists all have to be brilliant or geniuses,
link |
01:14:32.960
which is not true actually.
link |
01:14:34.160
And you know, you have to be relatively bright for sure.
link |
01:14:37.520
But you know, a lot of people,
link |
01:14:39.120
a lot of the most successful experimental physicists
link |
01:14:41.560
are not necessarily the people with the biggest brains.
link |
01:14:43.960
They're the people who, you know,
link |
01:14:45.680
particularly one of the skills that's most important
link |
01:14:47.440
in particle physics is the ability to work
link |
01:14:49.560
with others and to collaborate and exchange ideas
link |
01:14:51.320
and also to work hard.
link |
01:14:52.360
And it's a sort of, often it's more a determination
link |
01:14:55.520
or a sort of other set of skills.
link |
01:14:57.520
It's not just being, you know, kind of some great brain.
link |
01:15:01.440
Very true.
link |
01:15:02.280
So, I mean, there's parallels to that
link |
01:15:04.160
in the machine learning world.
link |
01:15:05.160
If you wanna solve any real world problems,
link |
01:15:08.200
which I see as the particle accelerators,
link |
01:15:11.200
essentially a real world instantiation
link |
01:15:14.920
of theoretical physics.
link |
01:15:16.720
And for that, you have to not necessarily be brilliant,
link |
01:15:20.280
but be sort of obsessed, systematic, rigorous,
link |
01:15:26.320
sort of unborable, stubborn, all those kind of qualities
link |
01:15:29.840
that make for a great engineer.
link |
01:15:31.160
So, scientists purely speaking,
link |
01:15:34.200
that practitioner of the scientific method.
link |
01:15:36.200
So you're right.
link |
01:15:37.400
But nevertheless, to me that's brilliant.
link |
01:15:39.800
My dad's a physicist.
link |
01:15:41.600
I argue with him all the time.
link |
01:15:43.040
To me, engineering is the highest form of science.
link |
01:15:46.000
And he thinks that's all nonsense,
link |
01:15:48.360
that the real work is done by the theoretician.
link |
01:15:50.640
So, in fact, we have arguments about like people
link |
01:15:54.320
like Elon Musk, for example,
link |
01:15:56.080
because I think his work is quite brilliant,
link |
01:15:58.640
but he's fundamentally not coming up
link |
01:16:00.520
with any serious breakthroughs.
link |
01:16:02.480
He's just creating in this world, implementing,
link |
01:16:07.080
like making ideas happen that have a huge impact.
link |
01:16:09.640
To me, that's the Edison.
link |
01:16:12.200
That to me is a brilliant work,
link |
01:16:17.400
but to him, it's messy details
link |
01:16:22.840
that somebody will figure out anyway.
link |
01:16:25.440
I mean, I don't know whether you think
link |
01:16:26.640
there is a actual difference in temperament
link |
01:16:29.000
between say a physicist and an engineer,
link |
01:16:31.160
whether it's just what you got interested in.
link |
01:16:33.000
I don't know.
link |
01:16:34.240
I mean, a lot of what experimental physicists do
link |
01:16:37.920
is to some extent engineering.
link |
01:16:40.040
I mean, it's not what I do.
link |
01:16:40.880
I mostly do data stuff,
link |
01:16:42.120
but a lot of people would be called electrical engineers,
link |
01:16:45.520
but they trained as physicists,
link |
01:16:46.960
but they learned electrical engineering, for example,
link |
01:16:48.880
because they were building detectors.
link |
01:16:50.960
So, there's not such a clear divide, I think.
link |
01:16:52.880
Yeah, it's interesting.
link |
01:16:53.720
I mean, but there does seem to be,
link |
01:16:55.600
like you work with data.
link |
01:16:57.120
There does seem to be a certain,
link |
01:16:59.920
like I love data collection.
link |
01:17:01.640
There might be an OCD element or something
link |
01:17:03.680
that you're more naturally predisposed to
link |
01:17:06.600
as opposed to theory.
link |
01:17:07.600
Like I'm not afraid of data.
link |
01:17:08.880
I love data.
link |
01:17:10.160
And there's a lot of people in machine learning
link |
01:17:11.680
who are more like,
link |
01:17:14.360
they're basically afraid of data collection,
link |
01:17:16.920
afraid of data sets, afraid of all of that.
link |
01:17:18.880
They just want to stay in more than theoretical
link |
01:17:20.720
and they're really good at it, space.
link |
01:17:22.800
So, I don't know if that's the genetic,
link |
01:17:24.040
that's your upbringing, the way you go to school,
link |
01:17:28.280
but looking into the future of LHC and other colliders.
link |
01:17:33.400
So, there's in America,
link |
01:17:35.320
there's whatever it was called, the super,
link |
01:17:37.520
there's a lot of super.
link |
01:17:38.360
Superconducting super colliders.
link |
01:17:39.840
Yeah, superconducting.
link |
01:17:40.840
The desertron, yeah.
link |
01:17:41.880
Desertron, yeah.
link |
01:17:43.000
So, that was canceled, the construction of that.
link |
01:17:45.880
Yeah.
link |
01:17:48.120
Which is a sad thing,
link |
01:17:50.880
but what do you think is the future of these efforts?
link |
01:17:54.160
Will a bigger collider be built?
link |
01:17:56.480
Will LHC be expanded?
link |
01:17:58.560
What do you think?
link |
01:17:59.920
Well, in the near future, the LHC is gonna get an upgrade.
link |
01:18:03.360
So, that's pretty much confirmed.
link |
01:18:04.840
I think it is confirmed, which is,
link |
01:18:07.160
it's not an energy upgrade.
link |
01:18:08.160
It's what we call a luminosity upgrade.
link |
01:18:10.200
So, it basically means increasing
link |
01:18:11.680
the data collection rates.
link |
01:18:13.400
So, more collisions per second, basically,
link |
01:18:15.920
because after a few years of data taking,
link |
01:18:18.160
you get this law of diminishing returns
link |
01:18:19.560
where each year's worth of data
link |
01:18:20.680
is a smaller and smaller fraction
link |
01:18:21.960
of the lot you've already got.
link |
01:18:23.440
So, to get a real improvement in sensitivity,
link |
01:18:25.840
you need to increase the data rate
link |
01:18:27.200
by an order of magnitude.
link |
01:18:28.280
So, that's what this upgrade is gonna do.
link |
01:18:30.520
LHCb, at the moment, the whole detector
link |
01:18:32.680
is basically being rebuilt to allow it to record data
link |
01:18:36.240
at a much larger rate than we could before.
link |
01:18:38.000
So, that will make us sensitive
link |
01:18:39.240
to whole loads of new processes
link |
01:18:40.680
that we weren't able to study before.
link |
01:18:42.200
And I mentioned briefly these anomalies that we've seen.
link |
01:18:45.760
So, we've seen a bunch of very intriguing anomalies
link |
01:18:49.040
in these b quark decays,
link |
01:18:52.320
which may be hinting at the first signs
link |
01:18:55.480
of this kind of the elephant,
link |
01:18:57.360
the signs of some new quantum field
link |
01:18:59.640
or fields maybe beyond the standard model.
link |
01:19:01.200
It's not yet at the statistical threshold
link |
01:19:02.920
where you can say that you've observed something,
link |
01:19:06.200
but there's lots of anomalies in many measurements
link |
01:19:08.840
that all seem to be consistent with each other.
link |
01:19:11.040
So, it's quite interesting.
link |
01:19:12.000
So, the upgrade will allow us
link |
01:19:13.600
to really home in on these things
link |
01:19:15.840
and see whether these anomalies are real,
link |
01:19:17.360
because if they are real,
link |
01:19:19.480
and this kind of connects to your point
link |
01:19:20.880
about the next generation of machines,
link |
01:19:23.720
what we would have seen then is,
link |
01:19:26.320
we would have seen the tail end of some quantum field
link |
01:19:29.240
in influencing these b quarks.
link |
01:19:31.800
What we then need to do is to build a bigger collider
link |
01:19:34.520
to actually make the particle of that field.
link |
01:19:37.480
So, if these things really do exist.
link |
01:19:40.240
So, that would be one argument.
link |
01:19:41.280
I mean, so at the moment,
link |
01:19:42.360
Europe is going through this process
link |
01:19:44.000
of thinking about the strategy for the future.
link |
01:19:47.800
So, there are a number of different proposals on the table.
link |
01:19:49.720
One is for a sort of higher energy upgrade of the LHC,
link |
01:19:53.600
where you just build more powerful magnets
link |
01:19:55.280
and put them in the same tunnel.
link |
01:19:56.200
That's a sort of cheaper, less ambitious possibility.
link |
01:19:59.680
Most people don't really like it
link |
01:20:00.840
because it's sort of a bit of a dead end,
link |
01:20:02.560
because once you've done that, there's nowhere to go.
link |
01:20:05.560
There's a machine called Click,
link |
01:20:06.840
which is a compact linear collider,
link |
01:20:08.960
which is a electron positron collider
link |
01:20:10.720
that uses a novel type of acceleration technology
link |
01:20:13.440
to accelerate at shorter distances.
link |
01:20:15.520
We're still talking kilometers long,
link |
01:20:17.000
but not like 100 kilometers long.
link |
01:20:19.880
And then probably the project that is,
link |
01:20:22.480
I think getting the most support,
link |
01:20:23.920
it'd be interesting to see what happens,
link |
01:20:25.400
something called the Future Circular Collider,
link |
01:20:28.040
which is a really ambitious longterm multi decade project
link |
01:20:32.040
to build a 100 kilometer circumference tunnel
link |
01:20:35.960
under the Geneva region.
link |
01:20:38.160
The LHC would become a kind of feeding machine.
link |
01:20:40.720
It would just feed.
link |
01:20:41.560
So the same area, so it would be a feeder for the.
link |
01:20:44.080
Yeah.
link |
01:20:44.920
So it would kind of, the edge of this machine
link |
01:20:46.400
would be where the LHC is,
link |
01:20:47.640
but it would sort of go under Lake Geneva
link |
01:20:49.120
and round to the Alps, basically,
link |
01:20:51.560
up to the edge of the Geneva basin.
link |
01:20:52.920
So it's basically the biggest tunnel you can fit
link |
01:20:55.560
in the region based on the geology.
link |
01:20:57.240
100 kilometers.
link |
01:20:58.080
Yeah, so it's big.
link |
01:20:58.920
It'd be a long drive if your experiment's on one side.
link |
01:21:01.880
You've got to go back to CERN for lunch,
link |
01:21:03.080
so that would be a pain.
link |
01:21:04.280
But you know, so this project is,
link |
01:21:07.600
in principle, it's actually two accelerators.
link |
01:21:09.120
The first thing you would do
link |
01:21:09.960
is put an electron positron machine
link |
01:21:11.720
in the 100 kilometer tunnel to study the Higgs.
link |
01:21:14.360
So you'd make lots of Higgs bows
link |
01:21:15.440
and study it really precisely
link |
01:21:16.960
in the hope that you see it misbehaving
link |
01:21:18.600
and doing something it's not supposed to.
link |
01:21:20.480
And then in the much longer term,
link |
01:21:22.880
100, that machine gets taken out,
link |
01:21:24.840
you put in a proton proton machine.
link |
01:21:26.520
So it's like the LHC, but much bigger.
link |
01:21:29.040
And that's the way you start going
link |
01:21:30.440
and looking for dark matter,
link |
01:21:32.400
or you're trying to recreate this phase transition
link |
01:21:35.960
that I talked about in the early universe,
link |
01:21:37.120
where you can see matter anti matter being made,
link |
01:21:39.360
for example.
link |
01:21:40.200
There's lots of things you can do with these machines.
link |
01:21:41.080
The problem is that they will take,
link |
01:21:43.560
you know, the most optimistic,
link |
01:21:45.440
you're not gonna have any data
link |
01:21:46.720
from any of these machines until 2040,
link |
01:21:49.080
or, you know, because they take such a long time to build
link |
01:21:51.840
and they're so expensive.
link |
01:21:52.920
So you have, there'll be a process of R&D design,
link |
01:21:55.960
but also the political case being made.
link |
01:21:57.960
So LHC, what costs a few billion?
link |
01:22:01.280
Depends how you count it.
link |
01:22:03.200
I think most of the sort of more reasonable estimates
link |
01:22:05.440
that take everything into account properly,
link |
01:22:07.000
it's around the sort of 10, 11, 12 billion euro mark.
link |
01:22:10.400
What would be the future, sorry,
link |
01:22:12.400
I forgot the name already.
link |
01:22:13.240
Future Circular Collider.
link |
01:22:14.720
Future Circular Collider.
link |
01:22:15.560
Presumably they won't call it that when it's built,
link |
01:22:16.920
cause it won't be the future anymore.
link |
01:22:18.280
But I don't know, I don't know what they'll call it then.
link |
01:22:20.680
The very big Hadron Collider, I don't know.
link |
01:22:25.120
But that will, now I should know the numbers,
link |
01:22:28.840
but I think the whole project is estimated
link |
01:22:31.160
at about 30 billion euros,
link |
01:22:32.880
but that's money spent over between now and 2070 probably,
link |
01:22:37.840
which is when the last bit of it
link |
01:22:39.840
would be sort of finishing up, I guess.
link |
01:22:42.360
So you're talking a half a century of science
link |
01:22:46.560
coming out of this thing, shared by many countries.
link |
01:22:48.720
So the actual cost, the arguments that are made
link |
01:22:51.200
is that you could make this project fit
link |
01:22:53.120
within the existing budget of CERN,
link |
01:22:56.160
if you didn't do anything else.
link |
01:22:57.480
And CERN, by the way, we didn't mention, what is CERN?
link |
01:23:00.520
CERN is the European Organization for Nuclear Research.
link |
01:23:03.280
It's an international organization
link |
01:23:05.240
that was established in the 1950s
link |
01:23:07.080
in the wake of the second world war as a kind of,
link |
01:23:10.280
it was sort of like a scientific Marshall plan for Europe.
link |
01:23:12.520
The idea was that you bring European science back together
link |
01:23:16.080
for peaceful purposes,
link |
01:23:17.320
because what happened in the forties was,
link |
01:23:20.000
a lot of particular Jewish scientists,
link |
01:23:21.280
but a lot of scientists from central Europe
link |
01:23:22.640
had fled to the United States
link |
01:23:25.000
and Europe had sort of seen this brain drain.
link |
01:23:27.240
So there was a desire to bring the community back together
link |
01:23:29.920
for a project that wasn't building nasty bombs,
link |
01:23:32.280
but was doing something that was curiosity driven.
link |
01:23:34.280
So, and that has continued since then.
link |
01:23:37.320
So it's kind of a unique organization.
link |
01:23:38.840
It's you, to be a member as a country,
link |
01:23:41.480
you sort of sign up as a member
link |
01:23:43.040
and then you have to pay a fraction of your GDP
link |
01:23:45.960
each year as a subscription.
link |
01:23:47.360
I mean, it's a very small fraction, relatively speaking.
link |
01:23:49.520
I think it's like, I think the UK's contribution
link |
01:23:51.480
is a hundred or 200 million quid or something like that.
link |
01:23:54.840
Yeah, which is quite a lot, but not so.
link |
01:23:57.480
That's fascinating.
link |
01:23:58.400
I mean, just the whole thing that is possible,
link |
01:24:00.040
it's beautiful.
link |
01:24:01.240
It's a beautiful idea,
link |
01:24:02.240
especially when there's no wars on the line,
link |
01:24:05.320
it's not like we're freaking out,
link |
01:24:06.560
as we're actually legitimately collaborating
link |
01:24:08.880
to do good science.
link |
01:24:09.880
One of the things I don't think we really mentioned
link |
01:24:11.880
is on the final side, that sort of the data analysis side,
link |
01:24:15.360
is there breakthroughs possible there
link |
01:24:17.080
and the machine learning side,
link |
01:24:18.160
like is there a lot more signal to be mined
link |
01:24:22.680
in more effective ways from the actual raw data?
link |
01:24:25.400
Yeah, a lot of people are looking into that.
link |
01:24:27.680
I mean, so I use machine learning in my data analysis,
link |
01:24:31.600
but pretty naughty, basic stuff,
link |
01:24:33.840
cause I'm not a machine learning expert.
link |
01:24:35.440
I'm just a physicist who had to learn to do this stuff
link |
01:24:37.960
for my day job.
link |
01:24:38.800
So what a lot of people do is they use
link |
01:24:40.600
kind of off the shelf packages
link |
01:24:42.560
that you can train to do signal noise.
link |
01:24:46.240
Just clean up all the data.
link |
01:24:48.280
But one of the big challenges,
link |
01:24:50.040
the big challenge of the data is A, it's volume,
link |
01:24:52.720
there's huge amounts of data.
link |
01:24:53.880
So the LHC generates, now, okay,
link |
01:24:56.480
I try to remember what the actual numbers are,
link |
01:24:57.920
but if you, we don't record all our data,
link |
01:24:59.440
we record a tiny fraction of the data.
link |
01:25:02.240
It's like of order one 10,000th or something, I think.
link |
01:25:04.920
Is that right?
link |
01:25:05.880
Around that.
link |
01:25:07.040
So most of it gets thrown away.
link |
01:25:08.600
You couldn't record all the LHC data
link |
01:25:10.080
cause it would fill up every computer in the world
link |
01:25:11.480
in a matter of days, basically.
link |
01:25:13.680
So there's this process that happens on live,
link |
01:25:17.000
on the detector, something called a trigger,
link |
01:25:18.880
which in real time, 40 million times every second
link |
01:25:21.360
has to make a decision about whether this collision
link |
01:25:23.680
is likely to contain an interesting object,
link |
01:25:26.400
like a Higgs boson or a dark matter particle.
link |
01:25:28.560
And it has to do that very fast.
link |
01:25:29.760
And the software algorithms in the past
link |
01:25:33.240
were quite relatively basic.
link |
01:25:36.040
They did things like measure mementos
link |
01:25:37.840
and energies of particles and put some requirements.
link |
01:25:40.320
So you would say, if there's a particle
link |
01:25:42.200
with an energy above some threshold,
link |
01:25:43.640
then record this collision.
link |
01:25:44.840
But if there isn't, don't.
link |
01:25:46.240
Whereas now the attempt is get more and more
link |
01:25:47.960
machine learning in at the earliest possible stage.
link |
01:25:51.080
That's cool, at the stage of deciding
link |
01:25:53.160
whether we want to keep this data or not.
link |
01:25:55.280
But also maybe even lower down than that,
link |
01:25:57.640
which is the point where there's this,
link |
01:26:01.160
so generally how the data is reconstructed
link |
01:26:02.800
is you start off with a set of digital hits
link |
01:26:06.280
in your detector.
link |
01:26:07.120
So channels saying, did you see something?
link |
01:26:08.840
Did you not see something?
link |
01:26:10.120
That has to be then turned into tracks,
link |
01:26:12.560
particles going in different directions.
link |
01:26:14.040
And that's done by using fits
link |
01:26:15.520
that fit through the data points.
link |
01:26:17.200
And then that's passed to the algorithms
link |
01:26:18.640
that then go, is this interesting or not?
link |
01:26:20.520
What'd be better is you could train machine learning
link |
01:26:22.520
to just look at the raw hits,
link |
01:26:24.120
the basic real base level information,
link |
01:26:26.360
not have any of the reconstruction done.
link |
01:26:28.440
And it just goes, and it can learn to do pattern recognition
link |
01:26:31.040
on this strange three dimensional image that you get.
link |
01:26:34.240
And potentially that's where you could get really big gains
link |
01:26:36.800
because our triggers tend to be quite inefficient
link |
01:26:38.760
because they don't have time to do
link |
01:26:41.880
the full whiz bang processing
link |
01:26:43.360
to get all the information out that we would like,
link |
01:26:45.400
because you have to do the decision very quickly.
link |
01:26:46.760
So if you can come up with some clever
link |
01:26:48.760
machine learning technique,
link |
01:26:50.080
then potentially you can massively increase
link |
01:26:52.000
the amount of useful data you record
link |
01:26:54.960
and get rid of more of the background
link |
01:26:58.400
earlier in the process.
link |
01:26:59.800
Yeah, to me, that's an exciting possibility
link |
01:27:01.440
because then you don't have to build a sort of,
link |
01:27:04.880
you can get a gain without having to.
link |
01:27:08.640
Without having to build any hardware, I suppose.
link |
01:27:10.360
Hardware, yeah.
link |
01:27:11.200
Although you need lots of new GPU farms, I guess.
link |
01:27:13.960
So hardware still helps.
link |
01:27:15.280
But I got to talk to you,
link |
01:27:20.280
sort of I'm not sure how to ask,
link |
01:27:22.840
but you're clearly an incredible science communicator.
link |
01:27:27.480
I don't know if that's the right term,
link |
01:27:29.560
but you're basically a younger Neil deGrasse Tyson
link |
01:27:32.520
with a British accent.
link |
01:27:33.680
So, and you've, I mean,
link |
01:27:36.480
can you say where we are today, actually?
link |
01:27:39.160
Yeah, so today we're in the Royal Institution in London,
link |
01:27:42.560
which is a very old organization.
link |
01:27:45.880
It's been around for about 200 years now, I think.
link |
01:27:47.760
Maybe even I should know when it was founded.
link |
01:27:49.800
Sort of early 19th century,
link |
01:27:51.440
it was set up to basically communicate science to the public.
link |
01:27:55.880
So it was one of the first places in the world
link |
01:27:57.560
where famous scientists would come and give talks.
link |
01:28:01.240
So very famously Humphrey Davy, who you may know of,
link |
01:28:05.440
who was the person who discovered nitrous oxide.
link |
01:28:07.560
He was a very famous chemist and scientist.
link |
01:28:11.200
Also discovered electrolysis.
link |
01:28:12.720
So he used to do these fantastic,
link |
01:28:13.920
he was a very charismatic speaker.
link |
01:28:15.040
So he used to appear here.
link |
01:28:15.880
There's a big desk that they usually have in the theater
link |
01:28:18.440
and he would do demonstrations to the sort of the,
link |
01:28:21.160
the folk of London back in the early 19th century.
link |
01:28:23.760
And Michael Faraday, who I talked about,
link |
01:28:25.200
who is the person who did so much work on electromagnetism,
link |
01:28:27.280
he used, he lectured here.
link |
01:28:28.400
He also did experiments in the basement.
link |
01:28:29.880
So this place has got a long history
link |
01:28:31.240
of both scientific research,
link |
01:28:33.320
but also communication of scientific research.
link |
01:28:35.800
So you gave a few lectures here.
link |
01:28:38.040
How many, two?
link |
01:28:39.320
I've given, yeah, I've given a couple of lectures
link |
01:28:41.080
in this theater before, so.
link |
01:28:42.280
I mean, that's, so people should definitely go watch online.
link |
01:28:46.000
It's just the explanation of particle physics.
link |
01:28:48.640
So all the, I mean, it's incredible.
link |
01:28:50.480
Like your lectures are just incredible.
link |
01:28:53.360
I can't sing it enough praise.
link |
01:28:54.520
So it was awesome.
link |
01:28:55.480
But maybe can you say, what did that feel like?
link |
01:29:00.280
What does it feel like to lecture here, to talk about that?
link |
01:29:03.600
And maybe from a different perspective,
link |
01:29:06.440
more kind of like how the sausage is made is,
link |
01:29:09.360
how do you prepare for that kind of thing?
link |
01:29:12.120
How do you think about communication,
link |
01:29:14.320
the process of communicating these ideas
link |
01:29:16.440
in a way that's inspiring to,
link |
01:29:18.480
what I would say your talks are inspiring
link |
01:29:21.200
to like the general audience.
link |
01:29:22.560
You don't actually have to be a scientist.
link |
01:29:25.080
You can still be inspired without really knowing much of the,
link |
01:29:28.040
you start from the very basics.
link |
01:29:30.720
So what's the preparation process?
link |
01:29:33.320
And then the romantic question is,
link |
01:29:34.800
what did that feel like to perform here?
link |
01:29:38.000
I mean, profession, yeah.
link |
01:29:39.600
I mean, the process, I mean, the talk,
link |
01:29:42.200
my favorite talk that I gave here
link |
01:29:43.280
was one called Beyond the Higgs,
link |
01:29:44.520
which you can find on the Royal Institute's YouTube channel,
link |
01:29:46.800
which you should go and check out.
link |
01:29:48.280
I mean, and their channel's got loads of great talks
link |
01:29:50.000
with loads of great people as well.
link |
01:29:52.760
I mean, that one, I'd sort of given a version of it
link |
01:29:55.160
many times, so part of it is just practice, right?
link |
01:29:57.360
And actually, I don't have some great theory
link |
01:29:59.000
of how to communicate with people.
link |
01:30:00.360
It's more just that I'm really interested
link |
01:30:02.640
and excited by those ideas and I like talking about them.
link |
01:30:05.240
And through the process of doing that,
link |
01:30:07.280
I guess I figured out stories that work
link |
01:30:09.640
and explanations that work.
link |
01:30:10.840
When you say practice, you mean legitimately
link |
01:30:12.920
just giving talks? Just giving talks, yeah.
link |
01:30:14.960
I started off when I was a PhD student
link |
01:30:17.240
doing talks in schools and I still do that as well
link |
01:30:20.040
some of the time and doing things,
link |
01:30:21.760
I've even done a bit of standup comedy,
link |
01:30:23.200
which sort of went reasonably well,
link |
01:30:25.240
even if it was terrifying.
link |
01:30:26.280
And that's on YouTube as well.
link |
01:30:27.480
That's also on, I wouldn't necessarily recommend
link |
01:30:29.240
you check that out.
link |
01:30:30.080
I'm gonna post the links several places
link |
01:30:33.200
to make sure people click on it.
link |
01:30:35.400
But it's basically, I kind of have a story in my head
link |
01:30:37.760
and I kind of, I have to think about what I wanna say.
link |
01:30:41.720
I usually have some images to support what I'm saying
link |
01:30:43.480
and I get up and do it.
link |
01:30:44.440
And it's not really, I wish there was some kind of,
link |
01:30:47.200
I probably should have some proper process.
link |
01:30:48.640
This is very sounds like I'm just making up as I go along
link |
01:30:50.640
and I sort of am.
link |
01:30:52.200
Well, I think the fundamental thing that you said,
link |
01:30:54.240
I think it's like, I don't know if you know
link |
01:30:58.320
who a guy named Joe Rogan is.
link |
01:31:01.120
Yes, I do.
link |
01:31:02.200
So he's also kind of sounds like you in a sense
link |
01:31:05.040
that he's not very introspective about his process,
link |
01:31:08.560
but he's an incredibly engaging conversationalist.
link |
01:31:13.040
And I think one of the things that you and him share
link |
01:31:15.800
that I could see is like a genuine curiosity
link |
01:31:19.920
and passion for the topic.
link |
01:31:22.320
I think that could be systematically cultivated.
link |
01:31:26.840
I'm sure there's a process to it,
link |
01:31:28.200
but you come to it naturally somehow.
link |
01:31:30.520
I think maybe there's something else as well,
link |
01:31:31.920
which is to understand something.
link |
01:31:34.240
There's this quote by Feynman, which I really like,
link |
01:31:35.920
which is what I cannot create, I do not understand.
link |
01:31:38.240
So I'm not particularly super bright.
link |
01:31:43.200
So for me to understand something,
link |
01:31:44.680
I have to break it down into its simplest elements.
link |
01:31:47.240
And if I can then tell people about that,
link |
01:31:49.800
that helps me understand it as well.
link |
01:31:51.120
So I've learned to understand physics a lot more
link |
01:31:55.480
from the process of communicating,
link |
01:31:57.120
because it forces you to really scrutinize the ideas
link |
01:32:00.640
that you're communicating and it often makes you realize
link |
01:32:02.600
you don't really understand the ideas you're talking about.
link |
01:32:06.000
And I'm writing a book at the moment,
link |
01:32:08.120
and I had this experience yesterday where I realized
link |
01:32:09.960
I didn't really understand a pretty fundamental
link |
01:32:12.600
theoretical aspect of my own subject.
link |
01:32:14.480
And I had to go and I had to sort of spend
link |
01:32:15.960
a couple of days reading textbooks and thinking about it
link |
01:32:18.840
in order to make sure that the explanation I gave
link |
01:32:21.760
captured the, got as close to what is actually happening
link |
01:32:24.800
in the theory.
link |
01:32:26.040
And to do that, you have to really understand it properly.
link |
01:32:29.040
Yeah, and there's layers to understanding.
link |
01:32:31.040
It seems like the more,
link |
01:32:33.720
there must be some kind of Feynman law.
link |
01:32:35.920
I mean, the more you understand sort of the simpler
link |
01:32:39.680
you're able to really convey the essence of the idea, right?
link |
01:32:46.080
So it's like this reverse effect that it's like
link |
01:32:52.480
the more you understand, the simpler the final thing
link |
01:32:54.880
that you actually convey.
link |
01:32:56.280
And so the more accessible somehow it becomes.
link |
01:32:58.800
That's why Feynman's lectures are really accessible.
link |
01:33:03.200
It was just counterintuitive.
link |
01:33:04.880
Yeah, although there are some ideas
link |
01:33:06.720
that are very difficult to explain
link |
01:33:09.400
no matter how well or badly you understand them.
link |
01:33:12.240
Like I still can't really properly explain
link |
01:33:15.280
the Higgs mechanism.
link |
01:33:16.440
Yeah.
link |
01:33:17.400
Because some of these ideas only exist
link |
01:33:19.120
in mathematics really.
link |
01:33:21.680
And the only way to really develop an understanding
link |
01:33:24.320
is to go unfortunately to a graduate degree in physics.
link |
01:33:29.080
But you can get kind of a flavor of what's happening,
link |
01:33:31.880
I think, and it's trying to do that in a way
link |
01:33:33.520
that isn't misleading, but always also intelligible.
link |
01:33:36.840
So let me ask them the romantic question of
link |
01:33:39.760
what to you is the most, perhaps an unfair question,
link |
01:33:44.480
what is the most beautiful idea in physics?
link |
01:33:49.000
One that fills you with awe is the most surprising,
link |
01:33:52.680
the strangest, the weirdest.
link |
01:33:54.760
There's a lot of different definitions of beauty.
link |
01:33:57.600
And I'm sure there's several for you,
link |
01:33:59.320
but is there something that just jumps to mind
link |
01:34:01.080
that you think is just especially beautiful?
link |
01:34:07.080
There's a specific thing and a more general thing.
link |
01:34:08.760
So maybe the specific thing first,
link |
01:34:10.040
which I can now first came across as an undergraduate.
link |
01:34:12.400
I found this amazing.
link |
01:34:13.440
So this idea that the forces of nature,
link |
01:34:17.120
electromagnetism, strong force, the weak force,
link |
01:34:19.960
they arise in our theories as a consequence of symmetries.
link |
01:34:24.720
So symmetries in the laws of nature,
link |
01:34:27.480
in the equations essentially
link |
01:34:29.000
that used to describe these ideas,
link |
01:34:32.080
the process whereby theories come up
link |
01:34:34.440
with these sorts of models is they say,
link |
01:34:36.600
imagine the universe obeys this particular type of symmetry.
link |
01:34:39.920
It's a symmetry that isn't so far removed
link |
01:34:42.240
from a geometrical symmetry, like the rotations of a cube.
link |
01:34:44.880
It's not, you can't think of it quite that way,
link |
01:34:46.360
but it's sort of a similar sort of idea.
link |
01:34:49.040
And you say, okay, if the universe respects the symmetry,
link |
01:34:51.880
you find that you have to introduce a force
link |
01:34:54.720
which has the properties of electromagnetism
link |
01:34:57.960
or a different symmetry, you get the strong force
link |
01:35:00.080
or a different symmetry, you get the weak force.
link |
01:35:01.800
So these interactions seem to come from some deeper,
link |
01:35:05.160
it suggests that they come
link |
01:35:06.280
from some deeper symmetry principle.
link |
01:35:07.960
I mean, it depends a bit how you look at it
link |
01:35:09.680
because it could be that we're actually
link |
01:35:10.720
just recognizing symmetries in the things that we see,
link |
01:35:12.800
but there's something rather lovely about that.
link |
01:35:15.160
But I mean, I suppose a bigger thing that makes me wonder
link |
01:35:17.080
is actually, if you look at the laws of nature,
link |
01:35:20.200
how particles interact when you get really close down,
link |
01:35:22.680
they're basically pretty simple things.
link |
01:35:24.240
They bounce off each other by exchanging
link |
01:35:26.360
through force fields and they move around
link |
01:35:27.840
in very simple ways.
link |
01:35:29.280
And somehow these basic ingredients,
link |
01:35:31.880
these few particles that we know about in the forces
link |
01:35:34.560
creates this universe, which is unbelievably complicated
link |
01:35:37.360
and has things like you and me in it,
link |
01:35:39.520
and the earth and stars that make matter in their cores
link |
01:35:43.400
from the gravitational energy of their own bulk
link |
01:35:46.160
that then gets sprayed into the universe
link |
01:35:47.600
that forms other things.
link |
01:35:48.480
I mean, the fact that there's this incredibly long story
link |
01:35:52.880
that goes right back to the beginning,
link |
01:35:55.920
and we can take this story right back to a trillionth
link |
01:35:58.240
of a second after the Big Bang,
link |
01:35:59.440
and we can trace the origins of the stuff
link |
01:36:01.280
that we're made from.
link |
01:36:02.440
And it all ultimately comes from these simple ingredients
link |
01:36:05.040
with these simple rules.
link |
01:36:06.560
And the fact you can generate such complexity from that
link |
01:36:08.720
is really mysterious, I think, and strange.
link |
01:36:11.080
And it's not even a question that physicists
link |
01:36:12.920
can really tackle because we are sort of trying
link |
01:36:15.760
to find these really elementary laws.
link |
01:36:19.080
But it turns out that going from elementary laws
link |
01:36:21.880
and a few particles to something even as complicated
link |
01:36:24.040
as a molecule becomes very difficult.
link |
01:36:26.600
So going from a molecule to a human being
link |
01:36:28.640
is a problem that just can't be tackled,
link |
01:36:31.960
at least not at the moment, so.
link |
01:36:34.040
Yeah, the emergence of complexity from simple rules
link |
01:36:37.320
is so beautiful and so mysterious.
link |
01:36:40.600
And we don't have good mathematics
link |
01:36:43.600
to even try to approach that emergent phenomena.
link |
01:36:47.320
That's why we have chemistry and biology
link |
01:36:48.800
and all the other subjects, yeah, okay.
link |
01:36:52.040
I don't think there's a better way to end it, Harry.
link |
01:36:55.880
I can't, I mean, I think I speak for a lot of people
link |
01:36:59.040
that can't wait to see what happens
link |
01:37:01.880
in the next five, 10, 20 years with you.
link |
01:37:03.800
I think you're one of the great communicators of our time.
link |
01:37:06.080
So I hope you continue that and I hope that grows.
link |
01:37:09.840
And I'm definitely a huge fan.
link |
01:37:12.280
So it was an honor to talk to you today.
link |
01:37:13.960
Thanks so much, man.
link |
01:37:14.800
It was really fun, thanks very much.
link |
01:37:16.360
Thanks for listening to this conversation with Harry Kliff.
link |
01:37:19.040
And thank you to our sponsors, ExpressVPN
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01:37:22.000
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link |
01:37:23.240
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link |
01:37:25.000
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01:37:34.160
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01:37:36.760
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01:37:39.240
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link |
01:37:41.880
on Twitter at lexfreedman.
link |
01:37:45.440
And now let me leave you with some words from Harry Kliff.
link |
01:37:48.520
You and I are leftovers.
link |
01:37:51.160
Every particle in our bodies is a survivor
link |
01:37:53.760
from an almighty shootout between matter and antimatter
link |
01:37:57.080
that happened a little after the Big Bang.
link |
01:37:59.360
In fact, only one in a billion particles created
link |
01:38:02.760
at the beginning of time have survived to the present day.
link |
01:38:06.080
Thank you for listening and hope to see you next time.