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The following is a conversation with Harry Cliffe, a particle physicist at the University of Cambridge working on the Large Hadron Collider beauty experiment that specializes in investigating the slight differences between matter and antimatter by studying a type of particle called the beauty quark, or because in this way he's part of the group of physicists who are searching for the evidence of new particles that can answer some of the biggest questions in modern physics. He's also an exceptional communicator of science with some of the clearest and most captivating explanations of basic concepts in particle physicist that have ever heard.

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So when I visited London, I knew I had to talk to him and we did this conversation at the Royal Institute Lecture Theatre, which has hosted lectures for over two centuries from some of the greatest scientists and science communicators in history for Michael Faraday to Carl Sagan. This conversation was recorded before the outbreak of the pandemic for everyone feeling the medical and psychological and financial burden of this crisis. I'm sending love your way. Stay strong. We're in this together.

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We'll beat this thing. This is the artificial intelligence podcast. If you enjoy it, subscribe. I need to review it with five stars, an app, a podcast, supporter and patron, or simply connect with me on Twitter. Àlex Friedman spelled F.R. Idi Amin as usual.

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And now here's my conversation with Harry Cliff. Let's start with probably one of the coolest things that human beings have ever created, the Large Hadron Collider LHC, what is it? How does it work? OK, so essentially this gigantic 27 kilometer circumference particle accelerators, this big ring buried under 100 meters underneath the surface in the countryside, just outside Geneva in Switzerland. And really what it's for ultimately is to try to understand what are the basic building blocks of the universe.

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So you can think of it in a way as like a gigantic microscope. And the analogy is actually fairly precise. So gigantic microscope effectively, except as a microscope that looks at the structure of the vacuum in order for this kind of thing to study particles which are microscopic entities, it has to be huge, gigantic microscope.

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So what do you mean by studying vacuum?

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Okay, so I mean, it's a particle physics as as a field is kind of badly named in a way, because particles are not the fundamental ingredients of the universe. They're not fundamental at all. So the things that we believe are the real building blocks of the universe are objects, invisible fluid like objects called quantum fields. So these are fields like like the magnetic field around a magnet that exists everywhere in space that always there. In fact, actually, it's funny that we're in the wrong institution because this is where the idea of the field was effectively invented by Michael Faraday doing experiments with magnets and coils of wire.

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So he noticed that, you know, if it's a very famous experiment that he did where he got a magnet and put it on top of it, a piece of paper, and then sprinkled iron filings and he found the iron filings arranged themselves into these kind of loops, which was actually mapping out the invisible influence of this magnetic field, which is the thing, you know, we've all experienced we've all felt held a magnet and or two poles, the magnet put them together and felt this thing was force pushing back.

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So these are real physical objects. And the way we think of particles in modern physics is that they are essentially little vibrations, little ripples in these otherwise invisible fields that are everywhere.

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They fill the whole universe. You know, I don't apologise perhaps for the ridiculous question. Are you comfortable with the idea of the fundamental nature of our reality being fields'? Because to me, particles, you know, a bunch of different building blocks makes more sense, sort of intellectually, sort of visually, like it seems to I seem to be able to visualize the kind of idea easier. Yeah.

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Are you comfortable psychologically with the idea 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. I find it quite appealing. And it's well, it comes from a misunderstanding of what particles are so like when you when we do science at school and we draw a picture of an atom, you draw like, you know, a nucleus with some protons and neutrons, these little spheres in the middle. And then you have some electrons that are like little flies flying around the atom. And that is completely misleading.

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Picture of what an atom is like is nothing like the electron is not like a little planet orbiting the atom. It's this spread out wibbly wobbly, wavelike thing. And we know we've known that since, you know, the early 20th century thanks to quantum mechanics. So when we carry on using this word particle, because sometimes we do experiments, particles do behave like their little marbles or little bullets, you know, so the LHC, when we collide particles together, you'll get you know, you get like hundreds of particles all flying out through the detector and they all take a trajectory.

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And you can see from the detector where they've gone and they look like their little bullet.

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So they behave that way, you know, a lot of the time. But when you really study them carefully, you'll see that they are not little spheres. They are these ethereal disturbances in in these underlying fields. So this is this is really how we think nature is, which is surprising, but also, I think, kind of magic. So we are our bodies are basically made up of like little knots of energy in these invisible objects all around us.

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And what is the story of the vacuum when it comes to the LHC? So why did you mention the word vacuum?

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Okay, so if we just if we go back to the physics, we do know. So atoms are made of electrons, which were discovered 100 or so years ago. And then in the nucleus of the atom, you have two other types of particles. There's an up something called an up clock and a down quark. And those three particles make up every atom in the universe.

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So we think of these as ripples in field. So there is something called the electron field. And every electron in the universe is a ripple moving about in this electron field. So the electron field is all around us. We can't see it. But every electron in our body is a little ripple in this thing that's there all the time and the quark feels the same. So there's an up quark field and an up quark is literally up quark field and the down quark is a little.

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In something else called the down quark field, so these fields are always there. Now, there are potentially we know about a certain number of fields in what we call the standard model of particle physics. The most recent one we discovered was the Higgs field. And the way we discovered the Higgs field was to make a little ripple in it. So what the LHC did, it fired two protons into each other very, very hard with enough energy 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. So this particle that everyone's going on about eight or so years ago is proof. Really the particle in itself is I mean, it's interesting. But the thing is really interesting is the field, because it's the Higgs field that we believe is the reason that electrons and quarks have mass and it's that invisible field that's always there that gives mass to the particles.

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The Higgs boson is just our way of checking. It's there basically.

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And so the Large Hadron Collider, in order to get that ripple in the Higgs field, you know, it requires a huge amount of energy. Yes. So that's why this huge that's why size matters here. So maybe there's a million questions here. But let's backtrack. Why does size matter in the context of a heck of particle collider? So why does bigger allow you for higher energy collisions?

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Right. So the reason, well, is kind of simple, really, which is that there are two types of particle accelerator that you can build. One is circular, which is like the LHC. The other is a great long line. So the advantage of a circular machine is that you can send particles around a ring and you can give them a kick every time they go round. So imagine you have a is actually a bit of the LHC that's about only 30 metres long, where you have a bunch of metal boxes which have oscillating two million volt electric fields inside them, which are timed so that when a proton goes through one of these boxes, the field it sees as it approaches is attractive.

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Then as it leaves the box, it flips and becomes repulsive and the person gets attracted and kicked out the other side. So it gets a bit faster. So you send it, then you send it back round again.

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And it's incredible, like the timing of the synchronization where it really. Yeah, yeah, yeah. That's I think there's going to be a multiplicative effect.

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And the question is, OK, let me just take that attention for a second. The orchestration of that, is that fundamentally 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 say first of all, say I'm not an engineer. So the guy is I did not build the LHC so that people much, much better at this stuff than I could for sure.

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But maybe but from your sort of intuition, from the the echoes of what you understand, you heard of how is design, what's your sense, how what's the engineering aspects of the acceleration but is not challenging.

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OK, OK. There are always challenges of everything. But basically you have these the beams that go round the LHC, the beams of particles are divided into little bunches. So they're called debris like swarms of bees, if you like. And there are around I think it's something of the order. Two thousand bunches spaced around the ring. And they if you if you were given point on the ring counting bunches, you get 40 million bunches passing you every second.

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So they come in like, you know, like cars going past in a very fast motorway. So you need to have your electric field that you're using to accelerate the particles. That needs to be timed so that as a bunch of protons arrives, it's got the right sign to attract them and then flips at the right moment.

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But I think the voltage in those boxes oscillates at hundreds of megahertz. So the beams that like 40 megahertz is oscillating much more quickly than the beam. So I think, you know, it's difficult engineering, but in principle it's not, you know, a really serious challenge.

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The bigger problem is probably engineers like screaming at you right now, probably. So in terms of coming back to this thing, why is it so big? Well, the reason is you want to get the particles through that accelerating element over and over again. So you want to bring them back round. That's why it's round. The question is why couldn't you make it smaller? Well, the basic answer is that these particles are going unbelievably quickly.

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So they travel at ninety nine point nine nine nine nine nine nine one percent of the speed of light in the LHC. And if you think about C driving your car around the corner, a high speed, if you go fast, you need a very you need a lot of friction in the tires to make sure you don't slide off the road.

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So the the limiting factor is how powerful a magnet can you make? Because it's what we do is the magnets are used to bend the particles round the ring. And essentially the LHC, when it was designed, was designed with the most powerful magnets that could conceivably be built at the time. And so that's kind of limiting factors.

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If you wanted to make the machines smaller, that means a tighter band. You need to have a more powerful magnet. So it's this toss up between how strong your magnets versus how big a tunnel can you afford. The bigger the tunnel, the weaker the magnets. B, the smaller the tunnel, the stronger they've got to be. OK, so maybe can we backtrack that a model and say what kind of particles there are, period? And maybe the history of kind of assembling that, the standard model of physics and then how that leads up to the hopes and dreams and the accomplishments of the Large Hadron Collider.

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Yeah, sure. OK, so all of 20th century physics in like five minutes. Yeah, please. OK, so OK, the story really begins properly.

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End of the 19th century.

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The basic view of matter is that matter is made of atoms and the atoms are indestructible, immutable little spheres like the things we were talking about.

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They don't really exist. And there's one atom for every chemical element. So it's an atom for hydrogen, for helium, for carbon, for iron, etc.. And they're all different than in 1897. Experiments done at the Cavendish Laboratory in Cambridge, where I'm still where I'm based, show that there are actually smaller particles inside the atom, which eventually became known as electrons. These are these negatively charged things that go round the outside a few years later. And it's Rutherfords, very famous.

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Nuclear is one of the pioneers of nuclear physics, shows that the atom has a tiny nugget in the center, which we call the nucleus, which is a positively charged object. So then by like 1910 11, we have this model of the atom that we learn in school, which is you've got a nucleus, electrons go round it.

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Fast forward, you know, a few years the nucleus, people start doing experiments with radioactivity where they use alpha particles that are spat out of radioactive elements as as bullets and they fire them other atoms. And by banging things into each other, they see that they can knock bits out of the nucleus. So these things come out called protons, first of all, which are positively charged particles about 2000 times heavier than the electron. And then 10 years later, more or less a neutral particle is discovered called a neutron.

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So those are the three basic building blocks of atoms. You have protons and neutrons in the nucleus that are stuck together by something called a strong force, the strong nuclear force. And you have electrons in orbit around that held in by the electromagnetic force, which is one of the forces of nature. That's sort of where we get to by like 1932, more or less.

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Then what happens is physics is nice and neat. In 1932, everything is great. We've got three particles in all the atoms are made of. That's fine. But then cloud chamber experiments. These are devices that can be used to the first devices capable of imaging subatomic particles. So you can see their tracks and they're used to study cosmic rays, particles that come from outer space and bang into the atmosphere.

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And in these experiments, people start to see a whole lot of new particles. So they discover, for one thing, antimatter, which is the source of a mirror image of the particles. So we discover that there's also, as well as the negatively charged electron, there's something called a positron, which is a positively charged version of the electron. And there's an antiproton which is negatively charged, and then a whole load of other weird particles start to get discovered and no one really knows what they are.

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This is known as the zoo of particles. Are these discoveries not the first theoretical discoveries or the discoveries in an experiment? So like. Well, yeah. What's the process of discovery for these early sets of it is a mixture.

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I mean, the early stuff around the atom is really experimentally driven. It's not based on some theory. It's exploration in the lab using equipment. So it's really people just figuring out getting hands on with the phenomena of figuring out what these things are. And the theory comes a bit later that there is that's not always the case. So in the discovery of the anti electron, the positron that was predicted from quantum mechanics and relativity by a very clever theoretical physicist called Paul Dirac, who was probably the second brightest, you know, physicist of the 20th century, apart from Einstein, isn't as well anywhere near as well known.

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So he predicted the existence of the anti electron from basically a combination of the theories of quantum mechanics and relativity. And it was discovered about a year after he made that prediction.

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What happens when an electron meets a positron? They annihilate each other. So if you when you bring a particle into antiparticle together, they they react well, they react. They just wipe each other out and they turn their masses turned into energy, usually in the form of photons. So you get light produced.

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So when you have that kind of situation, why why does the universe exist at all? If there's matter in any matter? Oh, God. Now we're getting into really big questions.

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So you want to go there now?

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That's maybe go there later. That's because I mean, that is a very big question. Yeah. Let's let's let's take it slow with the standard model. So, OK, so there's this matter and antimatter in the 30s, so what else.

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So matter and antimatter and then a load of new particles start turning up in these cosmic ray experiments, first of all. And they don't seem to be particles that make up atoms. There's something else. They all mostly interact with a strong nuclear force. So they're a bit like protons and neutrons and buy in the 1960s in America particularly, but also in Europe and. Russia scientists, scientist, particle particle accelerator. So these are the forerunners of the LHC is a big ring shaped machines that were, you know, hundreds of meters long, which in those days was enormous in most physics.

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Up until that point had been done in labs, in universities with small bits of kit. So this is a big change. And when these accelerators are built, they start to find they can produce even more of these particles. So I don't know the exact numbers, but by around 1960, there are over 100 of these things that have been discovered and physicists are kind of tearing the hair out because physics is all about simplification. And suddenly what was simple has become messy and complicated.

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And everyone sort of wants to understand what's going on as a quick kind of aside and probably really dumb question.

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But how is it possible to take something like a like a photon or an electron and be able to control it enough, like to be able to do a controlled experiment where you collide against something else?

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Is that is that this seems like an exceptionally difficult engineering challenge because you mentioned vacuum tubes.

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So you basically want to remove every other distraction and really focus on this collision. How difficult of an engineering challenge that just to get a sense and it's very hard. I mean, in the early days, particularly when the first accelerators are being built in 1932, Ernest Lawrence builds the first what we call a cyclotron, which is like a little salary to this big or so. There's another one, that big, tiny little thing. Yeah. I mean, so most of the first accelerators were what we call fixed target experiments.

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So you had a ring. You accelerate particles around the ring and then you fire them out the side into some target. So that makes the kind of the colliding bit is relatively straightforward. Could use fire, whatever it is you want to fire. The hard bit is the steering, the beams with the magnetic fields getting, you know, strong enough electric fields to accelerate them, all that kind of stuff. The first colliders where you have two beams colliding head on, that comes later.

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And I don't think it's done until maybe the 1980s. I'm not entirely not entirely sure, but it is much harder problem.

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That's crazy because it's like perfectly the attempt to hit each other. And we're talking about what scale?

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What's the I mean, the temporal thing is a giant mess, but the spacially like the size. Mm. Is tiny. What's give you a sense that the LHC beams the cross-sectional diameter is that I think around a dozen or so microns.

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So you know ten, ten millions of a of a meter and a beam.

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So just to clarify, a beam contains how many is it the bunches that you mentioned. Yeah. Multiple partners is just one part. Oh no, no. The bunches contain say 100 billion protons each. So a bunch is is not rebundle shaped it. They're actually quite long. They're like 30 centimetres long but thinner than a human hair. So like very, very narrow, long sort of objects. Those are the things. So what happens in the LHC is you steer the beams so that they cross in the middle of the detector.

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So they basically have these swarms of protons that are flying through each other.

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And most of the you have 100 billion coming one way, billion another way, maybe ten of them will hit each other.

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Okay, so this is a lot more sense. That's nice. You're trying to use sort of it's a probabilistically you're not you can't make a single particle collide with a single.

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Yeah. So that's not an efficient way to do it. You'd be waiting a very long time to get anything. Yeah.

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So you're basically right. You're relying on probability to be some fraction of them are going to collide and then, you know, which is it? It's a it's a swarm of the same kind of particle.

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So it doesn't matter which ones each other. Exactly. I mean, that that's not to say it's not hard. You've got to one of the challenges to make the collisions work is you have to squash these beams to very, very basically the narrower they are, the better, because the higher the chances of them colliding. If you think about two flocks of birds flying through each other, the birds are far apart in the flocks. There's not much chance that they'll collide if they're all flying densely together and they're much more likely to collide with each other.

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So that's the sort of problem. It's tuning those magnetic fields, getting them powerful. If you squashed the beams and focused them so that you get enough collisions, that's super.

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Do you know how much software is involved here? I mean, it's sort of like on the software world and it's fascinating.

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This seems like it's a software as buggy and messy.

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And so, like, you almost don't want to rely on software too much. Like if you do, it has to be like low level, like Fortran style programming. Language software is a Large Hadron Collider.

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I mean, it depends at which level a lot. I mean, the whole thing is obviously computer controlled. So I mean, I don't know a huge amount about how the software for the actual accelerator works. But, you know, I've been in the. Control center, so at CERN, there's this big control room, which is like a bit like NASA mission control with big banks have, you know, desks where the engineers sit and they monitor the LHC because you obviously can't be in the tunnel when it's running.

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So everything's remote.

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I mean, one sort of anecdote about the sort of software side in 2008 when the LHC first switched on, they had this big launch event and then, you know, big press conference party to inaugurate the machine. And about 10 days after that, they were doing some tests and the dramatic event happened where a huge explosion basically took place in the tunnel that destroyed or damaged, badly damaged about about half a kilometer of the machine.

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But the stories the engineers are in the control room. That day, one guy told me the story about, you know, basically all these screens they have in the control room started going red. So these alarms like, you know, kind of in software going off. And then they assume that there's something wrong with the software because there's no way something this catastrophic could have could have happened.

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Yeah, but I mean, when I worked on when I was a teacher and one of my jobs was to help to maintain the software that's used to control the detector that we work on. And that was it's relatively robust. Not so you don't want it to be too fancy. You don't want to sort of fall over to the more clever stuff comes when you're talking about analyzing the data.

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And that's where they're sort of, you know, are we jumping around to make do we finish with a standard model? We didn't. We didn't. We started talking about quarks. We haven't talked to them yet.

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No, we got to the masses of particles.

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Let me go back there if it's OK. OK, that's going to take us the rest of the history of physics in the twentieth century. OK, sure. OK, so circa 1960, you have this you have these 100 or so particles. It's a bit like the periodic table all over again. So you've got like, like having 100 elements, sort of about like that and people trying to start to try to impose some order. So Murray Gellman, he's a theoretical physicist, American from New York.

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He realizes that there are these symmetries in these particles that if you arrange them in certain ways, that they relate to each other. And he uses the symmetry principles to predict the existence of particles that haven't been discovered, which are then discovered in accelerators. So this starts to suggest there's not just random collections of crap.

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There's like, you know, actually some order to this underlying it a little bit later in 1960, around the 1960s, he proposes, along with another physicist called George Zweig, that the symmetries arise because just like the patterns in the periodic table arise, because atoms are made of electrons and protons, that these patterns are due to the fact that these particles are made of smaller things and they are called quarks. So these are the particles that predicted from theory for a long time.

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No one really believes that real. A lot of people think that they're a kind of theoretical convenience that happen to fit the data. But there's no evidence. No one's ever seen a quark in any experiment and lots of experiments done to try to find quarks to try to knock a quark out of a.. So the idea if protons and neutrons are made of quarks, you should wait to knock a clock out and see the quark. That never happens. And we still have never actually managed to do that.

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We really know.

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So the way but the way that it's done in the end is this machine that's built in California at the Stanford lab, Stanford Linear Accelerator, which is essentially a gigantic three kilometer long electron gun fires, electrons, almost speed of light at protons.

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And when you do these experiments, what you find is a very high energy. The electrons bounce off small, hard objects inside the proton. So it's a bit like taking an X-ray of the proton. You're firing these very light high energy particles and they're pinging off. Little things inside the proton are like ball bearings, if you like. So you actually that way they resolve that there are three things inside the proton which are quarks, the quarks that Galman and Zweig had predicted.

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So that's really the evidence that convinces people that these things are real. The fact that we've never seen one in an experiment directly, they're always stuck inside other particles.

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And the reason for that is essentially to do with a strong force. The strong force is the force that holds quarks together and it's so strong that it's impossible to actually liberate a clock. So if you try and pull a quark out of a proton or actually ends up happening, is that the you kind of create this that this springlike bond in a strong force? Imagine two quarks that are held together by very powerful spring. You pull, pull and pull.

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More and more energy gets stored in that bond, like stretching a spring. And eventually the tension gets so great. The spring snaps and the energy in that bond gets turned into two new quarks that go on the broken ends. So you started with two quarks. You end up with four quarks. So you never actually get to take a clock out. You just end up making loads more quarks in the process.

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So how do we, again, forgive the dumb question. How do we know quarks are real then?

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Well, away from these experiments where we can scatter you fire electrons into the protons. They can. Burrow into the proton and knocka and they can bounce off these quark, so you can see from the angles the electrons come out, you can infer, you can infer that these things are there. The model can also be used.

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It has a lot of successes. So you can use it to predict the existence of new particles that hadn't been seen. So basically, there's lots of data basically showing from, you know, when we fire protons at each other at the LHC. A lot of clocks get knocked all over the place, and every time they try and escape from, say, one of their protons, they make a whole set of clocks that go flying off as bound up in other sorts of particles made of clocks.

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So that all the sort of the theoretical predictions from the basic theory of the strong force and the clocks all agrees with what we are saying experiments. We've just never seen an actual quark on its own because unfortunately, it's impossible to get them out on their own.

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So quarks these crazy, smaller things that are hard to imagine a real. So what else what else is part of the story here?

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So the other thing that's going on at the time around the 60s is an attempt to understand the forces that make these particles interact with each other. So you have the electromagnetic force, which is the force that was sort of discovered to some extent in this room or at least in this building. So the first what we call quantum field theory of the electromagnetic force is developed in the 1940s and 50s by Feynman, Richard Feynman, amongst other people, Julian Suring, a Tominaga who come up with the first what we call a quantum field theory of the electromagnetic force.

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And this is where this description of which I gave you at the beginning, that particles are ripples in fields. Well, in this theory, the photon, the particle of light is described as a ripple in this quantum field called the electromagnetic field and the attempt that is made to try what can we come up with, a quantum field theory of the other forces, of the strong force and the weak. The other the third force, which we haven't discussed, which is the weak force, which is a nuclear force.

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We don't really experience it in our everyday lives, but it's responsible for radioactive decay is the force that allows, you know, in a radioactive atom to turn into a different element, for example.

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And I don't know if you were explicitly mentioned, but so there's technically four forces.

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Yes.

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I guess three of them would be in the standard model, like the weak, the strong and the electromagnetic.

[00:31:30]

And then there's gravity and there's gravity, which we don't worry about that, because in this case, we bring that up at the end of the gravity. So far, we don't have a quantum theory of and if you can solve that problem, you win a Nobel Prize.

[00:31:42]

Well, we're going to have to bring up the graviton at some point. I'm going to ask you, but let's leave that aside for now. So those three, OK, Feynman electromagnetic force, the quantum field. Yeah.

[00:31:56]

So where does the weak force command. So so.

[00:31:59]

Yeah. Well, first of all, I mean, the strong force is the easiest, the strong force is a little bit like the electromagnetic force. It's a force that binds things together. So that's the force that holds quarks together inside the proton, for example.

[00:32:09]

So a quantum field theory of that force is discovered in the I think it's in the 60s and it predicts the existence of new force particles called gluons. So gluons are a bit like the photon. The photon is the particle of electromagnetism. Gluons are the particles of the strong force. So there's there's just like there's an electromagnetic field, there's something called a gluon field, which is also all around us.

[00:32:36]

So these are some of these particles, I guess, the force carriers or whatever, they carry them.

[00:32:41]

Well, it depends how you want to think about it. I mean, really, the field, the strong force field, the glue on field is the thing that binds the quarks together.

[00:32:49]

The gluons are the little ripples in that field so that in the same way that the photon is a ripple in the in the electromagnetic field. But the thing that really does the binding is the field. I mean, you may have heard people talk about things like virtual. You've had the phrase virtual particle. So sometimes in some if you hear people describing how forces are exchanged between particles, they quite often talk about the idea that, you know, if you have an electron and another electron say, and they're repelling each other through the electromagnetic electromagnetic force, you can think of that as if they're exchanging photons.

[00:33:22]

So they're kind of firing photons backwards and forwards between each other. And that causes them to repel that photons then a virtual particle.

[00:33:30]

Yes, that's what we call a virtual particle. In other words, it's not a real thing. It doesn't actually exist. So it's an artifact of the way theorists do calculations. So when they do calculations in quantum field theory, rather than there's no one discovered a way of just treating the whole field, you have to break the field down into simpler things so you can basically treat the field as if it's made up of lots of these virtual photons. But there's no experiment that you can do that can detect these particles being exchanged.

[00:33:55]

What's really happening in reality is that the electromagnetic field is warped by the charge of the electron and that causes the force. But the way we do calculations involves particles. So it's a bit confusing, but it is really a mathematical technique.

[00:34:10]

It's not something that corresponds to reality.

[00:34:12]

I mean, that's part, I guess, of the Feynman diagrams. Yes, this is virtual. That's right. Yeah. Some of these have mass.

[00:34:19]

Some of them don't. Is that does that or what does that even mean? Not to have mass and maybe you can say which one of them have mass, which don't. OK, so.

[00:34:31]

And why is mass important? All relevant in this in this in this field view of the universe.

[00:34:38]

Well, there are only two particles in the standard model that don't have mass, which are the photon and the gluons. So they are massless particles, but the electron, the quarks. And there are a bunch of other particles I haven't discussed. There's something called a million and a tau, which are basically heavy versions of the electron that are unstable. You can make them and accelerators, but they don't form atoms or anything.

[00:35:01]

They don't exist for long enough. But all the matter particles, there are 12 of them, six quarks and six what we call leptons, which includes the electron and its two heavy versions and three neutrinos. All of them have mass and so do the. This is the critical bit. So the weak force, which is the third of these quantum forces, which is one of the hardest to understand, the force particles of that force have very large masses and there are three of them.

[00:35:31]

They're called the W plus, the minus and the Z goes on and they have masses of between 80 and 90 times that of the the protons. They're very heavy.

[00:35:42]

And while they're very heavy, the what the heaviest I guess they're not the heaviest.

[00:35:47]

The heaviest particle is the top quark, which has a mass of about 175 ish protons. So that's really massive.

[00:35:56]

And we don't know why is so massive, but they're coming back to the weak force.

[00:36:00]

So the problem in the 60s and 70s was that the reason that the electromagnetic force is a force that we can experience in our everyday lives.

[00:36:08]

So if we have a magnet and a piece of metal, you can hold it, you know, a Metropol if it's powerful enough and you'll feel a force, whereas the weak force only becomes apparent when you basically have two particles touching at the scale of a nucleus. So you get to very short distances before this force becomes manifest.

[00:36:26]

It's not we don't get weak forces going on in this room. We don't notice them.

[00:36:30]

And the reason for that is that the particle, the the field that transmits the weak force, the particle that's associated with that field, has a very large mass, which means that the field dies off very quickly, says you. Whereas an electric charge, if you were to look at the shape of the electromagnetic field, it would fall off with this. You have this thing called the inverse square law, which is the idea that the force halves every time you double the distance.

[00:36:55]

No, sorry, it doesn't have quarters every time. Every time you double the distance between, say, the two particles, whereas the weak force kind of you move a little bit away from the nucleus and just disappears. The reason for that is because these these fields, the particles that go with them have a very large mass.

[00:37:12]

But the problem that was that theories faced in the 60s was that if you tried to introduce massive force fields, the theory gave you nonsensical answers. So you'd end up with infinite results for a lot of the calculations you tried to do.

[00:37:28]

So the basically turned out, it seemed the quantum field theory was incompatible with having massive particles, not just the force particles, actually, but even the electron was a problem.

[00:37:38]

So this is why the Higgs that we sort of alluded to comes in and the solution was to say, OK, well, actually all the particles in the standard model are mass. They have no mass. So the quarks, the electron, they don't have a mass. Neither do these weak particles. They don't have mass either. What happens is they actually acquire mass through another process. They get it from somewhere else. They don't actually have it intrinsically.

[00:38:00]

So this idea that was introduced by Peter Higgs is the most famous. But actually there are about six people that came up with the idea more or less the same time is that you introduce a new quantum field, which is another one of these invisible things that's everywhere.

[00:38:14]

And it's through the interaction with this field that particles get mass. So you can think of, say, an electron in the Higgs field called the Higgs field kind of bunches around the electron. It's sort of a drawn towards the electron. And that energy that's stored in that field around the electron is what we see as the mass of the electron.

[00:38:36]

But if you could somehow turn off the Higgs field, then all the particles in nature would become massless and fly around at the speed of light.

[00:38:43]

So this this idea of the Higgs field allowed other people or the theorists to come up with a well, it was another a unit, basically a unified theory of the electromagnetic force and the work force. So once you bring in the Higgs field, you can combine two of the forces into one. So it turns out the electromagnetic force and the weak force are just two aspects of the same fundamental force.

[00:39:09]

And at the LHC, we go to high enough energies that you see these two forces unifying effectively.

[00:39:16]

So so first of all, it started as a theoretical notion like this.

[00:39:22]

And then it wasn't the Higgs called the God particle. At some point it was by a guy trying to sell popular science books.

[00:39:30]

Yeah, yeah. But. I mean, I remember when I was hearing it, I thought it would. I mean, that would solve a lot of the unify a lot of our ideas of physics was my notion, but maybe you can speak to that was as big of a leap.

[00:39:47]

Is that as a God particle, that Jesus particle at which which, you know, what's the big contribution of Higgs in terms of this unification power?

[00:39:57]

Yeah, I mean, to understand that it maybe helps know the history a little bit. So when the what we call electroweak theory was put together, which is where you unify electromagnetism with a weak force and the Higgs is involved in all of that. So that theory, which was written in the mid 70s, predicted the existence of four new particles. The plus both on the minus goes on, the Z Bo's on, and the Higgs boson. So there were these four particles that came with the theory that were predicted by the theory in 1983, 84, the W's and the Z particles were discovered an accelerator at CERN called the Super Proton Synchrotron, which was a seven kilometer particle collider.

[00:40:36]

So three of the bits of this theory had already been found. So people were pretty confident from the 80s that the Higgs must exist because it was a part of this family of particles that this theoretical structure only works if the Higgs is there. So what then happens? So this question of why is the LHC the size it is? Yes. Well, actually, the tunnel that the LHC is in was not built for the LHC. It was built from for a previous accelerator called the Large Electron Positron Collider.

[00:41:05]

So that that was began operation in the late 80s, early 90s.

[00:41:10]

They basically that's when they dug the 27 kilometer tunnel. They put this accelerator into a collider that fires electrons and anti electrons at each other, electrons and positrons.

[00:41:19]

So the purpose of that machine was, well, it was actually to look for the Higgs. That was one of the things it was trying to do. It didn't matter. It didn't have enough energy to do it in the end.

[00:41:28]

But the main thing it achieved was it studied the W and the Z particles at very high precision. So it made loads of these things previously, only make a few of them at the previous accelerator. So you could study these. Really, really, precisely. And by studying their properties, you could really test this electroweak theory that had been invented in the 70s and really make sure that it worked. So actually by 1999, when this machine turned off, people knew.

[00:41:54]

Well, you never know until you until you find the thing. But people were really confident this electroweak theory was right and that the Higgs, almost the Higgs or something very like the Higgs had to exist because otherwise the whole thing doesn't work. It'd be really weird if you could discover and these particles, they all behave exactly as a theory, tells you they should. But somehow this key piece of the picture is not there.

[00:42:17]

So in a way, it depends how you look at it.

[00:42:20]

The discovery of the Higgs on its own is is a huge achievement in many, both experimentally and theoretically. On the other hand, it's this it's like having a jigsaw puzzle where every piece has been filled in this beautiful image.

[00:42:34]

There's one gap and you kind of know that that piece must be there somewhere. Right?

[00:42:39]

So if so, the discovery in itself, although it's important. Is not so interesting. It's a confirmation of the obvious at that point. But what makes it interesting is not it just completes the standard model, which is a theory that we've known had the basic layout office for 40 years or more. Now it's that the Higgs actually is a is a unique particle, is very different to any of the other particles in the standard model. And it's a theoretically very troublesome particle.

[00:43:12]

There are a lot of nasty things to do with the Higgs, but also opportunities.

[00:43:17]

So we basically don't really understand how such an object can exist in the form that it does. So there are lots of reasons for thinking that the Higgs must come with a bunch of other particles or that it's perhaps made of other things. So it's not a fundamental particle that it's made of smaller things. I can talk about that, if you like a bit.

[00:43:36]

That's still a notion. So, yeah. So so the Higgs might not be a fundamental particle that there might be some in my old man.

[00:43:44]

So that that is an idea is not you know, there's not been demonstrated to be true. But I mean, there's all of these ideas basically come from the fact that.

[00:43:53]

Is this is this is a problem that motivated a lot of development in physics in the last 30 years or so, and there's this basic fact that the Higgs field, which is this field that's everywhere in the universe, this is the thing that gives mass to the particles and the Higgs field is different from all the other fields in that, let's say you take the electromagnetic field, which is, you know, if we actually have to measure the electromagnetic field in this room, we would measure all kinds of stuff going on because there's light, there's going to be microwaves and radio waves and stuff.

[00:44:19]

But let's say we go to really, really remote part of empty space and shield it and put a big box around it and then measure the electromagnetic field in that box. The field would be almost zero apart from some little quantum fluctuations, but basically it goes to naught. The Higgs field has a value everywhere. So it's a bit like the whole like the entire of space has got this energy stored in the Higgs field, which is not zero.

[00:44:42]

It's it's finite. It's got some it's a bit like having the the temperature of space raised to, you know, some background temperature. And it's that energy that gives mass to the particles. So the reason that electrons and quarks have mass is through the interaction with this energy that's stored in the Higgs field.

[00:45:01]

Now, it turns out that the precise value of this energy has has to be very carefully tuned if you want a universe where interesting stuff can happen. So if you push the Higgs field down, it has a tendency to collapse to what? There's a tent. If you do your sort of naïf calculations, there are basically two possible likely configurations for the Higgs field, which is either it's zero everywhere, in which case you have a universe, which is just particles with no mass that can't form atoms and just fly about the speed of light or it explodes to an enormous value, what we call the Planck scale, which is the scale of quantum gravity.

[00:45:41]

And at that point, if the Higgs field was that strong, even an electron would become so massive that it would collapse into a black hole. And then you have a universe made of black holes and nothing like us.

[00:45:51]

So it seems that the strength of the Higgs field is to actually achieve the value that we see requires what we call fine tuning of the laws of physics. You have to fiddle around with the other fields in the standard model and their properties to just get it to this right sort of Goldilocks value that allows atoms to exist.

[00:46:10]

This is deeply fishy. People really dislike this.

[00:46:14]

Well, yeah, I guess so. What would be two explanations? One, there's a God, the design this perfectly. And two is there's an infinite number of alternate universes and we just happen to be in the one in which life is possible. Yeah, complexity. So when you say I mean life, any kind of complexity, that's not either complete chaos or black holes. Yeah, yeah. I mean, how does that make you feel?

[00:46:39]

What do you make that such a fascinating notion that this perfectly tuned field. That's the same everywhere. Yeah. Is there. What do you make of that. Yeah.

[00:46:50]

What do you make of that. I mean, yes, you laid out two of the possible explanations. Yeah. I mean, someone you know, some cosmic creator. Well, yeah. Let's fix that. Be at the right level. That's one possibility. I guess it's not a scientifically testable one. But, you know, theoretically, I guess it's possible.

[00:47:05]

Sorry to interrupt, but there could also be not a designer. But couldn't there be just I guess I'm not sure what that would be, but some kind of force that. That some kind of mechanism by which this this. This kind of field is enforced in order to create complexity, basic basically forces that. Paul, the universe towards an interesting complexity, I mean, yeah, I mean, those ideas, I don't really subscribe to them.

[00:47:40]

As I'm saying, it sounds really stupid. No, I mean, there are definitely people that make those kind of arguments, you know, those ideas that I think it's least Merlin's idea. I think that, you know, universes are born inside black holes.

[00:47:55]

And so universe is the have of Darwinian evolution of the universe where universes give birth to other universes. And if universes where black holes can form are more likely to give birth to more universes. So you end up with universes which have similar laws. I mean, I don't know whatever.

[00:48:09]

But I talked to Dr. Lee recently on this podcast, and he's he's a reminder to me that the physics community has like so many interesting characters. Yeah, it's fascinating. Anyway, so so, I mean, as an experimentalist, I tend to sort of think these are interesting ideas, but they're not really testable. So I tend to think about it very much. So. I mean, going back to the science of this, there wasn't there is an explanation.

[00:48:36]

There is a possible solution to this problem of the Higgs, which doesn't involve multiverses or creators fiddling about with the laws of physics. If the most popular solution was something called supersymmetry, which is a theory which is inveigle involves a new type of symmetry of the universe. In fact, it's one of the last types of symmetries that is possible to have that we haven't already seen in nature, which is a symmetry between force particles and matter particles.

[00:49:01]

So what we call fermions, which are the matter particles and bosons, which are force particles.

[00:49:06]

And if you have supersymmetry, then there is a super partner for every particle in the standard model and the without going into details, the effect of this basically is that you have a whole bunch of other fields and these fields cancel out the effect of the standard model fields and they stabilize the Higgs field at a nice, sensible value. So in supersymmetry, you naturally, without any tinkering about with the constants of nature or anything, you get Higgs field with a nice value, which is what we see.

[00:49:35]

So this is one of the supersymmetry is also got lots of other things going for it. It predicts the existence of a dark matter particle, which would be great. You know, it potentially suggests that the strong force and the electroweak force unify energy. So lots of reasons. People thought this was a productive idea. And when the LHC was just before it was turned on, there was a lot of hype, I guess a lot of an expectation that we would discover these super partners because and particularly the main reason was that if if supersymmetry stabilises the Higgs field at this nice Goldilocks value, these super particles should have a mass around the energy that we're probing at the LHC around the energy of the Higgs.

[00:50:16]

So it was kind of thought you discovered the Higgs. You probably discover super partners. So once you start creating ripples in this Higgs field, you should be able to see these kinds of it should be super fields would be there.

[00:50:27]

And at the very beginning, I said we're probing the vacuum. What I mean is really that, you know, let's say these super fields exist. The vacuum contains super fields. There were these supersymmetric fields. If we hit them hard enough, we can make them vibrate. We see super particles come flying out. That's the sort of that's the idea.

[00:50:43]

That's the whole point. But we haven't. But we haven't. So so far at least, I mean, we've had now a decade of data taking at the LHC. No signs of super partners have supersymmetric particles have been found. In fact, no signs of any physics, any new particles beyond the standard model have been found. So supersymmetry is not the only thing that can do this. There are other theories that involve additional dimensions of space or potentially involve the Higgs boson being made of smaller things being made of other particles.

[00:51:15]

Yeah, that's an interesting you know, I haven't heard that before. That's really that's an interesting point, because you maybe linger on that. Like what what could be what could the Higgs particle be made of?

[00:51:25]

Well, so the oldest I think the original ideas about this was these theories called Technicolor, which were basically like an analogy with the strong force.

[00:51:34]

So the idea was the Higgs boson was a bound state of two very strongly interacting particles that were a bit like quarks. So like quarks, but I guess higher energy things with a super strong force and not the strong force, but a new force that was very strong. And the Higgs was a bound state of of these these objects and the Higgs boson principle, if that was right, would be the first in a series of Technicolor particles, Technicolor, I think not being a theorist, but is not based basically not done very well, particularly since the LHC found the Higgs.

[00:52:06]

That kind of it rules out, you know, a lot of these Technicolor theories. But there are other things that are a bit like Technicolor. So there's a theory called partial composite ness, which is an idea that some of my colleagues at Cambridge have worked on, which is a similar sort of idea that the Higgs is a bound state of some strongly interacting particles and that the standard model particles themselves, the more exotic ones like the top. They are also sort of mixtures of these composite particles, so it's a kind of an extension to the standard model which explains this problem with the Higgs boson is Goldilocks value, but also helps us understand we have we're in this situation now, again, a bit like the periodic table where we have six quarks, six leptons in this kind of range, in this nice table.

[00:52:56]

And there you can see these columns where the patterns repeat and you go, OK, maybe there's something deeper going on here, you know? And so this would potentially be something this partial composite theory could explain a sort of enlarge this picture that allows us to see the whole symmetrical pattern and understand what the ingredients. Why do we have. So one of the big questions in particle physics is why are there three copies of the matter particles?

[00:53:23]

So in what we call the first generation, which is what we're made of, there's the electron, the electron neutrino, the up quark and the down quark. They're the most common matter particles in the universe. But then there are copies of these four particles in the second and third generations. So things like muons and top quarks and other stuff, we don't know why we see these patterns. We have no idea where it comes from. So that's another big question.

[00:53:45]

You know, can we find out the deeper order that explains this particular type periodic table of particles that we see is the possible that the the deeper order includes like almost a single entity.

[00:53:59]

So like something that I guess like string theory dreams about is this is this is this is this essentially the dream is to discover something simple, beautiful, unifying.

[00:54:10]

Yeah. I mean, that is the dream. And or I think for some people, for a lot of people it still is the dream.

[00:54:17]

So there's a great book by Steven Weinberg, who is one of the theoretical physicists who was instrumental in building the standard model. So he came up with some others with the electroweak theory, the theory that unified electromagnetism and the weak force. And he wrote this book, I think it was towards the end of the 80s, early 90s, called Dreams of a Final Theory, which is a very lovely, quite short book about this idea of a final unifying theory that brings everything together.

[00:54:44]

And I think you get a sense, reading his book written at the end of the 80s, early 90s, that there was this feeling that such a theory was coming. And that was the time when string theory had been was was very exciting. So string theory, there's been this thing called the super string revolution and theoretical physics are very excited. They discovered these theoretical objects, these little vibrating loops of string that in principle not only was a quantum theory of gravity, but could explain all the particles in the standard model and bring it all together.

[00:55:12]

And as you say, you have one object, the string, and you can pluck it. And the way it vibrates gives you these different notes, each of which is a different particle. So it's a very lovely idea.

[00:55:25]

But the problem is that there's there's a few people discovered the mathematics is very difficult. So people have spent three decades more trying to understand string theory. And I think, you know, if you spoke to my string theorists, they would probably freely admit that no one really knows what string theory is yet. I mean, there's been a lot of work, but it's not really understood.

[00:55:44]

And the other problem is that string theory mostly makes predictions about physics that occurs at energies far beyond what we will ever be able to probe in the laboratory. Yeah, probably ever, by the way, to say take a million tangents.

[00:56:01]

But is there room for complete innovation of how to build a particle collider that could give us an order of magnitude increase? And in the kind of energies or do we need to keep just increasing the size of the thing?

[00:56:15]

I mean, maybe yeah. I mean, there are ideas to give you a sense of the Gulf that has to be bridged. So the LHC collides particles at an energy of what we call 14 terra electron volts. So that's basically equivalent of you accelerated a proton through 14 trillion volts. That gets us to the energies where the Higgs and these weak particles live. They're very massive. The scale where strings become manifest is something called the Planck scale, which I think is of the order.

[00:56:47]

Ten to the hang on. It's right is ten to eighteen giga electron volts. So about 10 to the 15 Tera electron volts. So you're talking, you know, trillions of times more energy, more than 10 to the 15 attended the 14th larger.

[00:57:06]

I think it's a very big number. So, you know, we're not talking just an order of magnitude increase in energy. We're talking 14 orders of magnitude energy increase. So to give you a sense of what that would look like, were you to build a particle accelerator with today's technology bigger or smaller than our solar system, a site the size of the galaxy, the galaxy.

[00:57:27]

So you need to put a particle accelerator that circled the Milky Way to get. The energy is where you would see strings if they exist, so that is a fundamental problem, which is that most of the predictions of the unified, this unified theory, quantum theory of gravity only make statements that are testable at energies that we will not be able to probe.

[00:57:49]

And barring some unbelievable, you know, completely unexpected technological or scientific breakthrough, which is almost impossible to imagine, you never, never say never, but it seems very unlikely.

[00:57:59]

Yeah, I can just see the news story. Elon Musk decides to build a particle collider the size of our.

[00:58:07]

It would have to be we'd have to get together with all our galactic neighbors to to pay for it.

[00:58:11]

I think what is the exciting possibilities is the Large Hadron Collider. What is there to be discovered in this in this order of magnitude of scale?

[00:58:21]

Is there other bigger efforts on the horizon in this space where the open problems, the exciting possibilities? You mentioned supersymmetry. Yeah.

[00:58:32]

So well, there are lots of new ideas. Well, there are lots of problems that we're facing. So there's a problem with the Higgs field, which supersymmetry was supposed to solve. There's the fact that 95 percent of the universe we know from cosmology, astrophysics is invisible, that it's made of dark matter and dark energy, which are really just words for things that we don't know what they are. That's what Donald Rumsfeld called a known unknown. We know we don't know what they are.

[00:58:56]

Well, that's better than unknown unknown unknowns. Yeah, well, there may be some unknown unknowns, but we don't know what those are.

[00:59:03]

So, yeah, but the hope is the particle accelerator could help us make sense of dark energy, dark matter. There's still there's some hope for that. There's hope for that.

[00:59:15]

Yes. So one of the hopes is the LHC could produce a dark matter particle in its collisions.

[00:59:20]

And, you know, it may be that the LHC will still discover new particles, that it might still supersymmetry could still be there. We just it's just maybe more difficult to to find than we thought originally. And, you know, dark matter particles might be being produced, but we're just not looking in the right part of the data for them that that's possible. It might be that we need more data, that these processes are very rare and we need to collect lots and lots of data before we see them.

[00:59:44]

But I think a lot of people would say now that the chances of the LHC directly discovering new particles in the near future is quite slim. It may be that we need a decade more data before we can see something or we may not see anything. That's the that's why we are so I mean, the physics, the experiments that I work on. So I work on a detector called LHC B, which is one of these four big detectors that are spaced around the ring.

[01:00:11]

And we do slightly different stuff to the big guys. There's two big experiments, Cloud Atlas and CMS. Three thousand physicists and scientists and computer scientists on them each day are the ones that discovered the Higgs and they look for supersymmetry and dark matter and so on.

[01:00:25]

While we look at our standard model particles called B quarks, which depending on your preferences, either bottom or beauty, we tend to say beauty because it sounds sexier.

[01:00:35]

Yeah, for sure.

[01:00:37]

But these particles are interesting because they of we can make lots of them. We make billions and billions, hundreds of billions of these things. You can therefore measure their properties very precisely so you can make these really lovely precision measurements.

[01:00:51]

And what we are doing really is a sort of complementary thing to the other big experiments, which is they if you think of analogy, they often use is imagine you're looking in you're in a jungle and you're looking for an elephant, say, and you are a hunter and you're kind of like that said as the relevance, very rare.

[01:01:10]

You don't know where in the jungle the jungles, because there's two ways you go about this. Either you can go wandering around the jungle and try and find the elephant. The problem is, if the elephant is there's only one elephant in the jungle, bigger chances of running into a very small or you could look on the ground and see if you see footprints left by the elephant. And if the elephants moving around, you've got a chance that a chance maybe of seeing the elephants footprints.

[01:01:30]

If you see the footprints, you go, OK, there's an elephant. Maybe don't know what kind of elephant it is, but I got a sense there's something out there. So that's sort of what we do. We are the footprint people.

[01:01:40]

We we are we're looking for the footprints, the impressions that quantum fields that we haven't managed to directly create the particle of the effects these quantum fields have on the ordinary standard model fields that we already know about. So these these big particles, the way they behave, can be influenced by the presence of, say, super fields or dark matter fields or whatever you like. And the way they decay and behave can be altered slightly. From what our theory tells us, they ought to behave.

[01:02:09]

And it's easier to collect huge amounts of data and be unbe quarks. We get, you know, billions and billions of these things. You can make very precise measurements. And the only place really at the LHC or really in high energy physics at the moment, where there's a fairly compelling evidence that there might be something beyond the standard model is in these B. These beauty kwok's the case, just to clarify, which is the difference between the different the four experiments, for example, that you mentioned, is that the kind of particles that are being collided is that the energies of which they're collided?

[01:02:44]

What was the fundamental difference is the different experiments, the collisions of the same.

[01:02:49]

What's different is the design of the detectors. So Atlas and CMS are called they're called what are called general-purpose detectors, and they are basically barrel shaped machines. And the collisions happen in the middle of the barrel and the barrel captures all the particles that go flying out in every direction. So in a sphere, effectively, they come flying out and it can record all of those particles.

[01:03:08]

And what's the. So to be interrupting. But what's what's the mechanism of the recording?

[01:03:14]

Oh, these detectors, if you're seeing pictures of the huge like Atlas is 25 metres high in forty metres long and vast machines, instruments, I guess you could call them really.

[01:03:26]

They are they're kind of like onions.

[01:03:28]

So they have layers, concentric layers of detector detectors, different sorts detectors. So close into the beam pipe you have what are called usually made of silicon. They're tracking detectors. So they're little made of strips of silicon or pixels of silicon. And when a particle goes through the silicon, it gives a little electrical signal and you get these dots, you know, electrical dots through your detector, which allows you to reconstruct the trajectory of the particle. So that's the middle.

[01:03:51]

And then the outside of these detectors, you have things called calorimeter, which measure the energies of the particles and the very edge. You have things called muon chambers, which basically these Muan particles, which are the heavy version of the electron, they are they like high velocity bullets and they can get right to the edge of the detectors if you see something at the edge that's immune.

[01:04:09]

So that's broadly how they work. And all of that is being recorded. That's all being fed out to computers.

[01:04:15]

Data must be awesome. OK, so LHC is different. So we because we're looking for these B quarks. Yes. B quarks tend to be produced along the beamlines. So in a collision, the B tend to fly sort of close to the beam pipe. So we built the detector, that sort of pyramid cone shaped basically that just looks in one direction. So we ignore, give you a collision, stuff goes everywhere. We ignore all the stuff over here and going off sideways.

[01:04:40]

We're just looking in this little region close to the beam pipe where most of these big quarks are made.

[01:04:45]

So is there a different aspect of the sensors involved in the collection of the big quark? Is there are some differences. So one of the differences is that one of the ways, you know, you've seen a big walk is that B, corks are actually quite long lived by particle standards. So they live for one point five trillionths of a second, which is if you if you're a fundamental particle is a very long time. Because, you know, the Higgs boson, I think, lives for about a trillionth of a trillionth of a second or maybe even less than that.

[01:05:15]

So these are quite long lived things and they will actually fly a little distance before they decay. So they will fly, you know, a few centimetres. Maybe if you're lucky, then they'll decay into other stuff. So what we need to do in the middle of the detector, you want to be able to see you have your place where the protons crash into each other and that produces loads of particles that come flying out. So you have loads of lines, loads of tracks that point back to that proton collision.

[01:05:38]

And then you're looking for a couple of other tracks, maybe two or three, that point back to a different place that maybe a few centimetres away from the proton collision. And that's the sign that little B particle has flown a few centimetres and decayed somewhere else.

[01:05:50]

So we need to be able to very accurately resolve the proton collision from the B particle decay.

[01:05:56]

So we are the middle of our detector is very sensitive and it gets very close to the collisions. So you have this really beautiful, delicate silicone detector that sits I think it's seven mil millimeters from the beam. And the LHC beam has as much energy as a jumbo jet take off. So it's enough to melt a ton of copper. So you have this furiously powerful thing sitting next, this tiny, delicate silicon sensor.

[01:06:20]

So those aspects of architecture that are specialized to to to measure these particular B quarks that we're interested in.

[01:06:27]

And is there I mean, I remember seeing somewhere that there is some mention of matter and antimatter connected to the B, the these beautiful quarks. Is that what's the connection? Yeah. What's the connection there?

[01:06:42]

Yes, there is a connection, which is that when you produce these big particles, these particles actually to be quark, you see the thing that be quark is inside.

[01:06:52]

So they're bound up inside what we call beauty particles, where the big quokkas joined together with another quark or two, maybe two other quarks, depending on what it is. They're a particular set of these big particles that exhibit this property called oscillation. So if you make a for the sake of argument, amateur version of one of these B particles as it travels because of the magic of quantum mechanics, it oscillates backwards and forwards between its matter and antimatter versions.

[01:07:20]

So does this weird flipping about backwards and forwards. And what we can use this for is a laboratory for testing the symmetry between matter and antimatter. So if the if the symmetry between our two countries is precise, it's exact, then we should see these big particles decaying as often as matters. That doesn't matter, because this oscillation should be even it should spend as much time in each state. But what we actually see is that one of the states spends more time and it's more likely to decay in one state than the other.

[01:07:49]

So this gives us a way of testing this fundamental symmetry between matter and antimatter.

[01:07:56]

So what can you sort of return to the question before about this fundamental symmetry? It seems like if there's perfect symmetry between matter and antimatter, if we have the equal amount of each in our universe, it would just destroy itself. And just like you mentioned, we seem to live in a very unlikely universe where it doesn't destroy itself. Yeah. So just some intuition about why that is.

[01:08:24]

I mean, well, I'm not a theory. I don't have any particular ideas myself. I mean, I sort of do measurements to try and test these things. But I mean, the terms of the basic problem is that in the Big Bang, if you use the standard model to figure out what ought to have happened, you should have got equal amounts of matter and antimatter made. Because whenever you make a particle in our collisions, for example, when we collide stuff together, you make a particle, you make an antiparticle, they always come together, they always annihilate together.

[01:08:47]

So there's no way of making more matter and antimatter that we've discovered so far. So that means in the big bang, you get equal amounts of matter and antimatter as the universe expands and cools down during the Big Bang not very long after the Big Bang.

[01:09:00]

I think a few seconds after the Big Bang, you have this event called the Great Annihilation, which is where all the particles and antiparticles smack into each other annihilate, turn into light mostly, and you end up with a universe later. Or if that was what happened in the universe we live in today would be black and empty. Apart from some photons, that would be it. So there's stuff in this. There is stuff in the universe. It appears to be just made of matter.

[01:09:22]

There's this big mystery as to where the how did this happen? And there are various ideas. Which all involve sort of physics going on in the first trillionth of a second or so of the Big Bang, so it could be that one possibility is that the Higgs field is somehow implicated in this, that there was this event that took place in the early universe where the Higgs field basically switched on. It acquired its modern value.

[01:09:48]

And when that happened, this caused all the particles to acquire mass. And the universe basically went through a phase transition where you had a hot plasma of massless particles. And then in that plasma, it's almost like a gas turning into droplets of water. You get kind of these little bubbles forming in the universe where the Higgs field has acquired its modern value. Particles have got mass and this phase transition in some models can cause more matter and antimatter to be produced depending on how matter bounces off these bubbles in the early universe.

[01:10:18]

So that's one idea. There's other ideas to do with neutrinos, that there are exotic types of neutrinos that can decay in a biased way to just matter and not to actually matter. So people are trying to test these ideas. That's what we're trying to do at LHC base. There's neutrino experiments planned. They're trying to do these sorts of things as well. So, yeah, there are ideas, but at the moment, no clear evidence for which of these ideas might be right.

[01:10:39]

So we're talking about some incredible ideas, by the way, never heard anyone be so eloquent about describing even just the standard model. So, I mean, I just think interesting.

[01:10:52]

Just having fun, enjoying it. So the yes, the theoretical the particle physics is fascinating here. To me, one of the most fascinating things about the Large Hadron Collider is the human side of it that a bunch of. Sort of brilliant people that probably have egos got together and will collaborate together and countries, I guess collaborate together, you know, for the funds and everything, just collaboration everywhere, because you maybe I don't know what the right question here to ask almost was your intuition about how is it possible to make this happen and what are the lessons we should learn for the future of human civilization in terms of our scientific progress?

[01:11:34]

Because it seems like this is a great, great illustration of us working together to do something big.

[01:11:41]

Yeah, I think it's possibly the best example maybe I can think of of international collaboration that isn't for some unpleasant purpose. Basically, you know, is I mean, so I when I started out in the field in 2008 as a new student, the LHC was basically finished. So I didn't have to go around asking for money for it or trying to make the case. So I have huge admiration, admiration for the people who managed that, because this was a project that was first imagined in the 1970s.

[01:12:09]

In the late 70s was when the first conversations about the LHC were mooted.

[01:12:13]

And it took two and a half decades of campaigning and fundraising and persuasion until they started breaking ground and building the thing in the early noughties in 2000.

[01:12:24]

So, I mean, I think the reason just from a sort of from the point of view of the sort of science the scientists there, I think the reason it works ultimately is that everywhere, everyone there is there for the same reason, which is, well, in principle, at least they're there because they're interested in the world. They want to find out, you know, what are the basic ingredients of our universe, what are the laws of nature.

[01:12:47]

And so everyone is pulling in the same direction. Of course, everyone has their own things they're interested in. Everyone has their own careers to consider. And, you know, I wouldn't pretend that there isn't also a lot of competition. So there's this funny thing in these experiments where your collaborators, your eight hundred collaborators in LHC, but you're also competitors because your academics and your various universities and you want to be the one that gets the paper out on the most exciting new measurement.

[01:13:10]

So there's this funny thing where you're kind of trying to stake out your territory while also collaborating and having to work together to make the experiments work. And it does work amazingly well actually, considering all of that.

[01:13:22]

And I think there was actually I think McKinsey or one of these big management consultancy firms went into CERN maybe a decade or so ago to try to understand how these organizations functioned.

[01:13:32]

They figure it out that they think they could. I mean, I think one of the things that interesting, one of the other interesting things about these experiments is that they're big operations like, say, Atlas. Three thousand people.

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Now, there was a person nominally who is the head of Atlas. They're called the spokesperson. And the spokesperson is elected by usually by the collaboration.

[01:13:51]

But they have no actual power, really. I mean, they can't fire anyone. They're not anyone's boss.

[01:13:56]

So, you know, my boss is is a professor at Cambridge, not the head of my experiments. The head of my experiment can't tell me what to do, really. And that's all you've got is independent academics who are their own bosses, who, you know, so somehow it nonetheless, by kind of consensus and discussion and lots of meetings, these things do happen and it does get done.

[01:14:18]

But it's like the queen here in the UK is the spokesperson against those who actually say we don't elect her.

[01:14:23]

No, go after whatever everybody seems to love or don't know from the outside perspective.

[01:14:33]

But, yeah, giant egos, brilliant people, and moving forward, do you think there's actually I would pick up one thing you said just that just the brilliant people thing, because I'm not I'm not saying that people aren't great, but I think there is this sort of impression that physicists will have to be brilliant or geniuses, which is not true, actually. And, you know, you have to be relatively bright for sure.

[01:14:54]

But, you know, a lot of people, a lot of the most successful experimental physicists are not necessarily the people with the biggest brains that the people who, you know, particularly one of the skills that are most important in particle physics is the ability to work with others and to collaborate and exchange ideas and also to work hard. And it's the sort of often it's more determination or a sort of other set of skills is not just being, you know, kind of some great brain virtuoso.

[01:15:19]

I mean, there's parallels to that in the machine learning world. If you want to if you want to solve any real world problems, which I see as the the particle accelerator is essentially a real world instantiation of theoretical physics. And for that, you have to not necessarily be brilliant, but be sort of obsessed, systematic, rigorous, sort of unbearable Stober and all those kind of qualities that make for a great engineer. So the science scientist, purely speaking, that practitioner of the scientific method say you're right.

[01:15:54]

But nevertheless, to me, that's to me as my dad, as a physicist, I argue with him all the time. To me, engineering is the highest form of science and he thinks that's all nonsense, that the real work is done by the theoreticians. So in fact, we have arguments about like people like Elon Musk, for example, because I think his work is quite brilliant. But he's fundamentally not coming up with any serious breakthroughs. He's just creating in this world, implementing.

[01:16:23]

I like making ideas happen to have a huge impact to me. That is that's the Edison. That to me is is a brilliant work. But to him, it's you know, it's messy details that somebody will figure out anyway.

[01:16:42]

I mean, I don't know whether you think there is an actual difference in temperament between, say, a physicist and an engineer, whether it's just what you got interested in, I don't know.

[01:16:51]

I mean, a lot of what experimental physicists do is, to some extent, engineering. I mean, it's not why do I mostly do data stuff? But, you know, a lot of people would be called electrical engineers, but they trained as physicists, but they learn electrical engineering, for example, because they were building detectors. So there's not such a clear divide, I think.

[01:17:09]

Yeah, it's interesting. I mean, there does seem to be like you work with data, does seem to be a certain like I love data collection.

[01:17:18]

There may be an OCD element or something that you're more naturally predisposed to as opposed to like I'm not afraid of data. I love data.

[01:17:27]

And there's a lot of people machine learning or more like they're basically afraid of data collection, afraid of data sets, afraid of all that. They just want to stay in more than theoretical and they're really good at it. Space. I don't know if that's genetic. That's your upbringing, the way you were, the way you go to school, but looking into the future of LHC and other colliders.

[01:17:50]

So there's in there in America, there is, whatever it was called, a super there's a lot of superconducting supercollider supercollider in the desert from Desert Itron. Yeah. So that was cancelled. The construction of that, you know, of, which is a sad thing. But what do you think is the future of these efforts with a bigger collider to be built will be expanded. What do you think?

[01:18:16]

Well, in the near future, the LHC is going to get an upgrade. So that's pretty much confirmed. I think it is confirmed, which is it's not an energy upgrade. It's what we call a luminosity upgrade. So basically means increasing the data collection rates.

[01:18:30]

So more collisions per second, basically because after a few years of data taken, you get this law of diminishing returns where each year's worth of data is a smaller and smaller fraction of the lot. You've only got to to get a real improvement in sensitivity. You need to increase the data rate by an order of magnitude. So that's what this upgrade is going to do. LHC be the moment the whole detector is basically being rebuilt to allow it to record data at a much larger rate than we could before.

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So that will make us sensitive to whole loads of new processes that we weren't able to study before. And, you know, I mentioned briefly these anomalies, anomalies that we've seen.

[01:19:02]

So we've seen a bunch of very intriguing anomalies in these B quark decays, which may be hinting at the first signs of this kind of the elephant, you know, the signs of some new quantum field or fields maybe beyond the standard model. It's not yet at the statistical threshold where you can say that you've observed something, but there's lots of anomalies in many measurements that all seem to be consistent with each other. So it's quite interesting. So, you know, the upgradable allow us to really have.

[01:19:31]

I mean, on these things and see whether these challenges are real, because if they are real and this kind of connects to your point about the next generation of machines, what we would have seen then is, you know, we will have seen the tail end of some quantum field in influencing these big cork's. What we then need to do is to build a bigger collider to actually make the the particle of that field. So if these if these things really do exist.

[01:19:57]

So that would be one argument. I mean I mean, so at the moment, Europe is going through this process of thinking about the strategy for the future. So there are a number of different proposals on the table. One is for a sort of higher energy upgrade of the LHC where you just build more powerful magnets and put them in the same tunnel. That's a sort of cheap, cheaper, less ambitious possibility. Most people don't really like it because it's sort of a bit of a dead end, because once you've done that, there's nowhere to go.

[01:20:22]

There's a machine called Kallick, which is a compact, linear collider, which is an electron positron collider that uses a novel type of acceleration technology to accelerate shorter distances. We're still talking kilometres long, but not like 100 kilometres long. And then the probably the project that is, I think, getting the most support. They'll be interested to see what happens. Something called the Future Circular Collider, which is a really ambitious long term multi decade project to build a 100 km circumference tunnel under the Geneva region.

[01:20:55]

The LHC would become a kind of feeding machine.

[01:20:57]

It would just feed for the same area. So there would be a theater for the. Yeah. So it would kind of the machine would be where the LHC is, but it would sort of go under Lake Geneva and round the Alps basically, you know, up to the edge of the Geneva Basin. So its base, the biggest it's the biggest tunnel you can fit in the region based on the geology kilometres. Yes, it's big. It'd be a long drive.

[01:21:16]

If you're experiments on one side, you've got to go back to CERN for lunch. So that would be a pain for.

[01:21:22]

But, you know, so this project is in principle is actually to accelerate as the first thing you would do is put an electron positron machine in the 100 km tunnel to study the Higgs. You'd make lots of Higgs boson study it really precisely in the hope that you see it misbehaving and doing something that's not supposed to. And then in the much longer term, one that gets taken out, you put in a proton proton machine. So it's like the LHC, but much bigger and bigger.

[01:21:45]

And that's the way you start going and looking for dark matter or you're trying to recreate this phase transition. I talked about in the early universe where you can see matter and antimatter being made, for example, there are lots of things you can do with these machines.

[01:21:58]

The problem is that they will take, you know, the most optimistic. You're not going to have any data from any of these machines until 2040 or, you know, because they take such a long time to build and they're so expensive. So you have a process of R&D design and also the political case being made.

[01:22:14]

So LASU cost a few billion. Depends how you count it. I think most of the sort of more reasonable estimates that take everything into account properly. It's around the sort of 10, 11, 12 billion euro mark.

[01:22:27]

What would be the future? So I forgot the future circular collider for Future Circular. Presumably they won't call it that when it's built because it won't be the future anymore, but they'll call it that. The very Big Hadron Collider, I don't know. But that will I know I should know the numbers, but I think the whole project is estimated at about 30 billion euros. But that's money spent over between now and 2017, probably, which is when the last bit of it would be sort of finishing up, I guess.

[01:22:59]

So you're talking a half a century of science coming out of this thing shared by many countries. So the actual cost, the arguments that are made is that you could make this project fit within the existing budget of CERN if you didn't do anything else.

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CERN, by the way, we didn't mention what is CERN?

[01:23:17]

CERN is the European Organization for Nuclear Research. It's an international organization that was established in the 1950s in the wake of the Second World War as a kind of it was sort of like a scientific Marshall Plan for Europe. The idea was that you bring European science back together for peaceful purposes, because what happened in the forties was, you know, a lot of particular jury scientists, but a lot of scientists from Central Europe had fled to the United States and Europe had sort of seen this brain drain.

[01:23:44]

So as a desire to bring the community back together for a project that wasn't building nasty bombs but was doing something that was curiosity driven. So and that has continued since then. So it's kind of a unique organisation. It's you to be a member as a country. You sort of sign up as a member and then you have to pay a fraction of your GDP each year as a subscription. I mean, it's a very small fraction, relatively speaking.

[01:24:06]

I think it's like I think the UK's contribution is 100 or 200 million quid or something like that. Yeah.

[01:24:12]

Which is quite a lot, but not that fast. I mean, just the whole thing that is possible. It's beautiful. It's a beautiful idea, especially with when there's no wars on the line. Is that like we're freaking out as we actually legitimately collaborating to do good science? One of the things I don't think we really mention is on the final side that sort of the data. Nelson said, is a breakthrough is possible there and the machine learning is there.

[01:24:36]

Is there a lot more signal to be mined in more effective ways from the actual raw data? Yeah, a lot of people are looking into that.

[01:24:44]

I mean, know I'll use machine learning in my data analysis, but pretty nodi, you know, basic stuff because I'm not a machine learning expert. I'm just a physicist who had to learn to do this stuff from my day job. So while a lot of people do is they use kind of off the shelf packages that you can train to do signal noise, you know, just clean up or.

[01:25:04]

Yeah, but one of the big challenges, you know, the big challenge of the data is a it's volume. There's huge amounts of data. So the LHC generates now about the actual numbers are. But if we don't record all our data, we record a tiny fraction of the data. It's like Avoda one 10000 or something. I think that right around that. So it's mostly it's thrown away. You couldn't record or the LHC data because it would fill up every computer in the world in a matter of days, basically.

[01:25:30]

So there's this process that happens on live on the detector, something called a trigger, which in real time, 40 million times every second has to make a decision about whether this collision is likely to contain an interesting object like a Higgs boson or dark matter particle. And it to do that very fast.

[01:25:46]

And the software algorithms in the past were quite relatively basic.

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You know, they did things like measure momentos and energies of particles and put some requirements. So you would say if there's a particle with an energy above some threshold, then record this collision. But if there isn't, don't.

[01:26:03]

Whereas now the attempt to get more and more machine learning in the earliest possible stage, because cool at the stage of deciding whether we want to keep this data or not, but also even even maybe even lower down than that, which is the the point where there's this you know so well generally how the data is reconstructed as you start off with a digital a set of digital hits in your detector. So Channel saying, did you see something? Do you not see something that has to be then turned into tracks, particles going in different directions, and that's done by using fits that fit through the data points and then that's passed to the algorithms that then go, is this interesting or not?

[01:26:37]

Will be better if you could train and machine learning to just look at the raw hits, the basic real basic level information, not have any of the reconstruction done.

[01:26:45]

And it just goes and you can learn to do pattern recognition on this strange three dimensional image that you get. And potentially that's where you could get really big gains, because our triggers tend to be quite inefficient because they don't have time to do the full Whiz-Bang processing to get all the information out that we would like, because you have to do the decision very quickly. So if you can come up with some clever machine learning technique, then potentially you can massively increase the amount of useful data you record and, you know, get rid of more of the background earlier in the process.

[01:27:16]

To me, that's an exciting possibility because then you don't have to build a sort of you can get a gain without having to have to build any hardware or hardware that you need.

[01:27:29]

You need lots of new GPU farms, I guess. So hardware stops.

[01:27:32]

But the you know, I got to talk to you. I'm sort of I'm not sure how to ask, but you're clearly. An incredible science communicator, I don't know if that's the right term, but you're basically a younger Neil deGrasse Tyson with a British accent.

[01:27:51]

So and you've I mean, can you say where we are today? Actually, yeah.

[01:27:56]

So today we're in the Royal Institution in London, which is an old, very old organisation, has been around for about 200 years now.

[01:28:04]

I think maybe even I should know when it was founded sort of early 19th century, it was set up to basically communicate science to the public.

[01:28:12]

So it's one of the first places in the world where scientists, famous scientists would come and give talks. So very famously, Humphry Davy, who you may know of, who was the person who discovered nitrous oxide, is a very famous chemist and scientists also discovered electrolysis. So he used to do these fantastically, very charismatic speakers who used to peer here. There was a there's a big desk. They usually have it in the theatre. And he would do demonstrations to the sort of the the folk of London back in the early 19th century.

[01:28:40]

Michael Faraday, who I talked about, who is the person who did so much work, electromagnetism, he used he lectured here. He also did experiments in the basement. So this place has got a long history of both scientific research, but also in the communication of scientific research. So you gave a few lectures here.

[01:28:55]

How many to I've given you I've given a couple of lectures in this theatre before.

[01:28:59]

So I mean, that's so people should definitely go watch online. It's just the explanation of particle physics, although it's incredible. Like your your lectures are just incredible. I can't sing enough. So it was awesome.

[01:29:12]

But maybe can you say what did that feel like? What does it feel like to lecture here to talk about that? And maybe from a different perspective, more kind of like how the sausage is made is how do you prepare for that kind of thing? How do you think about communication, the process of communicating these ideas in a way that's inspiring to what I would say your talks are inspiring to the general audience. You don't actually have to be a scientist.

[01:29:42]

You can still be inspired without really knowing much of the you start from the very basics. So what's the preparation process? And then the romantic question is, what does that feel like to perform here? I mean, professionally?

[01:29:56]

Yeah, I mean the process. I mean, the talk that my favorite talk that I gave here was one called Beyond the Higgs, which you can find on the only role institutions YouTube channel, which you should go and check out. I mean, the channels got loads of great talks, a lot of great people as well.

[01:30:09]

I mean, that one I sort of given a version of it many times. So part of it is just practice. And actually I don't have some great theory of how to communicate with people. It's more just that I'm really interested and excited by those ideas and I talking about them. And through the process of doing that, I guess I figured out stories that work and explanations that when you say practice, you mean legitimately just giving just giving talks.

[01:30:31]

And I started off, you know, when I was a student doing talks and schools. And and I still do that as well some of the time and doing things. I've even done a bit of standup comedy, which was sort of went reasonably well, even if it was terrifying. And that's on YouTube as well. That's also I would I wouldn't necessarily recommend you check that out.

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That's going to post the links several places to make sure people click on it.

[01:30:51]

Yeah, but it's basically I kind of have a story in my head. And I was you know, I kind of I have to think about what I want to say, usually have some images to support what I'm saying. And I get up and do it. And it's not really I wish there was some kind of I probably should have some proper process.

[01:31:05]

This is very it sounds like I'm just making up as I go along and I sort of oh, I think the fundamental thing they said, I think it's like I don't know if you know who a guy named Joe Rogan is. Yes, I do it. So he he's also kind of sounds like you in a sense that he is not very introspective about his process, but he's an incredibly engaging conversationalist. And I think one of the things that you and him share that I could see is like a genuine curiosity and passion for the topic.

[01:31:39]

I think that could be systematically, you know, cultivated. I'm sure there's a process to it. But you come to it naturally somehow. I think maybe there's something else as well, which is to understand something. There's this quote by Feynman, which I really like, which is what I cannot create. I do not understand. So like, I'm not I'm not particularly super bright.

[01:31:59]

Like, so for me to understand something, I have to break it down into its simplest elements and that, you know, and if I can then tell people about that, that helps me understand it as well. So I've actually I've learned a lot to understand physics a lot more from the process of communication because it forces you to really scrutinize the ideas that you're communicating and often makes you realize you don't really understand the ideas you're talking about.

[01:32:22]

And I'm writing a book at the moment, and I had this experience yesterday where I realized I didn't really understand a pretty fundamental theoretical aspect of my own subject. And I had to go and spend a couple of days reading textbooks and thinking about it in order to make sure that the explanation I gave captured the got as close to what was actually.

[01:32:41]

Happening in the theory, and to do that, you have to really understand it properly and then there's layers to understanding. It seems like the more there must be some kind of Fineman law, I mean, the more you the more you understand sort of the sympathy you're able to really convey the, you know, the the essence of the idea. So it's like this reverse the reverse effect. That's like the more you understand, the simpler the final thing that you actually convey.

[01:33:13]

And so the more accessible somehow it becomes. That's why Fineman's lectures are really accessible. It was just counterintuitive. Yeah. Although there are some ideas that. Are very difficult to explain how well or badly you understand, like, I still can't really properly explain the Higgs mechanism.

[01:33:33]

Yeah, because some of these ideas only exist in mathematics, really. And the only way to really develop an understanding is to go, unfortunately, to a graduate degree in physics. But you can get kind of a flavor of what's happening, I think.

[01:33:49]

And it's trying to do that in a way that isn't misleading, but was also intelligible.

[01:33:53]

So let me ask then the romantic question of what do you is the most perhaps an unfair question? What is the most beautiful idea in physics? One that fills you with or is the most surprising, the strangest, the weirdest. There's a lot of different definitions of beauty, and I'm sure there's several for you. But is there something that just jumps to mind that you think is just especially. I mean, wow, beautiful. There's a specific thing in a more general thing, so maybe the specific thing first, which I can come across as an undergraduate, I found this amazing.

[01:34:30]

So this idea that the forces of nature, electromagnetism, the strong force, the weak force, they arise in our theories as a consequence of symmetries.

[01:34:41]

So symmetries in the laws of nature, in the equations essentially that used to describe these ideas, the process whereby theories come up with these sorts of models, as they say, imagine the universe obeys. This particular type of symmetry is a symmetry that isn't so far removed from a geometrical symmetry like the rotations of a cube. It's not you can't think of it quite that way, but it is sort of a similar sort of idea. And you say, OK, if the universe respects the symmetry, you find that you have to introduce a force which has the properties of electromagnetism or different symmetry.

[01:35:15]

You get the strong force or different symmetry, you get the weak force. So these interactions seem to come from some deeper. It suggests that they come from some deeper symmetry principle. I mean, depends a bit how you look at it, because it could be that we're actually just recognizing symmetries in the U.S. But there's something rather lovely about that. I mean, I suppose the biggest thing that makes me wonder is actually if you look at the laws of nature, how particles interact when you get really close down, they basically pretty simple things.

[01:35:41]

They bounce off each other by exchanging, you know, through force fields and they move around in very simple ways. And somehow these basic ingredients, these few particles that we know about in the forces creates this universe, which is unbelievably complicated and has things like you and me in it and, you know, the earth and stars that make matter in their cause by from the gravitational energy of their own. Bulc that then gets sprayed into the universe that forms other things.

[01:36:05]

I mean, the fact that there's this incredibly long story that goes right back to, you know, the can we can take this story right back to, you know, trillionth of a second after the big bang. And we can trace the origins of the stuff that we're made from and are all ultimately comes from these simple ingredients with these simple rules. And the fact you can generate such complexity from that is really mysterious, I think, and strange. And it's not even a question that physicists can really tackle because we are sort of trying to find these really elementary laws.

[01:36:35]

But it turns out that going from elementary laws and a few particles to something even as complicated as a molecule becomes very difficult. It's like going from molecule to a human being is a problem that just, you know, can't be can't be tackled, at least not at the moment.

[01:36:50]

So, yeah, the emergence of complexity from simple rules is so beautiful and so mysterious. And there's no we don't have good mathematics to even try to approach that emergent phenomena. That's why we have chemistry and biology and all the other subject.

[01:37:07]

Yeah, I don't think I don't think there's a better way to end it. Harry, I can't. I mean, I think I speak for a lot of people that can't wait to see what happens in the next five, 10, 20 years. Do I think you're one of the great communicators of our time? So I hope you continue that and I hope that grows. And definitely a huge fan. So it was an honor to talk to you today.

[01:37:30]

Thanks so much.

[01:37:31]

Thanks very much. Thanks for listening to this conversation with Harry Cliff and thank you to our sponsors Express, VPN and Kashyap. Please consider supporting the podcast by getting Express VPN and Express Report.com Flex Pod and downloading cache app and using Culex podcast. Enjoy this podcast. Subscribe on YouTube, review it with five stars, an Apple podcast supporter and patron, or simply connect with me on Twitter, Àlex Friedemann. And now let me leave you with some words from Harry Cliff.

[01:38:06]

You and I are leftovers, every particle in our bodies is a survivor from an almighty shootout between matter and antimatter that happened a little after the Big Bang. In fact, only one in a billion particles created at the beginning of time have survived to the present day. Thank you for listening and hope to see you next time.