In Our Time - Higgs Boson

Episode Date: November 18, 2004

Melvyn Bragg and guests discuss the Higgs Boson particle. One weekend in 1964 the Scottish scientist Peter Higgs was walking in the Cairngorm Mountains. On his return to his laboratory in Edinburgh th...e following Monday, he declared to his colleagues that he had just experienced his 'one big idea' and now had an answer to the mystery of how matter in the universe got its mass. That big idea took many years of refining, but it has now generated so much international interest and has such an important place in physics that well over one billion pounds is being spent in the hope that he was right. It's the biggest science project on Earth; the quest to find the 'Higgs Boson', a fundamental constituent of nature that - if it does exist - has such a central role in defining the universe that it's also known as the God Particle.What is the Higgs Boson? Why is it so important to scientists and how are they planning to find it?With Jim Al-Khalili, Senior Lecturer in Physics at the University of Surrey; David Wark, Professor of Experimental Physics at Imperial College London and the Rutherford Appleton Laboratory; Professor Roger Cashmore, former Research Director at CERN and now Principal of Brasenose College, Oxford.

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Starting point is 00:00:57 I hope you enjoy the program. Hello, one weekend in 1964, the Scottish scientist Peter Higgs was walking in the Cairn Gorn Mountains. On his return to his laboratory in Edinburgh the following Monday, he declared to his colleagues that he'd just experienced his one big idea, and now had an answer to the mystery of how matter in universe got its mass. That big idea took many years of refining, but it's now generated so much international interest and has such an important place in physics that well over one billion pounds is being spent on a collided. in CERN in the hope that he was right. It's the biggest science project on Earth.
Starting point is 00:01:33 The question to find the Higgs boson, a fundamental constituent of nature, that if it does exist, has such a central role in defining the universe that it's also known as God's particle. What is the Higgs boson? Why is it so important to scientists and how they're planning to find it?
Starting point is 00:01:48 With me to voyage into the quantum realm of the Higgs boson is Professor Roger Cashmore, the former director of research at CERN and now principal of Brazener's College Oxford. David Wock, Professor of Eighty experimental physics at Imperial College London and the Rutherford Appleton Laboratory, and Jim Alcalili, Senior Lecture in Physics at the University of Surrey. Jim Alcalili, before we start, why is this quest so important, just as it were a headline?
Starting point is 00:02:14 Well, I think ever since the ancient Greeks, we've been trying to understand the fundamental building blocks of everything in the universe. And we've come a long journey, and we've reached a stage now where we believe we know pretty much what everything is made of, the very constituents of all matter in the universe. But we're missing one or two pieces in the jigsaw, and we've got to this point where we're just waiting to be able to complete our picture of fundamental particles. What is the fundamental particle? Well, basically, it's an entity which isn't itself
Starting point is 00:02:49 composed of anything more basic. It's the most basic constituent of matter. So it's a basic building block of everything around us, this table, us, everything around us, everything around. That's right. And I think the very first fundamental particles to be discovered was, of course, the electron back in the end of the 19th century. And since then we've been discovering more and more particles. Some of them we've then discovered that are themselves made of more constituent pieces. We think we know what most of those constituent pieces are now, but there are still one or two gaps in our understanding. So there's a standard model of particles, isn't there, but there is this key missing gap which is going to be filled with. That's right. The standard model. is our best understanding of the particles that make up all of batter in the universe
Starting point is 00:03:33 and the forces between them. And it categorizes particles into groups and families, these fundamental particles. It's still rather strange to get your mind around, these particles, things we can't see, and most people actually make up everything that can be kicked, as it were, and look at it now. How do you find dealing with that, actually? Is it an active imagination all the time? I think many non-scientists would think that. They would see physicists suggesting that a particle would exist,
Starting point is 00:04:00 and then they go away, and lo and behold, they'd find it in an experiment. But science doesn't work that way. There are so many checks and verifications necessary to prove that a particle exists. Can you tell us of the families of particles briefly? What are these fundamental particles? Well, there are two categories. There are the particles of matter, known as the fermions, and then there are particles that somehow mediate the force
Starting point is 00:04:26 between these matter particles of the fermions, and those are called bosons. And there are a number of particles in each category. They're subdivided into other groupings and families. So we have quarks and leptons and bosons. Quarks and leptons are both the matter particles that make up everything, make up atoms, make up all of us and the universe.
Starting point is 00:04:47 The bosons are the particles of force that are exchanged between the matter particles. David, let's talk you about leptons, first of, Can you give the listeners some idea of how small they are, and then more importantly, what function they play? Okay, well, as for how small, this is in one of those concepts, which doesn't actually work very well when you start talking about fundamental particles. We don't usually think of a fundamental particle being like a marble that has a hard surface
Starting point is 00:05:21 and therefore a very well-defined size. particles have properties of particles. They carry discrete amounts of energy, for instance, but they also have the properties of waves. And if you look at a particle in great detail, what you find are the wave-like properties. And, of course, a wave doesn't have as well-defined as size. How do you look at a particle?
Starting point is 00:05:42 Well, mostly by bouncing off other particles off of it. Now, this might sound, you know, circular, but you can actually do this by producing beans of particles either in accelerators or nature produces particles for us in many cases. And you can then detect these particles using detectors, which mostly rely on the fact that some of the particles carry electric charge. So as they travel through these detectors, they will leave a detectable signal, either light or heat or ionization.
Starting point is 00:06:16 And so by taking a well-defined set of particles which we produce and then bouncing them off another set of particles, we can understand the properties of both. So by smashing things up, you find the smallest thing. Yes, Wolfgang Ponovsky once said it was like taking two watches and smashing them together at hundreds of miles an hour and trying to figure out how a watch works by looking at the bits that fly off. It might sound a bit silly, but it's the best way we found so far.
Starting point is 00:06:40 So what is a lepton doing all this, given that it's so important to us as we're talking now. We're full of leptons, and what is a lepton doing? Okay, well, leptons, leptons, the word is, just comes from the Greek word for light. And they're named that because the first lepton found, the electron, is much lighter than the other particles which were known at the time, which were protons and neutrons, which we now don't believe to be fundamental particles.
Starting point is 00:07:08 The leptons, there's only six of them. There are the three charged leptons, the electron, the muon, and the tau. And then there are three neutrinos that go along with them. The very puzzling thing we don't understand is why there are three. okay the muon and the tau are much heavier than the electron but otherwise seem to have the same properties so we have these three so-called families these three copies of the particles and we don't know why there are three have you any idea why i think the three well i'm a poor i'm a poor dumb experimentalist you know it's a theorist job to do that but one one speculation one one one uh reason you might think there are three is we know that in order to get the universe that we see, the laws of physics have to be different for particles and antiparticles,
Starting point is 00:08:01 and also the laws of physics have to be different for time going forward and time going back. Now, we know ways to generate such differences, but you have to have three generations of particles before you can do that. So there is an anthropic principle argument that states that three is the smallest number of particles you can have and make a universe like what we see, the smallest number of families you can have and make a universe like what we see. It's also the smallest number of family you can have, isn't it?
Starting point is 00:08:30 No, no. I personally, I think that why there are three and not two or four is one of those mysteries that we hope to solve by understanding physics beyond the standard model. Still on the fundamental particles, Robert Cashmore, people have heard of quarks,
Starting point is 00:08:49 partly because it's such a lovely word. Can you tell us what they are and how they relate to leptons? Well, as you heard a few moments ago, Dave mentioned protons and neutrons, and once upon a time they were thought to be fundamental particles as well. But in the 50s and 60, we start to find a plethora of particles, and clearly that wasn't the answer. And what grew up then was the idea that these protons and neutrons, which had many properties in common, but some different,
Starting point is 00:09:19 could be made up of some other particles, and these were the quarks that Gelman and George Zweig invented. And you can construct... You said invented rather than discovered. I know they have the same meaning, but it's interesting you chose invented. They thought of it rather than found it. Well, they had patterns of particles.
Starting point is 00:09:41 So it's a bit like having a Lego that you're going to put together to make up different shapes. And we had the order when I started my... life in particle physics the order of 50 to 100 fundamental particles so we thought they were there was obviously but they came in patterns and gell man was one of the first people to recognize this pattern and then said once you get a pattern in science there's probably something else underneath the pattern that produce it for you and that was where the idea of quarks came from he and george vike produced that idea and then you could start with just three quarks make up protons
Starting point is 00:10:18 neutrons and many of the other particles that we see today. And that was a great step forward. But I remember when it was first invented, and people thought this was just a simple way of trying to do complicated mathematics. And it was peeled to me because I was able then to understand what was going on. But it took a long while before people really believed that these quarks were there. And one of the ways that that happened was in the late 60s. there were experiments that were being done in California at Stanford
Starting point is 00:10:51 where you scattered the electrons, the things that Dave had been talking about, off a proton, and it looked as though from those experiments, the actually electron was scattering off little granular objects inside the proton. So the idea that there were really quarks locked up inside a proton, and then they produced the patterns of all the other particles, were then starting to be really accepted. So you've got the leptons and we've got the quarks. We're in fundamental particles.
Starting point is 00:11:18 We're convinced these are fundamental, I mean there's not going to be more fundamental inside these fundamental particles. You see, you're never sure. You're never sure. We're an experimental scientist. I mean, you go and look at the world around you and you see things that are there. We have this one thing where we have the patterns. We have these three families.
Starting point is 00:11:35 We have three families of leptons that Dave was talking about. We also have three families of quarks. and then that's one made of an up and a down quark, another one made of a charm and a strange quark, another one of a top and a bottom quark. Now, when you see things being replicated this way, any physicist says, is there something else going on deep down underneath or not?
Starting point is 00:12:00 At the moment, we can't see that they're made of anything themselves, following the same sort of idea, but who can tell? So we're still talking about the building blocks, so the listeners are everything in existence are coming from these things that we can't see and we can see traces of them after massive experiments. So we've got the leptons. We've got the quarks, and then we come to the barisons.
Starting point is 00:12:25 Right. Can you just tell us what they are first? Well, you have the question of, as Jim said earlier, of how these particles, let's take the quarks, hold together inside a proton. If I said there were two up quarks inside a proton and a down cork, the up quarks carry charge, and the natural inclination of them is to repel one another. So what we have to do is come up with another force
Starting point is 00:12:53 that will hold these things together. We'll beat that repulsion. Now, all of these forces we think of as being mediated by bosons, the carriers of these forces, and that's where the bosons come in. They give the quark and the leptons mass. They carry a force. They carry a force, but they carry the forces that are the interactions between.
Starting point is 00:13:16 We haven't got to the mass of the leptons. That was the big problem. So we didn't know how they got their mass, these fundamental particles. There they were. There were fundamental particles, and the easiest way to do with them was by calling them zero, but you knew they also had mass. But where did the mass come from?
Starting point is 00:13:31 Exactly. I mean, that was the great conundrum that people faced when Higgs came up with his idea, because many of people, Salam, Weinberg, Glashow, have got Nobel Prize for unifying some of these forces that we observed. But you mind all the particles to be massless. And that was Higgs' great triumph, us to go away and come back with an idea of how to give them some mass.
Starting point is 00:13:56 It is wonderfully romantic that a man goes for a walk on the Scottish Mountains and comes back on Monday and actually realizes that his head is one good idea. And then 40 years later, you were spending billions and billions of dollars trying to prove what he discovered on top of the cangons one misty morning. So what did he say that is so very, very important? Can we come to the Bezos, Nigel? Yeah, well, Peter Higgs's idea actually comes from another field of physics. We know that when electrons move through a crystal lattice,
Starting point is 00:14:26 they acquire, it looks like they have more mass. Why should they move through a crystal, what they're moving through this crystal lattice for? If electrons are moving through a material for any object, that conducts electricity, say, will allow electrons to move through it. These electrons, because they're moving through atoms with positive charge, if they're positive ions, they will try and slow down the electrons. They're trying to impede their progress through the lattice. And so it looks, viewing this from the outside,
Starting point is 00:14:57 as though the electrons are heavier than they really are. This was the idea that Peter Higgs then borrowed and applied to particle physics. Now the idea, the whole idea in particle physics is that we're trying to understand, unify all the forces of nature, understand hopefully one grand theory that describes all the particles of the whole forces. So right across the universe, from one end the thing called an electron is the same one end as it is at the other end and in the middle as well. That's the one thing. Exactly.
Starting point is 00:15:25 Right. And the thing that Weinberg and Salam and others that Roger mentioned described was how two of these forces of nature fit together. and are really part of one overriding force. Now, the four force of nature, there's the force of gravity, then there's the electromagnetic force, which basically holds us together. It's the force that keeps electrons in orbit around the atomic nucleus. And then there are two other forces which act inside the nucleus of atoms.
Starting point is 00:15:54 And with quantum mechanics throughout the 20th century, we've been able to understand how three of these four forces act. The one that's, the old one out is the force of gravity, and that's what many physicists are working on now. but to describe how these three forces fit within what we call the standard model requires seeing what they have in connection with each other and two of these forces fit together. Now, the problem is that the electromagnetic force comes about through particles exchanging
Starting point is 00:16:26 one type of boson, namely the photon. Another type of force, the weak nuclear force, comes about through exchange of two other types of bosons called the W and Z particles. Now, in the simplest version of the standard model, you would like to think that all these particles have no mass whatsoever. That's a nice, neat, symmetrical picture of nature. But unfortunately, the W and Z particles are heavy.
Starting point is 00:16:54 The photon doesn't have any mass at all. So the problem that Peter Higgs was addressing is how come the W&Z particles are heavy despite the fact that they should in this nice theory look just like photons. And so he invented this field, David. He imagined this field. Now, can you tell us about this field
Starting point is 00:17:11 and what its function is with regard to the other particles? Well, the Higgs field... Which goes right across the universe. That's the field. The field is... It's a big field. He was on a big mountain, but it's a big field.
Starting point is 00:17:22 It's a big field. The Higgs field has a very interesting property, and that is why it has this effect that it can give things mass. The Higgs field has the property that in the ground state, the lowest energy state, we believe that in nature of things tend to gravitate to the lowest energy state, the Higgs field doesn't have a zero value, okay? The lowest energy state with respect to, say, photons is to have no photons at all,
Starting point is 00:17:49 or the lowest energy state with respect to electrons is just not to have any. The lowest energy... You're kind of losing, maybe still, you better go on because we haven't got all that much done, right? Well, the lowest energy state of the Higgs field, you actually have Higgs. is present. The vacuum, the state if you go out far away from any object, has a field of Higgs's. Now as other particles try to propagate through the vacuum, so an electron is just moving along, it sees these Higgs particles, it sees this Higgs field, and it makes it harder to move the electron. The electron has to drag some of this Higgs field along with it, and that gives the electron a mass.
Starting point is 00:18:30 So masses can imagine it as if the Higgs-Busch is magnetizing the particle? Can we use that word with any sense at all? No, I wouldn't have said magnetising. I would have said a sort of analogy of people I think might be familiar with, say, bottles of syrup and water, and if you drop a ball bearing into such a one of those bottles, you'll see it'll fall in a different way when you go down through the bottle. You go down through the water very much more quickly than if the bottle was empty. Sorry, very much more slowly than if the bottle was empty.
Starting point is 00:19:07 And if you went into the glycerine or the syrup, it would go even more slowly. So it's that sort of interaction with the remedium around it, which gives it apparently different properties, different dynamical properties, different properties of mass. So let's just pause here from it. Higgs field is full of this stuff. And it's this stuff, whatever it is, these particles. And the boson is the aquaunties.
Starting point is 00:19:30 which works on other particles, leptons and quarks, coming through and gives some of their mass, and out of that mass eventually comes everything around us at the moment. That's the deal, is it? That's the deal, that's the idea. Good. You've got it. I think something that non-physists have difficulty with is the idea of a field itself, and the simplest example is a magnetic field. It's not something you can see your touch, but you play.
Starting point is 00:20:00 certain objects in that field and they know it exists, they feel its influence. So this Higgs field is something invisible. It pervades the whole of the universe if it exists, but it influences all particles travelling through it. And every force is associated with the field, the electromagnetic field, manifests itself as a particle as the photon. All fields have particles.
Starting point is 00:20:23 Why does the electromagnetic field, why has it to manifest itself as a photon? Why is it to manifest itself as a photon? manifest itself as a third one. This goes back to what I think Dave was saying earlier, that we've now got a place in physics where we know that you have this duality between waves and between particles, so that we don't talk about things as just one or the other.
Starting point is 00:20:49 Electrons, we can see them behaving as wave-like particles and being bent around, de facto around objects. so that we always expect everything to come up in these two guise, these manifestations as a field or as a particle. And so if we want to look for a Higgs field, then we'll also look for a Higgs particle. That's the idea that we have behind it. So we just have to take granted now that there are waves and particles,
Starting point is 00:21:18 this wave system, and this zapping between them are these packages of particles. Absolutely. Does the wave change into a particle, or do they, do they, coexist as words and particles. Well, this is, the way I think about it is that they coexist. Depending on exactly which
Starting point is 00:21:35 situation you're talking about, you use the most convenient description that you've got available to you. For instance, in the case of electromagnetism, if you have electromagnetic waves, which of course, our listeners today are benefiting from electromagnetic waves,
Starting point is 00:21:51 they wouldn't get this broadcast if there weren't electromagnetic waves. But we also know, when the we can get what are called packets of energy, the photons, which set off photomultipliers, which is the sort of experiments that Dave does, he's looking for these photons all the time in photomultipliers from experiments he does,
Starting point is 00:22:10 but they're very important in a lot of other areas of science for medical diagnostics and things like this. Do you want to talk about looking for these particles, looking, as has been said, they're looking for these particles, because people, they're so, very difficult to sort of get any grip or hold on them, and yet they're essential to any understanding
Starting point is 00:22:32 or to the basic understanding of how we've arrived at what we are. I think one can go too far and trying to make these things mysterious. It's only hard to see an electron because it's very small and your eye is very big. But essentially the way that you see an electron is no different than the way you see anything else. You make radiation interact with it. It comes off. For instance, we now have the capability,
Starting point is 00:22:57 to trap and hold a single electron in a trap, scatter radio photons off of it, and detect them. So you can see a single electron by scattering something off it. Now, you can't do that with your eye, because your eye isn't sensitive enough to see a single radio photon. But there's no fundamental difference between the two. You see when you look out in this room and see the walls, you're just seeing light scattering off of the electrons that make up
Starting point is 00:23:26 the material in the wall. So what we do in the case of our experiments is usually we try to make it easier to see a single particle. And we do that mostly by just making the energy very high. If you make the energy very high, then you can get a much greater disturbance off of a single particle. And then you can see it much more easily. Now, in the case of the Higgs,
Starting point is 00:23:53 we have a second reason to try to make the energy very high. which is that you can't make any particle until you put enough energy into the system to produce its rest mass. Okay, Einstein's famous E equals MC squared. In order to make a particle, you first have to put in an amount of energy equal to MC squared. And then you have to put in some more, usually, in order to get the particle to have enough energy that you can pick it up in your detectors. Now, in the case of the Higgs, it gives everything else mass, but in the theory itself, the mass of the Higgs isn't specified. We know it has a mass, but we don't know what it is. is. And so we've had to search for a very long time for the mass, for the Higgs particle, by banging
Starting point is 00:24:33 things together. And what we know is that we haven't done enough yet. We haven't bang things together hard enough yet to actually produce a Higgs boson. How did the Higgs field get that? This has been researching for this program, which has been hard, but a great pleasure. I've come across wonderful phrases, but there is no better phrase than spontaneous symmetry breaking, which is just a wonderful or phrase should be the title of a series of novels, really. Now, then, spontaneous symmetry baking was very important in creating the Higgs field, as I understand it.
Starting point is 00:25:02 Would you like a crack at that, Jim? Yeah, the idea of... It goes back to the idea of symmetry in physics. Now, we know, in sort of common use, language, when we talk about something symmetrical, we mean it looks the same under certain rotations, a mirror image
Starting point is 00:25:18 or something spherical, it's symmetrical, it doesn't change however you look at it. In physics, or even in pure mathematics, symmetry has a more basic meaning. It means certain properties stay the same when you change other properties. One of these properties in this context is the mass of these fundamental particles. The standard models suggest that the simplest version of it suggests that particles should all have zero mass,
Starting point is 00:25:44 and all the forces are somehow the same. But we know that's not the case. We now believe that just after the Big Bang, for instance, the forces were unified. They were all part of one super force. But as the universe expanded and cooled, the forces took on different properties
Starting point is 00:26:03 and the particles took on different properties. But how did this feel, and I wasn't, I mean, obviously, I like the first spontaneous symmetry working, that actually was essential in the creation of the Higgs field, isn't it? Because out of the symmetry, it broke, the symmetry, it broke
Starting point is 00:26:19 spontaneously. Now, how did it break spontaneously? And have we only idea why it broke simultaneously? Because you and maybe Roger takes up as well. Well, there's a nice example of what breaking a symmetry means. If you have a blank piece of paper, it's symmetrical in the sense that you don't know if it's upside down or one side or the other. But as soon as you start writing on it, you break the symmetry because now you have an up and a down, you have a front and a back. So something has to change so that you lose this symmetry. So how did the, what happened to create the Higgs field, Roger?
Starting point is 00:26:54 That's not a small question. It's not a small question at all, in fact, is a question that a lot of people will juggle with for a very long while. I mean, I don't know if I can answer that question, actually, right? I mean, because... Well, describe what it meant then. What it means is that if symmetry breaks down, what do we get instead of symmetry that makes it a Higgs field?
Starting point is 00:27:18 Well, let me say it goes back a little bit to what Dave was talking about. that a little earlier. We expect, as Jim were also saying, that you have a symmetry in any of our interactions. Let me give you another example, just for one way or way so people get an idea. I mean, the standard example of spontaneous symmetry breaking is that you all sit down at a circular dinner table, and there is a plate laid out and on the left-hand side of the plate, there's a fork, on the right-hand side, there's a knife, and then there's a napkin. then you go on then there's a fork then there's a plate then there's a knife
Starting point is 00:27:54 then's a napkin you go all around the table you all sit down for dinner now it's completely symmetrical whether you go left or right the pattern is there as soon as the first person picks up a napkin everybody else has to pick up
Starting point is 00:28:09 the napkin in the same way because otherwise you'll never all of you get napkins or somebody will be left with two so that's an example for something you look completely symmetrical to begin with actually when you're make you move, everything comes out that way. Now, that's the idea, some of the idea
Starting point is 00:28:24 in spontaneous symmetry with the Higgs field, is that you go, once one choice is made, then you get this resulting pattern of particles, and that's the spontaneous symmetry breaking. Right. So, but this is sometime after the Big Bang. The Higgs field, the, they, go on, you tell me. Let me risk a slightly technical example. This is the standard one in textbooks. It's the example of a ferro magnet. Now, if you have a magnet, it's made up of a bunch of atoms, and each atom is a little magnet itself and generates a little magnetic field. Now, that's true of pretty much all atoms, even the atoms in the wood in this table. But all of the atoms in the wood in this table are pointing in different directions, so there's no net magnetic field. What happens
Starting point is 00:29:09 in a ferro magnet is all the atoms line up, and in the process of lining up, they produce an exterior magnetic field, a b-field, a magnetic field, we can see. see outside. And in the process, they break the symmetry. Because if you initially start out with a very hot magnet, so the temperature is enough to randomize the direction of all the magnets, there's no net magnetic field. There's no preferred orientation in space. It's totally symmetric. All directions look the same. As you cool it down, you reach a critical temperature. All the magnets line up. And now there's a specified direction in space. And that spontaneous symmetry breaking generates the magnetic field.
Starting point is 00:29:50 Now, the Higgs does something analogous to that. At very high energies, right, there's no preferred orientation to an internal symmetry of the Higgs field. We don't want to get into that detail. There's no preferred orientation. As you cool it down, it has to pick one direction for this particular parameter, and when it does so,
Starting point is 00:30:08 it actually generates a Higgs field. It generates this non-zero Higgs field that goes all throughout the universe. This is called a phase shift, isn't it, Jim? and they all point the same, and it becomes like a magnet there. Yes, that's right. I think those analogy is very good, that the magnetic field that is produced
Starting point is 00:30:24 when these atoms line up their magnetic fields produces the magnetic field around it in the same way as the universe calls, and the symmetry is broken, it produces the Higgs field. And it's that field then that says that certain particles will behave differently to other particles in the sense that some have,
Starting point is 00:30:42 some are heavy, some have large mass, others have very small mass, or no mass at all. But this is spontaneous in the sense that it happened, as Roger was describing, like somebody, you have to pick up, and you have to see. It's a sudden process, yes, in that sense, it's a phase transition. It's not a gradual thing. And then once it's in that, it could change again, of course.
Starting point is 00:31:03 Could change back again. Well, let's leave it. Well, everything in settles down. Everything settles down. Yeah. But what you'd have to do is inject a lot of energy back into the system to get it up again where it came out. of that
Starting point is 00:31:16 sort of of rest energy position and then it could fall down into another state as
Starting point is 00:31:22 well now we don't think there's enough energy around to be able to
Starting point is 00:31:26 make that to happen so that happened thousands of millions of years ago
Starting point is 00:31:31 and particles went through and mass accumulated but we're still looking
Starting point is 00:31:35 for this wonderful theory the Higgs bos in nobody's seen it
Starting point is 00:31:40 and you were running Cern Roger Cajmore and now can you
Starting point is 00:31:45 just tell us the size of this job to find this particle. How big is the collider? We know masses of money has gone into it. Can you just give us some practical idea of it? Well, okay. The accelerators being built at C,
Starting point is 00:32:01 the large Hadron Collider, the LHC, is being built in a tunnel that housed a previous accelerator at CERM which had a lot to do with the detailed discussion of the Higgs. Maybe I come back to that later. But it's 27 kilometres in circumference. about 100 meters underground, and running through this tunnel,
Starting point is 00:32:22 there will be large number of superconducting magnets, which run with very high magnetic fields in them. Now, the idea of that is, the higher the magnetic field, particles, when they move in a magnetic field, get deflected. So what you're doing is you're deflecting them, so they're going around a circle in this magnetic field. And as they go around this magnetic circle, you give them a kick at regular intervals to increase their energy with electric field.
Starting point is 00:32:51 And as they get more energetic, you need a higher magnet to keep them in the same orbit, and so we keep them going around until we get to very high energies. Then we have some going one way, protons going one way, protons going the other way, and we bring them into collision with the very high energies that we'll be able to achieve with that accelerator. And then you have the detectors to see what happens when this collision. So at each point, it's four points round this ring that being built, big detectors that between them will cost almost as much as the accelerator itself. They're very sophisticated detectors,
Starting point is 00:33:28 and what they're looking for is when the protons collide, or rather the corks that are inside the protons collide with one another, they will potentially have enough energy to put this energy E, into a very small area to produce a large mass. if there's any particle that's around, using again good old Einstein and the equals MC squared. So the idea is that we build an accelerator, which we know must be able to produce particles, get up to sufficient masses that we've got to find the Higgs if the Higgs exists. David, do you end up to that?
Starting point is 00:34:02 Well, the detectors themselves are an incredible piece of technology. If you look at the largest of these, the Atlas detector, It's the size of broadcasting house, essentially, set on its side. And the reason for that is just that we're producing particles of very high energies, and if you want to measure them very accurately, you have to stop them. It requires a huge amount of material to stop them. But this material is the most complex detector, certainly ever built in particle physics. And in addition to that, it sits in this incredibly high radiation environment
Starting point is 00:34:39 near the collision points between the two protons. And so it has to be able to withstand levels of radiation that are even higher than the core of a nuclear reactor. And it still has to work after 10 years of this. So this has been an enormous effort to do this, and it's required thousands of physicists from around the world to build these. They really are an amazing example of physicists from all over the world working together to produce these common goals.
Starting point is 00:35:07 Yeah, if I was to say, I mean, way back in 1982, when we first thought of the Large Hadron Collider, we didn't know how to build the accelerator. It took 10 years to develop the magnets and the technology to be able to build the accelerator. That took us up to about 1990, then we knew we could build the accelerator. Then came the issue, can we build the detectors that will be able to detect the Higgs if it's produced in these collisions? That took about another 10 years, really, to develop the technology to do it. which has really pushed all elements of electronics, sensors and things like this to an unprecedented level. Now we're building it, and we know we can do it.
Starting point is 00:35:47 So it's a good example of people, scientists, setting off an objective to do something, and then achieving it, but it takes a while. And, of course, the reason why there's so much technical difficulty in building these detectors, two reasons, really. One is that, of course, even if we do have enough energy to create, create the Higgs, that's not the only part it was going to be created. We're smashing protons together such high energy that anything that can be produced with that energy through E equals M2E squared will be produced.
Starting point is 00:36:20 And so the big problem is looking through these billions of events that are going on and pulling out the one event that is important that suggests the Higgs exists. The other problem, of course, is that when the Higgs is created, it doesn't hang around for long as a very, very short, lifetime. What's short in your terms? I don't know exactly what the lifetime things, but these are tiny, tiny for fraction, billions of a second.
Starting point is 00:36:45 And the problem is then you don't look for the Higgs particle itself. You look for the decay products of the Higgs, the particles that the Higgs will decay into and it has certain signatures. And that in itself is very, very difficult because, see, what it turns into depends on what mass it
Starting point is 00:37:01 has. And since we don't know what it's mass is, we're not quite sure what we're looking for. So it's a tremendously difficult problem, but on the whole, I think the majority of physicists are nevertheless encouraged that they will find the Higgs sooner or later. Do you see this as a high-risk experiment? So many people who have involved in so much money in cautious contrast with British physicists at the fore, like a gentleman on my right here, so it seems very steady and sensible,
Starting point is 00:37:28 but looked at it from where I'm sitting to spend billions of pounds chasing something you don't know exists and you might not see. Oh, no, no, that's the guaranteed payoff part. If we don't see the Higgs, that would in many ways be much more interesting than to see the Higgs. The standard model is magnificently successful at predicting what it predicts, and magnificently useless at predicting anything else. For instance, when I say that the Higgs gives the mass to all the fermions, you might think that I've now explained the mass of all the forms.
Starting point is 00:38:05 leptons in the quarks. But I haven't really. I said where it comes from, but I haven't said how big it would be. We now know that if you take the lightest of the neutrinos to the heaviest top quark, there's sort of 14 orders of magnitude range in mass there. And the standard model doesn't explain where this 14 orders of magnitude range comes from. In fact, in the standard model, that 14 orders and magnitude creates real problems. It makes, it's very difficult to have a theory where you can have such a huge range of mass and it's stable. And so we think there must be some physics beyond the standard model. There must be something that's explaining these 14 orders of magnitude.
Starting point is 00:38:44 And by not finding the Higgs, we might actually get a better hint as to what that is. Yeah, I mean, let me pick up on that. I mean, it's not such a random activity that we're engaged in. I mean, if we look around at all the particles that we've got at the moment, and the previous accelerators CERN LEP was magnificent in doing this, we've measured them, we've understood how they interact. act with one another. We've got very accurate measurements of lots of the
Starting point is 00:39:09 parameters of, as we call it, the standard model. However, it doesn't work. There's some missing ingredient. That's Mr. Higgs's particle. And it's wonderful if we do a track come up with the Higgs's particle, but we know there's a missing
Starting point is 00:39:25 ingredient, and we know that the experience of the LHC that we will do will break, our fear is break down unless something new comes in. the Higgs particle, possibly. Because it could be something else. I mean, it's experimental science.
Starting point is 00:39:39 You actually don't know the mix of the Higgs is right. Yeah, yes. Until you've seen his experiments are the result? When you're saying your theories will break down, does that mean that the world changes, or you just you change? I mean, there's tables still the table. I mean, your theory is. Exactly, exactly.
Starting point is 00:39:52 We're experimental scientists, so the table still stays there. We still get our observations, but we try to understand how they all relate to one another. And at the moment, they don't relate to one another unless you have a Higgs particle. Is this why it was called the gods particle by one biophysicist colleague of your? Yes, I think there's Leon Leideman, American Nobel Prize winner. Because it's the, as Roger says, it's the missing piece in the jigsaw. We think we know all the fundamental particles that make up the universe,
Starting point is 00:40:21 apart from the Higgs boson. Now, it may well be that even the Higgs itself isn't a fundamental particle. I mean, there are many theories that suggest there's else, something else that we should be looking for. In fact, one theory called supersymmetry suggests that every particle that we know of has another as yet undiscovered partner. It may well be that that's the way our universe works. We simply don't know. The Higgs could be the missing piece in the jigsaw, but then as David says, even if we don't find it, there's a wonderful, different picture that we need to discover.
Starting point is 00:40:53 Yeah, when I say we may not find the Higgs. As Roger says, there's a very, very, very strong indications we have to find something. it just might not have exactly the properties of the Higgs boson in the standard model. For instance, it was mentioned earlier that the Higgs model is related to condensed matter theories. And in condensed matter, there's an analogous thing to the Higgs called the Cooper Pair, and you would never actually find a Cooper pair in nature. It may be that Higgs is a similar thing, that it is a property of the theory that doesn't correspond to an actual particle. and so we may discover when we look at it
Starting point is 00:41:33 that we find some deeper understanding of the theory that doesn't correspond to an actual particle briefly, it's an awfully awful question to ask you to answer briefly about you but when we're talking about Faraday and other scientists and long of them, they're doing experience they're discovering things for the sake of discovering then modern worlds are created out of their discoveries
Starting point is 00:41:52 do you see any, have you any idea of any practical consequences of finding if you do find this, exposed on this God's particle? Other than the fact that we will have understood physics somewhat better and understand how physics works on the world around us perhaps works and can use those ideas and perhaps as we've been hearing move those ideas over into some other area which will have great benefit, I don't think I can honestly. I mean here we're really seeking after what made us, what made us the world around us the
Starting point is 00:42:27 way it is. where did it come from and I think those are great things to go for as well but I think I can't see any of the practical application but you know you should always be worried I mean even Faraday thought that he didn't know quite how he would
Starting point is 00:42:44 discoveries would be used except he said to one, Chancellor, you'll tax it Thank you all very much indeed that was terrific next week we'll be discussing the venerable B from the 8th century thanks for listening We hope you've enjoyed this Radio 4 podcast. You can find hundreds of other programmes about history, science and philosophy at BBC.com.ukuk forward slash radio 4.

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