رونوشت 🔗
1
00:00:06,560 --> 00:00:12,920
So thanks a lot. It's really a pleasure to be here and to talk this morning on the Standard Model and the Large Hadron Collider and the Higgs boson.
2
00:00:14,250 --> 00:00:22,050
So let me begin the first part of my talk to review something that most of you will know about, which is the start of particle physics.
3
00:00:22,270 --> 00:00:28,230
I, in connection with previous lectures of this morning that you have had, so James mentioned the quantum field theory, right?
4
00:00:28,440 --> 00:00:34,830
The standard model is perhaps the greatest success of this very important theory, which is quantum field theory.
5
00:00:35,540 --> 00:00:40,379
So first of all, let me mention that this is really an extremely exciting time to be a particle physicist.
6
00:00:40,380 --> 00:00:44,670
Right? So in the last years, particle physics had to be in the headlines several times.
7
00:00:45,090 --> 00:00:51,749
And this is fully justified by the discovery of the Higgs boson at the Large Hadron Collider in thousand 12 is the most
8
00:00:51,750 --> 00:00:57,930
important discovery in our field in the last 25 years because it completes the extremely successful standard model.
9
00:00:58,290 --> 00:01:03,420
But at the same time, it opens a large number of crucial questions for our field that we need to answer.
10
00:01:04,290 --> 00:01:10,710
And the Large Hadron Collider will play a central role in exploring this high energy frontier for the last for the next 20 years.
11
00:01:12,240 --> 00:01:14,030
So what is this? I'm not a modest I'm not a model,
12
00:01:14,040 --> 00:01:21,870
is the theory which explains a wide variety of microscopic phenomena into a single unified framework, which is quantum field theory.
13
00:01:22,350 --> 00:01:28,080
It describes all elementary particles and their interactions with the only exception of of gravity.
14
00:01:28,620 --> 00:01:33,689
So what is the standard model composed of? First of all, in this matter, right.
15
00:01:33,690 --> 00:01:39,240
It describes a protons and electrons and also other of the particles.
16
00:01:39,540 --> 00:01:42,780
Its content is composed, organised in quarks,
17
00:01:43,680 --> 00:01:49,920
which experience the strong interaction and leptons which they only experience a weak electronics electromagnetic interaction.
18
00:01:50,190 --> 00:01:54,840
There are six quarks. They are called up, down, strange bottom and top.
19
00:01:55,440 --> 00:02:04,590
There are also six leptons, six from the electron familiar with, but it also has two headed counterparts, the new and under and the Lepton.
20
00:02:04,950 --> 00:02:09,420
And also there are three neutrinos which are massless electron neutrino, neutrino and neutrino.
21
00:02:10,080 --> 00:02:15,390
And then there are the interactions which relate these particles among them.
22
00:02:15,630 --> 00:02:26,220
And these forces are governed by the exchange of the so called a force carriers, and that is one force carrier for each of the interactions.
23
00:02:26,730 --> 00:02:29,850
The electromagnetism is based on the exchange of photons.
24
00:02:30,000 --> 00:02:35,310
These you are familiar with the strong interaction, as I will explain, is characterised by an exchange of gluons.
25
00:02:35,670 --> 00:02:41,430
And then the weak force is defined by the interaction, by the exchange of divergence at bosons.
26
00:02:42,120 --> 00:02:46,050
And the last ingredient, which was found only three years ago, was the Higgs boson,
27
00:02:46,350 --> 00:02:53,190
which is really essential because it's the way in which all the particles in this field can acquire mass,
28
00:02:53,190 --> 00:02:56,220
because this mass is forbidden by the symmetries of the Lagrangian.
29
00:02:57,210 --> 00:03:01,080
So let me begin by recalling where all this comes from, right?
30
00:03:01,290 --> 00:03:07,769
So let's go to the early thirties. And after a number of very important discoveries, the electron, the proton,
31
00:03:07,770 --> 00:03:12,980
the neutron and the positron, we have more or less a complete understanding.
32
00:03:12,990 --> 00:03:16,260
I can read the scripture of particle physics. I do have the atom we had.
33
00:03:16,380 --> 00:03:22,560
We understood the atom as composed by atomic nuclei of protons and neutrons, and then of the electron electron layers.
34
00:03:23,040 --> 00:03:26,219
So it seems that more or less things were in place.
35
00:03:26,220 --> 00:03:29,790
Of course they were important questions, but some people thought perhaps there are minor issues.
36
00:03:30,330 --> 00:03:37,649
However, the discovery of the moon of 37, which is a heavier electron, basically was completely unexpected.
37
00:03:37,650 --> 00:03:41,810
Like nobody expected the the moon, as some people put it for that.
38
00:03:41,970 --> 00:03:48,880
Why do we need to have the electron? What does this state in the scheme of things and to make things worse then a plethora of newer,
39
00:03:48,900 --> 00:03:52,979
strongly interacting particles called pions chaos was soon discovered.
40
00:03:52,980 --> 00:04:01,200
So as you can see in this time and here. So by 33 we had the neutron, the positron, but then we had the mean pions cones and then,
41
00:04:01,350 --> 00:04:04,500
you know, a large array of other particles, lambdas, obstinance.
42
00:04:05,070 --> 00:04:10,650
And the question is, can we make sense of this really [INAUDIBLE] situation?
43
00:04:11,430 --> 00:04:14,370
And moreover, many important conceptual questions were left unanswered.
44
00:04:14,490 --> 00:04:19,500
For example, if you have protons together in the atomic nuclei, they have Coulomb repulsion, right?
45
00:04:19,740 --> 00:04:23,729
So they should be atomic nuclei should explode. Why? Atomic nuclei are stable.
46
00:04:23,730 --> 00:04:27,540
What close together protons in the nucleus. What is the origin of weak interactions?
47
Load full transcript
00:04:27,540 --> 00:04:33,150
Which are the life radioactive decays so why we atoms decay radioactively we had no theory to explain this.
48
00:04:34,500 --> 00:04:38,130
Moreover, all these particles are fundamental. They are composite.
49
00:04:38,670 --> 00:04:40,200
They didn't have any structure.
50
00:04:40,710 --> 00:04:49,490
And even more important, which is a suitable mathematical language to describe particle physics is quantum mechanics is something else.
51
00:04:49,500 --> 00:04:55,440
This was not clear to many people. Now, let me begin with the first thing that actually this is quantum quantum electrodynamics.
52
00:04:55,650 --> 00:04:59,820
This was well, this is it is the quantum version of electromagnetism.
53
00:04:59,820 --> 00:05:07,500
So electromagnetism was discovered by many people in the late 19th century, and it describes the interactions of charged particles.
54
00:05:07,500 --> 00:05:10,800
We had exchange of of photons, however,
55
00:05:11,190 --> 00:05:16,829
making sense of quantum thermodynamics so making sense of electromagnetism once we called
56
00:05:16,830 --> 00:05:20,730
quantum mechanics was extremely challenging y because you had to apply multiple infinities.
57
00:05:21,300 --> 00:05:27,870
When we try to compute corrections, quantum corrections to electromagnetism, we encounter infinities and how to deal with these infinities.
58
00:05:27,870 --> 00:05:33,360
What have theoretical thought? The force, which took ten years until the formulation of quantum electrodynamics was achieved?
59
00:05:34,230 --> 00:05:39,330
I'm sure these are very beautiful theory because starting from simple rules, which are called the Feynman rules,
60
00:05:39,630 --> 00:05:44,670
we can compute any terms as an expansion in power based on the weak coupling.
61
00:05:44,760 --> 00:05:47,940
The electromagnetic coupling is basically the electron chatter square.
62
00:05:48,360 --> 00:05:49,410
So these are small number.
63
00:05:49,650 --> 00:05:56,700
So you can compute the leading term and then subsequently add more and more complicated attempts, each of which will be in principle.
64
00:05:56,700 --> 00:06:01,170
It's my of the others. They can achieve an arbitrary position, make computing more and more complicated diagram.
65
00:06:01,530 --> 00:06:06,719
So if I put together all these lines and all these vertices and I do the entire in principle,
66
00:06:06,720 --> 00:06:11,190
I can achieve arbitrary accuracy in any any process and actually some of the most precise.
67
00:06:11,440 --> 00:06:15,760
Nations that we have never done have been done with quantum electrodynamics, for example.
68
00:06:15,940 --> 00:06:20,080
These are quantitative, which is called the anomalous magnetic moment of the moon,
69
00:06:20,440 --> 00:06:24,460
which equity is known to an accuracy better than one part in 1 billion.
70
00:06:24,970 --> 00:06:30,310
Imagine this we can compute something with this incredible precision and attack this with experiment.
71
00:06:30,590 --> 00:06:35,319
It's really a major success of quantum theory. Of course, this is not an easy task.
72
00:06:35,320 --> 00:06:39,190
We'll have to compute extremely complicated diagrams which involve complex interest.
73
00:06:39,550 --> 00:06:43,900
But in principle, starting from these rules, everything else is fully, fully predicted.
74
00:06:45,320 --> 00:06:49,160
Now, what about the poor? How they were just how they were discovered?
75
00:06:49,430 --> 00:06:58,640
Well, in the beginning of the century, there were experiments discovered in internal structure of of atoms.
76
00:06:58,940 --> 00:07:02,749
How this this was discovered. Well, so that was the experiment.
77
00:07:02,750 --> 00:07:10,370
There was a theme, a theme for love of God. And then you had this was bombarded with alpha particles, which basically helium nuclei.
78
00:07:10,730 --> 00:07:15,530
And we looked at a ruler for look at the reflection of this of these of these alpha particles.
79
00:07:15,770 --> 00:07:19,370
Right. And by looking at the scattering angles of these alpha particles,
80
00:07:19,370 --> 00:07:24,590
after interacting with their with atoms, they realised that the atom is not like a pancake.
81
00:07:24,740 --> 00:07:26,270
The atom is really odd.
82
00:07:26,270 --> 00:07:35,240
The all the positive charge is constituting a very small volume, which is the atomic nuclei, and then the electrons are around these nuclei.
83
00:07:35,750 --> 00:07:38,810
So this was, of course, our impressive discovery.
84
00:07:39,290 --> 00:07:43,460
Very interestingly, 70 years later, the very same technique was used to discover quarks.
85
00:07:44,300 --> 00:07:51,930
What did we do? Well, in this case, instead of using alpha particles against atoms, we use very energetic electrons and we bombarded a protons.
86
00:07:51,950 --> 00:07:56,480
Right. And by looking at how the electrons were deflected, whereas when they scatter with a product,
87
00:07:56,750 --> 00:08:03,710
we discovered that in the proton the charge is also point, like it's concentrated in small volumes.
88
00:08:04,010 --> 00:08:09,649
And this what is what led to the discovery of of of quarks in there in the proton by the same
89
00:08:09,650 --> 00:08:13,820
mechanism as the discovery of the atomic nuclei by their in their order for experiment.
90
00:08:14,890 --> 00:08:17,980
Of course, the concept, of course, had been known for a while.
91
00:08:17,980 --> 00:08:27,490
Right. Since it seems since the sixties we had the Constitution Park model, which allowed to describe all the all the others as composed by this.
92
00:08:28,960 --> 00:08:33,190
This. Hypothetical particles, which are called the quarks, like example,
93
00:08:33,490 --> 00:08:39,610
the proton can be understood as as composed by two apart and one network and the neutrons one upward to the quarks.
94
00:08:40,000 --> 00:08:44,170
However, these
works were very peculiar, right? To begin with, they had fractional charge.
95
00:08:44,260 --> 00:08:49,900
So they tell us either two thirds or minus one set. And we have never seen a particle fractional, fractional charge.
96
00:08:50,290 --> 00:08:57,280
So many people was a sceptic and they thought that perhaps this is just a mathematical trick to organise hadrons by physical existence.
97
00:08:57,730 --> 00:09:06,500
However, after the experiments that I mentioned here, people realised that they are able to play a good mathematical description.
98
00:09:06,520 --> 00:09:15,420
They are really they have a physical existence and describe their. The structure of Aladdin's soap with just up down a stretch we could describe.
99
00:09:16,110 --> 00:09:24,240
Essentially all known. No. So again, we had the very interesting surprise winning the 73 to 77.
100
00:09:24,270 --> 00:09:32,930
Two new, heavier quarks were soon discovered, the Champ Quark, with a mass of about 1.5 and the bottom quark with almost about five g.
101
00:09:33,690 --> 00:09:38,370
So this is there in this spot here, you can see that their discovery of their channel.
102
00:09:39,060 --> 00:09:42,900
So how these things were discovered, we had an electron positron collision.
103
00:09:42,930 --> 00:09:46,050
Right. And we've vary the mass, the energy of the collision.
104
00:09:46,500 --> 00:09:48,760
And at some point we see that there's a peak. Right?
105
00:09:49,020 --> 00:09:55,020
This peak is indicating that in this collision there is a particle which has been formed with Hamas around three TB.
106
00:09:55,440 --> 00:10:00,269
This particle was called the jape site, which corresponds to a mass of our time.
107
00:10:00,270 --> 00:10:08,849
And so this was the discovery of the Templars in 73 and there is an even heavier support of 475 times.
108
00:10:08,850 --> 00:10:13,230
The proton mass is it's a single particle which is almost 200 times heavy on the proton.
109
00:10:13,650 --> 00:10:17,340
Had to wait until 1995 to be discovered because it's being so massive.
110
00:10:17,340 --> 00:10:24,860
We need very high energy colliders to be to be able to. To detect it now.
111
00:10:25,400 --> 00:10:28,580
So I've thought about quantum electrodynamics, this activity spectra.
112
00:10:28,580 --> 00:10:34,550
But if I can compute terms because the coupling is small, I can just compute 10% expansion in orders of this coupling.
113
00:10:35,420 --> 00:10:41,719
So this, of course, makes a theory very predictive. I thought my Feynman ephemeris I can draw diagrams for any process.
114
00:10:41,720 --> 00:10:46,460
I can compute the corresponding cross-sections. However, the atoms interact strongly.
115
00:10:46,850 --> 00:10:51,920
Right? The interaction is characterised by if like it's coupling is something which is very strong.
116
00:10:52,430 --> 00:10:59,050
So it seems that the model of QED is of, of affirmative quantum field theory is not applicable and that we need something else.
117
00:10:59,060 --> 00:11:03,110
And people working this are extensions of like a theory or its matrix.
118
00:11:03,650 --> 00:11:11,780
However, a breakthrough came in in 1973 when it was realised that there was a theory that could describe the strong interaction.
119
00:11:12,140 --> 00:11:18,440
At the same time, the attractive theory is called quantum thermodynamics, and quantum computing has a very peculiar feature,
120
00:11:18,440 --> 00:11:22,670
which is the following, which is the strength of the strong interaction.
121
00:11:22,730 --> 00:11:29,420
So this is the value of the QCT coupling as a value, as a function of the energy right in the remains able quantum of series,
122
00:11:29,690 --> 00:11:35,240
the value of the couplings around this with the energy. This is the three romanisation group equations.
123
00:11:35,600 --> 00:11:39,350
Now, if you look at low energies, for example, well below the proton mass,
124
00:11:39,590 --> 00:11:43,970
this coupling is very large and the theory is strong, interacting as all the data suggested.
125
00:11:44,360 --> 00:11:48,890
However, once we look at very high energies, for example, 100 times the proton mass,
126
00:11:49,190 --> 00:11:53,690
the theory becomes quickly weakly coupled because alpha is a small number.
127
00:11:54,170 --> 00:11:56,690
And in this regime, what I'll face is a small.
128
00:11:56,930 --> 00:12:02,900
We can just exactly the same techniques as what QED to do to computer, to compute predictions for physical observables.
129
00:12:03,230 --> 00:12:05,540
And this was verified to very, very high accuracy.
130
00:12:05,540 --> 00:12:13,250
So again, quantitative theory is the right language to describe not only the electromagnetism, but also the strong interaction.
131
00:12:14,450 --> 00:12:20,240
So the strong interaction, say, QED, has the photon. In the case of a you see we have the gluon,
132
00:12:20,480 --> 00:12:28,790
which is the particle that made this interaction and is responsible of binding together the quarks in there in the proton.
133
00:12:28,910 --> 00:12:34,400
And this you can understand that easily. So we see that the strong interaction is something that the coupling but also with the energy.
134
00:12:34,490 --> 00:12:41,690
Right. We know that even in quantum mechanics growing with the energy, so it's more energy to correspond to larger distances.
135
00:12:41,930 --> 00:12:45,140
Now, imagine they have two quarks and they have they are very close together.
136
00:12:45,590 --> 00:12:48,860
If they are close, it corresponds to basically large energies.
137
00:12:49,160 --> 00:12:53,209
So the copying is small, but if I tried to pull them together, so I pulled them apart.
138
00:12:53,210 --> 00:12:58,640
Sorry, their distance will increase. At this point, these correspond to lower energies and they will become a strong.
139
00:12:59,060 --> 00:13:06,010
So the fact that the
coupling is large is large. A small energies for large distances implies that we cannot have quarks isolated.
140
00:13:06,020 --> 00:13:08,960
They will always be bound together because this coupling is very large.
141
00:13:09,500 --> 00:13:17,470
Now, the gluon was also discovered but also verified experimental its existence in 1977 and this is called three jet events.
142
00:13:17,480 --> 00:13:21,710
So the theory of the strong interaction predicts that if we collide electrons and positrons,
143
00:13:22,040 --> 00:13:27,560
some of the events that we will see in our detector will have kind of mercedes's shape.
144
00:13:27,830 --> 00:13:32,360
You have to quirks here. And then there's a gluon recoiling and this is exactly what was seen.
145
00:13:32,360 --> 00:13:35,240
So this would be awkward yet quartette the yet.
146
00:13:35,570 --> 00:13:42,080
So again this provided an extra evidence that electricity was the right theory for the strong for the strong interactions.
147
00:13:42,770 --> 00:13:47,270
Now going to the interactions with interactions are something that was having known for
148
00:13:47,270 --> 00:13:52,400
a while because it's allowed to explain the idea of metallic metallic of of nuclei.
149
00:13:52,970 --> 00:13:58,280
Now, in the 1930s, Fermi explained the metallic of nuclei by full body interaction.
150
00:13:58,960 --> 00:14:08,060
So basically you have a neutron and these news on the case into a proton and neutrino and the electron in out for body interaction.
151
00:14:08,270 --> 00:14:15,620
So therefore the atomic number of this nucleus would change by what one unit as modified in better metallic experiments.
152
00:14:16,250 --> 00:14:20,780
So it seems that these are also very different from the strong, from the it from QED, right?
153
00:14:21,120 --> 00:14:23,120
Yeah. There is no particle mediating this force.
154
00:14:23,600 --> 00:14:28,700
So what's it is possible to describe the weak interaction in the framework of this quantum field theory?
155
00:14:29,270 --> 00:14:30,200
And the answer is yes.
156
00:14:30,440 --> 00:14:37,040
And the point is that as opposed to the blue one and the photon, which has no mass, they are massless the carriers of the weak interaction,
157
00:14:37,250 --> 00:14:44,060
which are the WS and their bosses, they have a very massive they have a mass of almost 80 GBPS, so 80 times the proton mass.
158
00:14:44,750 --> 00:14:52,730
Therefore, if you look at weak interactions at low energies, you would never resolve the mass with just a point interaction as once you hear.
159
00:14:53,000 --> 00:14:54,350
But if you go to very high energy,
160
00:14:54,440 --> 00:15:00,500
you will see that actually there is a particle propagating like just like the photon or it, but that is very massive.
161
00:15:00,950 --> 00:15:05,630
So in the standard model, the weak interaction of Fermi can be seen as here.
162
00:15:05,660 --> 00:15:09,320
So we have this ah neutron composed down, up, down.
163
00:15:09,590 --> 00:15:17,360
These are proton composite, right down, up, up. And then the down emits the larger you boson so transforms into an output and it will
164
00:15:17,360 --> 00:15:22,880
give us some indication for the electron unable to do so exactly as s as Fermi had.
165
00:15:23,540 --> 00:15:27,200
But now in the context of that, nobody is able quantum theory.
166
00:15:28,200 --> 00:15:33,930
So also in this in the seventies, the fact that this theory was the right explanation of the interactions was verified.
167
00:15:34,350 --> 00:15:38,340
So, for example, the discovery of neutral currency neutrino scattering.
168
00:15:38,700 --> 00:15:47,460
So you have high energy beams of neutrinos which you point to some target, and then you try to reconstruct the results of this collision.
169
00:15:47,940 --> 00:15:52,919
Now, one of the predictions of this was that the neutrino there would be neutral patterns in the sense
170
00:15:52,920 --> 00:15:58,110
that the neutrino will interact via the neutral particle that and then hadrons would be formed,
171
00:15:58,110 --> 00:16:06,480
but no other charge that happens. So these the neutrino these are the traces of the of the evidence for the collision, but there's no charge at level.
172
00:16:06,750 --> 00:16:13,660
So you have neutral currents. And then you also mentioned that the analysis of this kind of images was done among other places.
173
00:16:13,860 --> 00:16:19,770
Know what we are speaking now, which had a crucial role in the discovery of that of the neutral currents.
174
00:16:21,520 --> 00:16:25,850
So we have seen the electromagnetism, the strong interaction and the weak interaction.
175
00:16:26,050 --> 00:16:29,170
What is the only missing piece? This is the the Higgs mechanism. Right.
176
00:16:29,650 --> 00:16:33,720
So what's the problem? Well, Julia will talk much more about this.
177
00:16:33,740 --> 00:16:41,680
Let me just explain it briefly. So the problem is that in the standard model, its symmetries don't allow to have mass in the Lagrangian.
178
00:16:41,770 --> 00:16:44,470
Right. So in particular, we have a electroweak.
179
00:16:45,370 --> 00:16:53,230
A Electroweak theory has a asymmetry between left handed and right handed particles, which for beat the particles.
180
00:16:54,730 --> 00:17:02,170
So what is the Higgs mechanism? These are very clever trick to bypass the restriction, because in the Higgs mechanism the laws are still symmetric.
181
00:17:02,410 --> 00:17:05,680
But the configuration that nature has chosen is not symmetric. Right.
182
00:17:06,010 --> 00:17:09,130
Is this is the famous Mexican hat potential.
183
00:17:09,280 --> 00:17:12,850
Right. If you look at this potential, this potential exploitation, asymmetric, right.
184
00:17:13,150 --> 00:17:20,720
Any direction looks the same. However, the point where the Higgs field just has to be is not is not traditional
185
00:17:20,770 --> 00:17:25,180
symmetric is just one point of all the possible end points of the of the minima.
186
00:17:25,630 --> 00:17:28,900
So these are spontaneously symmetric breaking that laws asymmetric.
187
00:17:29,230 --> 00:17:32,800
However, the specific configuration of the vacuum is not.
188
00:17:33,720 --> 00:17:38,760
So it's actually a mechanism that all the particles in the standard model can operate en masse.
189
00:17:39,600 --> 00:17:45,180
And it's a crucial product. If the energy of interaction is high enough, we can excite the Higgs field.
190
00:17:45,600 --> 00:17:49,450
And excitations of this Higgs field are the Higgs particle which can be produced.
191
00:17:49,470 --> 00:17:53,010
And that's the ultimate test, that this explanation is the right one,
192
00:17:53,010 --> 00:17:58,800
that the Higgs mechanism is correct description of the mass, and the model is the discovery of the Higgs boson.
193
00:17:59,520 --> 00:18:02,010
So it was predicted more than 50 years ago,
194
00:18:02,220 --> 00:18:08,940
but it took an impressive and impressive effort from theories that experimentalists to be able to develop the calculations
195
00:18:08,940 --> 00:18:14,940
and the machines to be able to finally vindicate this prediction and was discovered two years ago at the Lateran Collider.
196
00:18:16,320 --> 00:18:19,650
Okay. So this is the standard model. Let me move to the second part of my thought.
197
00:18:20,250 --> 00:18:26,160
How can we explore the high energy frontier? And this is the best machine we have nowadays to explore the frontier.
198
00:18:26,700 --> 00:18:28,020
Is there a Large Hadron Collider?
199
00:18:28,920 --> 00:18:34,800
So, first of all, why do we care about high energy colliders, what they are suitable to explore really nature at the smallest possible distances.
200
00:18:35,280 --> 00:18:43,530
But we know from the Heisenberg Principle this is there was a question here that if we want to prove something which very small resolution,
201
00:18:43,860 --> 00:18:46,490
we need to have a proof which is very energetic. Right.
202
00:18:46,860 --> 00:18:55,680
So if we want to resolve an object to very small scale, we with a particle which is very energetic, if not, it will be impossible.
203
00:18:56,130 --> 00:19:00,600
So a rule of thumb is to convert distances in energies is the following.
204
00:19:00,930 --> 00:19:10,440
If I have a particle with one GV, this corresponds to roughly a distance of a .8.42 ten to the minus time into a matter of 50 metres.
205
00:19:10,440 --> 00:19:19,710
It's called 0.2 pendulums. This conversion sets the energy that we need to more or less use to explore smaller and smaller objects.
206
00:19:19,800 --> 00:19:25,710
Like, for example, a an atom has a length of about 10 to -8 centimetres, right?
207
00:19:26,100 --> 00:19:30,750
So we need energy of the earth at about 2.5 million to exploit a structure.
208
00:19:31,990 --> 00:19:37,420
If
we want to prove the structure of an atomic nucleus, this is an object of about ten to the -40 metres.
209
00:19:37,720 --> 00:19:46,090
We energies of the order of 200 amoebae, which makes sense because these are typical energies which are that are relevant for nuclear processes.
210
00:19:46,570 --> 00:19:55,450
If we want to go to even smaller distances in particular to to prove the structure of the proton, we need a particle has energies in the GBE range.
211
00:19:55,870 --> 00:20:02,890
And this was precisely by the experiments in like a ten GB because this is right energy to be able to resolve the internal structure of the proton.
212
00:20:03,460 --> 00:20:09,970
If we want to go further and explore, for example, if electrons or quarks have a further structure,
213
00:20:10,330 --> 00:20:15,700
then we need to prove energies because a quad is known to have our radius of a smaller than 10 to 16 centimetres.
214
00:20:15,970 --> 00:20:23,770
So with energies of of two TB right. So if we want to reach really the smallest possible distances, there is no other option.
215
00:20:23,950 --> 00:20:28,770
But going to that to these wide the LHC collider that is bring the escape.
216
00:20:29,780 --> 00:20:33,200
No high energy carriers have been around for a while.
217
00:20:33,230 --> 00:20:38,210
Right. The first collider was there, the Lawrence cyclotron in Berkeley.
218
00:20:38,810 --> 00:20:44,180
And as you can see, by the standards that we are now used to, it is just, you know,
219
00:20:44,330 --> 00:20:51,210
it's almost at that point, right, is only 1.5 metres and the energy seems very small at 15 maybe.
220
00:20:51,500 --> 00:20:56,660
But this was really crucial, right? Because this was the first time that in a controlled setup,
221
00:20:56,720 --> 00:21:01,850
you could accelerate particles and restore its results without a with without the collider.
222
00:21:01,850 --> 00:21:07,580
What is the problem? And we want to use we can only use cosmic rays, for example, or, or that natural process.
223
00:21:08,120 --> 00:21:11,540
So we cannot control in detail which are the settings of our collision.
224
00:21:11,540 --> 00:21:14,659
And this is of course not good for extend our point of view.
225
00:21:14,660 --> 00:21:22,459
We want to control everything. And in the case of our cyclotron, we have all the activities that we want to to control the energy of the collisions.
226
00:21:22,460 --> 00:21:26,840
And then these are very clean proof of air. Of our experiment.
227
00:21:27,380 --> 00:21:32,210
So they have many other colliders being built. And then I would just highlight three of them.
228
00:21:32,840 --> 00:21:37,760
One of these is it's like this the Stanford Linear Collider with a length of three kilometres.
229
00:21:37,760 --> 00:21:45,530
This is in in California. And an edge of 98 is a linear collider, which means that I collide electrons with positrons.
230
00:21:45,980 --> 00:21:49,610
These are
very clean experiment. However, it switching energies limited.
231
00:21:50,530 --> 00:21:57,459
There's also the collider in Amber, which was the first and only electron proton collider ever built.
232
00:21:57,460 --> 00:22:05,380
So we have a high energy beam of electrons colliding with a high energy team of protons, the length of six kilometres and the energy of 210 GB.
233
00:22:06,390 --> 00:22:12,840
And then there was the platinum collider in Chicago, which was before the energy was the highest energy collider of the world,
234
00:22:13,110 --> 00:22:16,200
which is a proton collider in a tunnel of six kilometres.
235
00:22:16,200 --> 00:22:23,400
And the energy you have out to TV. Each of these experiments has provided us crucial information of the standard model.
236
00:22:23,910 --> 00:22:30,870
But since a some years, some years ago, we have the Large Hadron Collider really and is an impressive machine.
237
00:22:30,870 --> 00:22:34,890
Right? It's the most powerful accelerator ever built by mankind.
238
00:22:35,190 --> 00:22:40,620
They taught it at CERN in Geneva, which is the sun, is the European Laboratory for particle physics.
239
00:22:41,070 --> 00:22:47,190
So it's composed by a massive 27 kilometre long tunnel with four gigantic detectors in them.
240
00:22:47,490 --> 00:22:51,690
So this is the this is a photo taking of the LHC area.
241
00:22:51,720 --> 00:22:56,640
So this is the Geneva Airport for those of you that nobody at the Geneva.
242
00:22:57,450 --> 00:23:01,080
This is where seven is located. So my office used to be here for three years.
243
00:23:01,470 --> 00:23:06,720
And then underneath all this area, there is a Large Hadron Collider. So these are the SPS.
244
00:23:07,020 --> 00:23:11,570
And then this is the LHC tunnel that goes almost from the airport to the lake.
245
00:23:11,580 --> 00:23:14,880
And then today I'm on the other side of the lake.
246
00:23:16,120 --> 00:23:22,209
And identity of the protons attacks had the highest energies ever approved with the goal,
247
00:23:22,210 --> 00:23:27,370
as I was mentioning, to explore the laws of nature, the smallest distances ever achieved.
248
00:23:28,290 --> 00:23:31,950
So in the LHC there are four massive detectors.
249
00:23:32,280 --> 00:23:35,540
They are called Atlas CMS, satellite TB.
250
00:23:36,120 --> 00:23:42,750
You can see, you know, by comparing with the size of a of a of a person, they are really they're really massive.
251
00:23:42,960 --> 00:23:48,030
They are like six, seven, eight story buildings of an amazing technology.
252
00:23:48,540 --> 00:23:53,580
I'm always impressed that these things even managed to work. Right. You have something which is huge as a building.
253
00:23:53,610 --> 00:23:57,899
Everything wires and detectors. And, you know, it manages to work on two quite impressive measurements.
254
00:23:57,900 --> 00:24:01,020
I think that's the technological is an impressive achievement.
255
00:24:01,770 --> 00:24:09,059
So I say, well, I also wanted to mention that Oxford has played the central role both in building
256
00:24:09,060 --> 00:24:13,470
these detectors and now in operating them and extracting the most of that information.
257
00:24:14,250 --> 00:24:16,050
The galaxies are an impressive machine, right?
258
00:24:16,260 --> 00:24:23,440
But without its detectors, which are able to explore, you know, and able to extract information from the collisions, then it would be useless.
259
00:24:23,460 --> 00:24:26,820
So we thought the detector, having very energetic protons, is not very useful.
260
00:24:27,660 --> 00:24:32,610
So let me show how articulation looks like. So these are nice video done by their Atlas collaboration.
261
00:24:33,120 --> 00:24:41,260
So this is the LHC tunnel. Right. So here you have there we have that protons, which are actually a very, very high energies.
262
00:24:42,000 --> 00:24:48,030
Right. So let's go inside the beam. This is the proton composed by in this video by three quarks.
263
00:24:48,540 --> 00:24:51,569
And the proton is six and eight of them. At some point the beams will cross.
264
00:24:51,570 --> 00:24:55,410
Right, and they will cross in the interaction points whether that they are located.
265
00:24:55,680 --> 00:25:00,210
So we have their proton beams, they get close to each other, and then eventually they collide.
266
00:25:01,050 --> 00:25:10,530
And what the detector does is by reconstructing the traces of the collision, reconstructing the hadrons, the leptons, the most, the missing energy,
267
00:25:11,070 --> 00:25:18,690
that the aim is to reconstruct what has happened in this interaction point, because this interaction point is that collision of very high energies.
268
00:25:18,930 --> 00:25:23,400
So therefore, here is precisely what we are calling nature at the smallest distances.
269
00:25:25,470 --> 00:25:29,520
So let me mention some facts about the LHC, which I think are quite interesting.
270
00:25:29,760 --> 00:25:35,930
So first of all, LHC is one of the coldest places in the universe in order to keep it in magnets.
271
00:25:36,060 --> 00:25:42,860
So it is based on semiconductor superconducting magnet in order to keep these magnets operating with very, very low temperatures.
272
00:25:42,900 --> 00:25:51,810
So the LHC will have a 30 kilometres tunnel just kept at only two degrees above absolute zero, which is, you know, it's called the interstellar space.
273
00:25:52,790 --> 00:25:56,270
Another interesting fact is this is one of the empty space in the solar system.
274
00:25:56,450 --> 00:26:03,110
Why? Because if in the beam where we have the problems running, there is even a very small density of air particles.
275
00:26:03,410 --> 00:26:09,200
The problem we've had with these particles and we will not be able to explore the in the detector.
276
00:26:09,500 --> 00:26:13,000
So we with really a very, very high vacuum like us.
277
00:26:13,010 --> 00:26:16,050
Another interesting fact is that it's one of the hottest places in the galaxy.
278
00:26:16,100 --> 00:26:20,840
So, for example, when we collide, heavy ions like for example, that in the LHC,
279
00:26:21,200 --> 00:26:27,019
the temperature that we generate is an example of these collisions are billions of times larger than in the sun.
280
00:26:27,020 --> 00:26:30,920
Right. Which is the conditions similar to those in the very, very early universe.
281
00:26:31,910 --> 00:26:40,790
And also a final score. They think it's really impressive is the amount of information that we extract from the LHC in just one second.
282
00:26:41,120 --> 00:26:45,780
The LHC in principle could record one third of out of data just per second.
283
00:26:45,800 --> 00:26:50,750
Right. So this is like having to record 10,000 sets of Encyclopaedia Britannica per second.
284
00:26:51,410 --> 00:27:00,470
So it is it's an impressive technological challenging to be able to efficiently skim all this huge amount of information for the relevant events.
285
00:27:01,490 --> 00:27:06,590
So what bility has has what have we learned fertility up to now?
286
00:27:07,130 --> 00:27:10,730
So the first result has been that rediscovery of this model.
287
00:27:11,090 --> 00:27:18,320
What do you mean by rediscovery? Well, in the previous slides I mentioned the discovery of the deep sea obsidian as a particle.
288
00:27:18,800 --> 00:27:22,580
The very first thing that DDT had to do is to check that everything was still there.
289
00:27:22,820 --> 00:27:27,260
And this might seem obvious, but it is not because this machine is technologically very complex.
290
00:27:27,260 --> 00:27:32,330
So first of all, we have to validate that everything is in place, that the detectors went to the detectors, its performance.
291
00:27:32,720 --> 00:27:36,590
And also, we need to check out our calculations, which have been tested before at lower identities.
292
00:27:37,160 --> 00:27:41,070
Also hold high energies, because we are these are very largely average.
293
00:27:41,190 --> 00:27:46,640
That's increasing the energies. So the in this book here by this collaboration, this is a plot of the.
294
00:27:47,030 --> 00:27:50,720
This is proton proton collisions into the news in this case.
295
00:27:51,290 --> 00:27:56,240
And each time we see a peak, it means that there is a new particle has been produced in this collision.
296
00:27:56,600 --> 00:27:59,989
So, for example, if we look at around three, three gbps, we see a peak.
297
00:27:59,990 --> 00:28:06,629
This is a site discovered in 73. If we look at above at 1022, we see the epsilon.
298
00:28:06,630 --> 00:28:11,930
This is bottom 90, both the mission discovery in 77 and then at around 100 GB that does have mass, right.
299
00:28:12,260 --> 00:28:14,150
It was very nice to see that no ability.
300
00:28:14,330 --> 00:28:20,210
We can quickly rediscover the oldest under model and test our calculation with a very high degree of accuracy.
301
00:28:20,690 --> 00:28:27,139
And this is very important because predicting the standard as well as just passing predicted processes with
302
00:28:27,140 --> 00:28:31,700
very high accuracy could be the key to discover new physical reality in there in the following years.
303
00:28:33,110 --> 00:28:36,890
Of course, the biggest achievement of the LHC has been the discovery of the Higgs boson.
304
00:28:37,220 --> 00:28:44,040
In this video here, I'm showing a collision in which a Higgs boson candidate is being is being formed into four into four leptons.
305
00:28:44,040 --> 00:28:47,629
So each of these four lines is are four leptons,
306
00:28:47,630 --> 00:28:52,520
which is one of the cleanest channels of the production of the K and Julia know talk about this later.
307
00:28:53,180 --> 00:28:59,750
And this is a extremely challenging measurement, right? Because it requires to disentangle a very small signal from of a large background
308
00:29:00,200 --> 00:29:05,450
and to try to to convey the message of how challenging these measurements are.
309
00:29:05,810 --> 00:29:10,820
Let me show you an extended mission by the Atlas collaboration. So how we discovered the Higgs from the practical point of view.
310
00:29:10,850 --> 00:29:14,630
So we begin without any data, right? And we want to measure two things.
311
00:29:14,990 --> 00:29:19,580
One, to measure the masses of default numbers so the Higgs can decay into pairs of photons.
312
00:29:19,850 --> 00:29:25,130
So if we look at beta photons and compute the mass, if we see a peak, that would be a discovery of the Higgs boson.
313
00:29:25,610 --> 00:29:27,380
The same the Higgs can be came to four letters.
314
00:29:27,650 --> 00:29:33,140
So if I compute the mass of four atom events, which is not in this model, will be evidence for the Higgs.
315
00:29:33,650 --> 00:29:38,390
Right. So let me begin to take data. So slowly I began to accumulate data.
316
00:29:38,540 --> 00:29:44,420
But here there's nothing, just a flat line. So just background. But with more and more data, right?
317
00:29:44,720 --> 00:29:48,440
Something will appear. What will appear? There's a structure forming here, right?
318
00:29:49,100 --> 00:29:52,640
And what is this structure? This is a peak around 25.
319
00:29:52,850 --> 00:29:57,350
TV is very interesting because this is this could be the mass of the Higgs boson.
320
00:29:57,830 --> 00:30:02,000
Now, is it really the Higgs boson could be something as a statistical fluke?
321
00:30:02,090 --> 00:30:07,700
Well, what we do is to go to the other process, which is going to four leptons and also big data here.
322
00:30:07,740 --> 00:30:12,170
Right. So I'm taking data in the Higgs into four letters to begin with.
323
00:30:12,320 --> 00:30:16,940
I don't have anything. So I need to more and more data. Everything looks under model no Higgs.
324
00:30:17,360 --> 00:30:24,110
But
eventually there are some events here that hey, they are their mass 125 GV and they are not they are not.
325
00:30:24,110 --> 00:30:26,390
Some said that for example, this could be a Higgs.
326
00:30:26,810 --> 00:30:34,190
And the crucial thing is that this signal here has a peak at exactly the same mass as they're wanting today for the channel.
327
00:30:34,610 --> 00:30:39,860
These are very strong. Check that this feature here, this feature here correspond to the same logic like this,
328
00:30:39,860 --> 00:30:45,680
that the Higgs boson and actually at the at the LHC, these two channels, two forms, four letters.
329
00:30:45,980 --> 00:30:51,140
What are the ones that we are able to proclaim our discovery in July 2012.
330
00:30:52,050 --> 00:31:00,420
So it really this is why after this massive exercise, we can be happy because we found the Higgs boson.
331
00:31:01,600 --> 00:31:08,860
No. Okay. However. Some of our models is an impressive success and we should be really proud of.
332
00:31:08,860 --> 00:31:11,500
It is one of the greatest success of modern science.
333
00:31:12,070 --> 00:31:19,750
However, despite its successes and discoveries, Higgs boson, there are many crucial questions which are still left open.
334
00:31:20,050 --> 00:31:27,280
For example, the stability of the Higgs Mass. Why the Higgs Mass is what it is and not the mass of the mass at very, very high energies.
335
00:31:28,030 --> 00:31:33,579
What is the nature of dark matter or that cannot see those forces unify into a single one?
336
00:31:33,580 --> 00:31:38,290
So our strong interactions with interactions and explanation aspects of the same force or they are not.
337
00:31:38,830 --> 00:31:43,540
Is there a theory of everything? What is the role of gravity? Because the gravity doesn't fit in a standard model, right?
338
00:31:44,230 --> 00:31:46,209
What is the origin of the matter? Anti-matter asymmetry.
339
00:31:46,210 --> 00:31:50,820
So there are many questions which are really crucial that have been not that are left open by another model.
340
00:31:51,610 --> 00:31:58,629
And the interesting thing is that there are many theories that go beyond the standard model, and many of these can be tested at the LHC.
341
00:31:58,630 --> 00:32:06,220
So the LHC is a unique tool to scrutinise these theories, which will try to attempt some of the limitations of the standard model.
342
00:32:07,000 --> 00:32:11,200
One popular example that you might have heard about is called supersymmetry.
343
00:32:11,590 --> 00:32:19,690
So in supersymmetry, each particle has a super partner. So we have talked about quarks, neutrinos, the force carriers and the Higgs boson.
344
00:32:20,110 --> 00:32:27,190
So in supersymmetry, we have the standard model and we have another copy of all the particles with the spin the force by one half.
345
00:32:27,490 --> 00:32:31,450
So you have the force which had us no fermions anymore.
346
00:32:31,900 --> 00:32:40,150
We have this leptons and then we have the the best symmetric version of the case, Boston Dynamics of the Higgs, which is called the Higgs.
347
00:32:40,870 --> 00:32:43,900
And among all the things that have been predictions of supersymmetry,
348
00:32:44,140 --> 00:32:49,030
it predicts that all the free forces are strong with magnetic, if you will, two very high energies.
349
00:32:49,390 --> 00:32:51,120
They become just a single, single force.
350
00:32:51,130 --> 00:32:57,910
So this what is called a force unification, which is, of course, a very attractive theory out of a fundamental theory of nature.
351
00:32:58,480 --> 00:33:02,740
However, as of today, there are no hints of yes in physics ability.
352
00:33:03,190 --> 00:33:08,620
However, in just a few months, data will have started even higher energies and will have ten, 15,
353
00:33:08,620 --> 00:33:15,040
20 years to keep exploring the high energy frontier and try to understand all these pressing and very important questions.
354
00:33:15,490 --> 00:33:21,370
So I think that it is very likely that we have many new breakthroughs and we are on the corner.
355
00:33:23,050 --> 00:33:26,770
Okay. So in the last 5 minutes, I want to mention what's next, right?
356
00:33:27,310 --> 00:33:33,490
What's what's beyond reality? And this is important because in high energy physics, building these facilities,
357
00:33:34,000 --> 00:33:38,080
since it's really at the cutting edge of technology, it takes long timescales.
358
00:33:38,470 --> 00:33:42,790
Right. Both from the civil engineering to a technology to or to the physics,
359
00:33:43,210 --> 00:33:49,030
say something that even if we are only at the beginning of the LHC problem, we have to begin to think what comes next.
360
00:33:49,930 --> 00:33:53,710
So this is the scale of the LHC for the next 25 years.
361
00:33:54,250 --> 00:33:59,709
So I'll say what's amazing, they deliver a huge amount of interesting results, but we are just at the very beginning of the problem.
362
00:33:59,710 --> 00:34:07,810
Right. So we have seen how they can data for three years at seven TV and a TV reality has some that are going along shut down of two years.
363
00:34:08,050 --> 00:34:15,490
And now we are here. We are about at the beginning of day, which is called rental, where the energy has increased from eight TV from 13 to 14 TV.
364
00:34:16,240 --> 00:34:22,330
So there will be a period of about eight years of running for TV and then there will
365
00:34:22,330 --> 00:34:26,709
be a very important upgrade in which the LHC will be turned into the high luminosity.
366
00:34:26,710 --> 00:34:28,390
LHC What's a high luminosity?
367
00:34:28,460 --> 00:34:36,370
It's only the number of collisions per bunch crossing will be increased substantially, so increasing the chances of finding interesting events.
368
00:34:37,690 --> 00:34:42,610
So we have half work for the next 20 years to really try to explore the high
energy frontier.
369
00:34:42,850 --> 00:34:50,950
And the LHC is the best machine that we have for this. And something which is crucial, especially in the lack of any evident signal of BFM theory,
370
00:34:51,400 --> 00:34:59,410
is to try to sharpen our understanding of the weak interactions, electromagnetism, because this would be the key of new discoveries.
371
00:34:59,680 --> 00:35:03,250
New discoveries would appear as a subtle deviation from some normal prediction.
372
00:35:03,520 --> 00:35:09,010
So the better you can compute things with high precision, the closer could be to a new discovery.
373
00:35:09,310 --> 00:35:14,590
At the Large Hadron Collider. And of course, it's essential to have a very close interplay between theory and experiment.
374
00:35:14,590 --> 00:35:20,520
Right. And two of the central ingredients of the LHC program for the next 20 years.
375
00:35:20,730 --> 00:35:25,860
Well, first of all, precision measurements of the Higgs couplings. And Julia will talk about this in her talk.
376
00:35:26,280 --> 00:35:31,140
And then the search for dark matter. The LHC and Woolly again will tell us about this.
377
00:35:32,570 --> 00:35:39,890
So as I was saying in about 2022, we have to upgrade the LHC and turn it into our high luminosity machine.
378
00:35:40,550 --> 00:35:45,330
What's the high luminosity, as it was mentioning, is now in the municipality.
379
00:35:45,380 --> 00:35:52,040
The number of collisions that a bunch of crossing would be much higher, which means that the chances of finding interesting events will be larger.
380
00:35:52,490 --> 00:35:57,770
Of course this has challenges because if you have more collisions, you have more single events,
381
00:35:58,130 --> 00:36:02,150
but also many more background events like these because this looks extremely messy.
382
00:36:02,390 --> 00:36:10,460
We have to extract interesting signal in a in a collision where we have almost 200 collisions, literally a background noise and need to be removed.
383
00:36:11,090 --> 00:36:15,910
So this requires a complete upgrade of the LHC detector.
384
00:36:16,370 --> 00:36:23,090
And also here, Oxford is studying a central role, in particular in the case of Atlas in building the new Atlas Atlas Silicon Tracker.
385
00:36:24,410 --> 00:36:28,820
And so let's try to think even bigger. So what comes in the next 20, 30 years?
386
00:36:29,240 --> 00:36:34,310
Well, as I was mentioning, the planning of these facilities is always an expression of very long timescale.
387
00:36:34,400 --> 00:36:38,750
Right. Because we are at the cutting edge of technology, of civil engineering.
388
00:36:38,960 --> 00:36:42,830
You know, there are problems that these machines are planning the solution.
389
00:36:43,480 --> 00:36:51,100
So we to think we are out of time. So in particular now we are discussing whether the next peak machine would be 100 TV.
390
00:36:51,100 --> 00:36:54,400
Collider So seven times higher than the Large Hadron Collider.
391
00:36:54,880 --> 00:37:03,910
Also, we have electron positron, an electron proton model. This is called tentatively Future Collider and this is the plan of a possible site.
392
00:37:03,910 --> 00:37:07,990
This would be again in Geneva. So is the LHC tunnel.
393
00:37:08,350 --> 00:37:12,430
This would be the 100 kilometre long tunnel where this could be built.
394
00:37:12,540 --> 00:37:19,870
So you see that it's quite impressive that as compared to the FCC, it's very small, despite being an incredibly large machine.
395
00:37:20,590 --> 00:37:26,230
Also sites China is very interested in this kind of projects. And there's a proposal for the FCC in China.
396
00:37:26,860 --> 00:37:29,290
And now in the context of of working groups,
397
00:37:29,290 --> 00:37:35,800
there is a worldwide effort trying to understand both the technical feasibility and the physics motivation of this of this proposal.
398
00:37:36,400 --> 00:37:39,670
There are also other ways that we could explore the hydrogen from the earth.
399
00:37:39,670 --> 00:37:45,940
For example, there are plans to build a linear collider where you have electrons and positron collisions at very high energies.
400
00:37:45,940 --> 00:37:49,030
For example, there is the plan of having click in Geneva.
401
00:37:49,120 --> 00:37:59,050
It would be a linear, linear tunnel that goes from the French part of the French area to almost all given crossing all the Geneva area.
402
00:37:59,680 --> 00:38:04,540
These are cleaner machines because electrons are fundamental constituents, so there is less background noise.
403
00:38:04,870 --> 00:38:08,110
However, they have greatly reduced reduce friction.
404
00:38:08,970 --> 00:38:15,550
In. So I think that I've tried to convey that this is really a fascinating time to be in particle physics,
405
00:38:16,060 --> 00:38:21,459
that this has been an incredibly successful theory and that it will be the
406
00:38:21,460 --> 00:38:25,810
best tool we have to explore the high energy frontier for the next 20 years.
407
00:38:25,810 --> 00:38:29,590
I think that you should really stay tuned for news for the LHC because I'm sure that
408
00:38:29,590 --> 00:38:33,600
there will be very interesting results from us and you will be happy to have them about.
409
00:38:33,710 --> 00:38:35,290
So thanks for your attention.