1 00:00:00,120 --> 00:00:04,530 Okay, thanks. Okay, so good afternoon. So I was asked to give this overview of the 2 00:00:04,530 --> 00:00:12,300 physics case for future hadron colliders. And let me just start by giving a you 3 00:00:12,300 --> 00:00:18,900 know, more more broad general view of what a future project in energy physics might 4 00:00:19,110 --> 00:00:23,940 want to achieve. So, you know, as a first bullet you would like to explore the 5 00:00:23,940 --> 00:00:30,480 energy frontier. And you would like, hopefully to address some of the questions 6 00:00:30,480 --> 00:00:35,370 on physics beyond the Standard Model such as market nuclear mass, and the matter 7 00:00:35,370 --> 00:00:40,050 antimatter symmetry. Of course, no collider experiment, actually, no hype 8 00:00:40,050 --> 00:00:46,110 experiment can hope to answer decisively all of these questions, what you can 9 00:00:46,110 --> 00:00:53,100 answer is yes or no to precise scenarios of such questions. And this is what you 10 00:00:53,100 --> 00:01:02,250 can actually hope for a collider experiment on the other hand, We know that 11 00:01:02,250 --> 00:01:08,580 the Higgs there so we have found it a galaxy. And this is kind of a guaranteed 12 00:01:08,580 --> 00:01:15,330 deliverable if you can prove that your collider can measure very precisely the 13 00:01:15,330 --> 00:01:22,800 parameters of the Higgs potential and Higgs couplings, you have a guaranteed 14 00:01:22,800 --> 00:01:28,500 deliverable. So, what kind of hadron colliders that are on the market. So, as 15 00:01:28,500 --> 00:01:34,740 you will imagine, I will talk mostly about the FCC Ah, I think Daniel shooty later 16 00:01:34,740 --> 00:01:41,400 will give you an overview of all these various options probably with a focus on 17 00:01:41,400 --> 00:01:45,420 the accelerator so I won't discuss them too much here. As I said, I would focus 18 00:01:45,420 --> 00:01:52,440 mostly on the FSH which is a project for 100 TV Collider in 100 kilometer tunnel in 19 00:01:52,440 --> 00:01:58,590 the scenario, so this would be the second step or the first e plus e minus Collider. 20 00:01:59,580 --> 00:02:05,550 That will Be essentially electroweak and Higgs factory. You might know that there 21 00:02:05,550 --> 00:02:11,520 are two other possible options on the tables which are less fashionable. So one 22 00:02:11,520 --> 00:02:16,380 is the energetic shear or you take 16th as a magnet inside the UFC and you get the 27 23 00:02:16,380 --> 00:02:21,060 pt Collider. Another option that came out during the European strategy is a so 24 00:02:21,060 --> 00:02:26,910 called low energy FCC h h, which will have the 100 kilometer tunnel, you fill in with 25 00:02:28,110 --> 00:02:33,870 the cheapest possible magnets you get to 37 TV, and you wait to have the technology 26 00:02:33,870 --> 00:02:38,310 to get on the TVs. In case you don't want to start with any plus or minus Collider. 27 00:02:39,570 --> 00:02:45,900 All of these options are described in various cdrs in European strategy. Now 28 00:02:45,900 --> 00:02:51,810 more precisely 400 TV so this will be my benchmark for for assessing the potential 29 00:02:52,260 --> 00:02:56,760 of a future Hadron Collider. More precisely, you would like to problem the 30 00:02:56,760 --> 00:03:02,100 exact coupling to the percent level, measure percent level precision, the 31 00:03:02,100 --> 00:03:09,330 Tokugawa and second generation so he's tomeo don't talk cetera and measure the 32 00:03:09,330 --> 00:03:13,050 Standard Model parameter with high precision. And of course, what you have is 33 00:03:14,310 --> 00:03:18,750 you really can explore the complementarity with the plus and minus machines because 34 00:03:18,750 --> 00:03:22,890 you can access read case not only for the Higgs but also for you know, some other 35 00:03:22,890 --> 00:03:30,750 processes. And also you have access to high dimensional parameters in unity. To 36 00:03:30,750 --> 00:03:34,710 extend kinetic regime which you don't have any plus or minus, at least in circular 37 00:03:34,710 --> 00:03:39,690 collider where you have limited amount of energy is not Rothko's, for clinical 38 00:03:39,690 --> 00:03:46,620 either way, you can also higher energy and neon collider even more and on the other 39 00:03:46,620 --> 00:03:51,210 hand, you know, if you're caught onto TV, you want this machine to be discovered a 40 00:03:51,210 --> 00:03:56,220 machine is why you're caught for such high energy because you're no you're your 41 00:03:56,220 --> 00:04:03,150 discovery potential in principle goes up by a factor 700 divided by 14. And in 42 00:04:03,150 --> 00:04:06,330 fact, your targets will be known for you for this kind of math, very heavy 43 00:04:06,330 --> 00:04:14,580 resonances in the range of 4050. TV for soaz 20, stops and 15. And what you can 44 00:04:14,580 --> 00:04:19,410 see here is that, you know, it's very similar to get in the sense that the 45 00:04:19,410 --> 00:04:24,420 physics problem program spans over a fairly wide range of characteristic energy 46 00:04:24,420 --> 00:04:29,970 scales, but even more so, because you still want to measure stuff at the hundred 47 00:04:29,970 --> 00:04:36,450 gv electroweak scale. But on the other hand, you also want to go possibly almost 48 00:04:36,450 --> 00:04:42,420 an order of magnitude higher in energy to discover new states. 49 00:04:43,740 --> 00:04:50,400 Just some very naive characterization of what physics collision will look look like 50 00:04:50,400 --> 00:04:55,950 in in 100. tv regime. So the first thing you'll notice in this plot or use or I 51 00:04:55,950 --> 00:05:00,690 should the cross section is a function on this square root of s. terms of the pee 52 00:05:00,690 --> 00:05:05,040 pee coalition. You already see that the pee pee cross section doesn't increase 53 00:05:05,040 --> 00:05:09,900 much between 14 and 100 t. So basically what this means is that the levels of 54 00:05:09,930 --> 00:05:15,870 pileup will scale as the as the level of the something luminosity and not a typical 55 00:05:15,900 --> 00:05:20,550 BP cross section is not increasing that much. This also means that the interesting 56 00:05:20,550 --> 00:05:25,230 physics sticks out more provided that you have the same luminosity, or at least the 57 00:05:25,230 --> 00:05:30,570 same regime of luminosity, that you have a tidal menos etc. So, typically, for 58 00:05:30,570 --> 00:05:36,930 example, for Higgs processes, you have a factor of 20 to 50 in case something as 59 00:05:36,930 --> 00:05:44,160 that changes, or at least slightly shifts perspective at Hunter TV is that standard 60 00:05:44,160 --> 00:05:47,850 model of physics or stuff that is produced basically a threshold when you don't 61 00:05:48,000 --> 00:05:53,490 require high school class is produced more forward is because you have larger 62 00:05:53,490 --> 00:06:01,380 possible imbalance between the two buttons inside the proton and any fact Something 63 00:06:01,380 --> 00:06:04,710 you can see and it's something you have to address if you want to actually be the 64 00:06:04,710 --> 00:06:09,000 detector that can collect these interesting physics is shown in the bottom 65 00:06:09,000 --> 00:06:13,710 plot here. You see a Higgs to follow up on event that falls forward leptons as a 66 00:06:13,710 --> 00:06:18,480 higher detail in rapidity. And for example, if ebf Victor Muslim fusion Higgs 67 00:06:18,480 --> 00:06:22,320 process, where you have this characteristic forward jets, whereas the 68 00:06:22,320 --> 00:06:27,540 30 DVDs picks around typically three or four inches of variability, a tablet TV 69 00:06:27,600 --> 00:06:31,890 would pick around four and five. So you have to instrument these regions. If you 70 00:06:31,890 --> 00:06:36,330 want to collect this physics or you, you have several experiments and we'd like to 71 00:06:36,330 --> 00:06:45,090 see type CB use case for example. On the other on the other end of the spectrum, 72 00:06:45,090 --> 00:06:49,650 you have the boosted physics case, want to make sure you can reconstruct these very 73 00:06:49,650 --> 00:06:54,450 high p particles. This means for cracking, you have to have a large the square or a 74 00:06:54,450 --> 00:07:00,840 single point resolution that can you know, that can that can cope with the With a 75 00:07:00,840 --> 00:07:06,660 high momentum that can handle these high momenta particularly meters, you want to 76 00:07:06,660 --> 00:07:13,380 make sure that you have enough you know, radiation and actual lengths to to stop 77 00:07:13,380 --> 00:07:18,750 these high PT particles. You're lucky in the sense because you know the energy 78 00:07:18,750 --> 00:07:22,440 growth is logarithmic. So, we just add one other additional length and you're 79 00:07:22,440 --> 00:07:26,070 basically done, but this means the more material means that you have a Solomon 80 00:07:26,100 --> 00:07:33,060 behind you know, the whole thing up just scales up by by by a large factor and of 81 00:07:33,060 --> 00:07:39,900 course, this is also possible concern for the for the price, but a principle we 82 00:07:39,900 --> 00:07:44,700 showed that in a car that is assumable to have this kind of to fulfill this kind of 83 00:07:44,700 --> 00:07:51,780 requirement pretty easily provided you build a large enough detector, you have 84 00:07:51,780 --> 00:07:58,590 something that also changes a bit to the in terms of, you know, phenomenology so 85 00:07:58,590 --> 00:08:02,670 for example, a we are using At the NFC to reconstruct the moderately boasted 86 00:08:02,790 --> 00:08:07,500 headphones. So you have this typical displacement of you know, 500 microns for 87 00:08:07,590 --> 00:08:12,690 standard your threshold, you don't have so many one TVs and the LFC or four or five 88 00:08:12,690 --> 00:08:17,430 TVs. Now, if you want to look at resonances, for example, in tops that will 89 00:08:17,430 --> 00:08:21,240 contain 50 VPN and you have to keep in mind that, you know, you're typically the 90 00:08:21,240 --> 00:08:25,860 head and we live 50 centimeter inside the detector and so it will decay later, look 91 00:08:25,860 --> 00:08:30,690 more like you know, emerging chat or chat. So you have to think a bit how you're 92 00:08:30,900 --> 00:08:40,500 designing a talker and you have kind of a dense, dense proportion of material even 93 00:08:40,980 --> 00:08:47,400 even outside your, your your your pizza region. This will allow you to, you know, 94 00:08:47,910 --> 00:08:51,990 to construct these very displaced topology, which is also important for for 95 00:08:51,990 --> 00:08:59,280 new physics. And you're talking about a change in terms of algorithms, right. We 96 00:08:59,280 --> 00:09:03,540 look at This kind of behavior ends in a different way because we look for example 97 00:09:03,540 --> 00:09:10,140 from multiplicity jumps in science from earlier Congress also very highly boosted 98 00:09:10,530 --> 00:09:18,330 WCS and Hicks, you know, attend TV, who will have its decay product which will be 99 00:09:18,330 --> 00:09:23,010 separated by time units. Typically, this is already very short, very small four 100 00:09:23,010 --> 00:09:28,920 kilometer cell and, you know, keep become more outrageous on a medical ultimatum. 101 00:09:28,920 --> 00:09:32,580 So, you will have to rely more and more on tracking to reconstruct these kind of 102 00:09:33,090 --> 00:09:38,220 particles. Now, maybe it's more on the physics program. So, let me start with the 103 00:09:38,220 --> 00:09:41,580 Higgs. So, as I mentioned already, the 104 00:09:42,870 --> 00:09:48,690 Higgs production rates at at FCC h 100. tv will increase by a factor of 20 to 60 105 00:09:48,690 --> 00:09:52,440 depending on which process you're looking at. This gives you access to very early k 106 00:09:52,440 --> 00:09:57,450 modes. Typically, for example, links to email and also which are very 107 00:09:57,450 --> 00:10:02,700 complimentary, plus minus it will give you x Software, a large dynamic range for x 108 00:10:02,700 --> 00:10:08,070 production would produce it addressed. And you will have millions of events with the 109 00:10:08,070 --> 00:10:13,230 one TV Higgs, for example, which give you indirect sensitivity to get some effects, 110 00:10:13,800 --> 00:10:17,490 for example, for particles running in the living room fusion. And also, of course, 111 00:10:17,490 --> 00:10:21,120 the Higgs is a tool for doing Bs and discoveries, because you can have the 112 00:10:21,120 --> 00:10:30,930 stuff that decays into the Higgs and also profitably. And we start with discussing 113 00:10:30,930 --> 00:10:36,030 the rate of the stable so this would be the table of a list of the precision that 114 00:10:36,030 --> 00:10:40,410 is achievable in terms of Higgs couplings at the end of high luminosity hc and 115 00:10:40,440 --> 00:10:44,910 compared to FCC, and it's also to show a little bit of the complementarity between 116 00:10:44,910 --> 00:10:50,370 the hardener experiment and the plasmonics experiment. You can see that for a bunch 117 00:10:50,370 --> 00:10:55,860 of measurement, typical x to z, z, w, w and x two heavy quarks, as long as the 118 00:10:55,860 --> 00:11:01,920 Higgs can came to them. Yes, he does. Very good because branching ratio is larger. 119 00:11:02,910 --> 00:11:07,620 Now, when you go to more read case when the company is smaller, you see that the 120 00:11:07,620 --> 00:11:11,700 FCC runs out of steam. Typically this is the case for external external, my gamma 121 00:11:11,700 --> 00:11:15,990 is a branching ratio, the order of 10 to the minus 310 to the minus four. The 122 00:11:15,990 --> 00:11:20,490 reason is because the SEC can produce only 1 million Hicks's so if you're not if 123 00:11:20,490 --> 00:11:24,750 you're if you're lost a factor of 10 to the forward by by decaying them, you 124 00:11:24,900 --> 00:11:28,470 simply run out of steam to measure them and so, this is what you have cch can 125 00:11:28,470 --> 00:11:32,310 really make the difference. So, another another aspect in which the FCC h h is 126 00:11:32,310 --> 00:11:39,240 complimentary FCC is that at the FCC, so, you can use the very precise measurement 127 00:11:39,240 --> 00:11:44,520 of the SEC. For example, it was easy to normalize what would be relative measure 128 00:11:44,520 --> 00:11:49,140 metal FCC church in order to collider you cannot really measure directly the 129 00:11:49,140 --> 00:11:52,800 coupling of the Higgs you have to make assumption on the Higgs which is not true 130 00:11:52,800 --> 00:11:58,080 at the FCC because at FCC you can measure directly the scalping zz because you 131 00:11:58,080 --> 00:12:02,880 cannot have the Higgs Mass Effect measurement. And this is very interesting 132 00:12:02,880 --> 00:12:06,180 because now once you have this measure this coupling which is precisely measured 133 00:12:06,570 --> 00:12:09,840 at the level of one per minute sec, this gives you an absolute normalization 134 00:12:09,840 --> 00:12:15,180 provided that you can measure these ratios at sec Ah, so maybe a bit more concrete 135 00:12:15,180 --> 00:12:20,310 here what we studied this, for example, here I'm showing the ratio of Hicks to Mew 136 00:12:20,310 --> 00:12:24,660 Mew two weeks to four leptons, which are it's very advantageous because you have 137 00:12:24,660 --> 00:12:27,870 the same object in different states so most of the systematics will cancel out 138 00:12:28,260 --> 00:12:34,230 all the production systematics cancel out and you know city theory uncertainties and 139 00:12:34,230 --> 00:12:38,460 you can see that you can actually measure very precisely this ratio the FCC entered 140 00:12:38,460 --> 00:12:42,630 at the level of 1% which means that since you know the denominator at the level of 141 00:12:42,630 --> 00:12:47,670 one premedia a measurement of extreme you know, the level of 1% this is true also 142 00:12:47,670 --> 00:12:54,330 for z two for a to z gamma for example, and Hicks to gamma gamma. Of course, 143 00:12:54,330 --> 00:13:00,990 another very important measurement at cch is the exact coupling He's a measurement 144 00:13:00,990 --> 00:13:06,270 which is hard even at the FCC ah because of course, this processes that is more 145 00:13:06,270 --> 00:13:10,590 cross section because of these destructive interference between this box and triangle 146 00:13:10,590 --> 00:13:16,440 diagrams. What is on your side is at the FCC church you have a factor 14 creating a 147 00:13:16,440 --> 00:13:20,310 cross section and you have another factor turning your data to university which 148 00:13:20,310 --> 00:13:24,810 gives you a factor for under the event here is an entry effective 20 position 149 00:13:25,230 --> 00:13:30,540 assuming this is statistically limited, which is more or less the case. Now, we 150 00:13:30,540 --> 00:13:35,790 studied this for traumas, which you can see on the right here the negative log 151 00:13:35,790 --> 00:13:39,930 likelihood for each of the channels the most dominant the channel that drives the 152 00:13:39,930 --> 00:13:45,180 sensitivities to be gamma gamma tonics with a precision between three and 8% 153 00:13:45,510 --> 00:13:49,380 depending on which kind of systematic uncertainty you assume Of course, you have 154 00:13:49,380 --> 00:13:53,010 to make a lot of assumption because this machine which will probably be seen today, 155 00:13:53,850 --> 00:13:59,160 you know 50 to 50 years from now, we computed the combination which gives you a 156 00:13:59,190 --> 00:14:08,040 measurement of level of 5% What is interesting is also to see how the self 157 00:14:08,040 --> 00:14:12,150 coupling precision varies as a function of the integrated luminosity. Of course, with 158 00:14:12,150 --> 00:14:18,480 the full ftth runtime you get to precision of order 5% but even if you work around 159 00:14:18,480 --> 00:14:22,440 only three minutes at the bar, which is basically a couple of years of running the 160 00:14:22,440 --> 00:14:27,330 FCC hh you can reach the 10% precision which is the precision you get click for 161 00:14:27,330 --> 00:14:34,650 example or I NC. We also measure we also computed the the precision on k lambda. So 162 00:14:34,650 --> 00:14:39,510 the Higgs f coupling as a function of the coupling of course, this assumes you have 163 00:14:39,510 --> 00:14:42,870 standard model coupling and you don't bury the other couplings. 164 00:14:44,640 --> 00:14:50,070 But this can be interesting for example, you know, for for scenarios or vertically 165 00:14:50,070 --> 00:14:55,890 but identities where you have this large change index, self coupling. This is a 166 00:14:55,890 --> 00:15:02,640 summary of the values Higgs measurements. Between FCC and FTC ah You can see that 167 00:15:02,640 --> 00:15:07,380 there is this very nice complementarity or you get below 1% for most of them and you 168 00:15:07,380 --> 00:15:12,840 will really have some of them which can be measured better with FCC and others which 169 00:15:12,840 --> 00:15:17,520 can be measured with FCC judge because these are kth to me Mr. gamma gamma 170 00:15:17,520 --> 00:15:21,120 described earlier and of course, acts of copying which you cannot measure it 171 00:15:21,660 --> 00:15:27,600 directly can only do it to the oddity productions. Something I mentioned before 172 00:15:27,600 --> 00:15:34,830 also, it's something which is very interesting at the FCC. hh is this 173 00:15:34,920 --> 00:15:39,810 complementarity in the, in the in the measurement of the Higgs of coupling and 174 00:15:39,810 --> 00:15:45,900 the search for, you know, the creation of the standard model which could explain the 175 00:15:45,900 --> 00:15:49,380 larger volume of symmetry in our universe. So, you can have this extension of the 176 00:15:49,380 --> 00:15:55,860 standard model with a with a singlet on the left plot, you can see what is covered 177 00:15:55,860 --> 00:16:00,510 in these bands is basically these points that give you these stamps. First on the 178 00:16:00,510 --> 00:16:05,880 first condition, and you can see that with 100 kV a 13, or sarcoma these red occur 179 00:16:06,120 --> 00:16:11,160 allows you to exclude most of the of the of the point. And on the right block even 180 00:16:11,160 --> 00:16:16,230 more interesting plot which gives you in the x axis the pressure on the Higgs of 181 00:16:16,230 --> 00:16:20,730 coupling on the y axis, the precision on the X was easy coupling, which is 182 00:16:20,730 --> 00:16:25,110 basically the flagship measurement of the SEC, all these thoughts are thoughts that 183 00:16:25,110 --> 00:16:28,860 give you again, the strong first quarter 10th edition, the ones which are favored 184 00:16:28,890 --> 00:16:37,110 by, by, by this theory, and in fact, what you can see is that the SEC can exclude 185 00:16:37,110 --> 00:16:43,050 basically most of the points on the Z on the X on the y axis whereas your ch can 186 00:16:43,440 --> 00:16:45,690 actually constrain the most on the x axis. 187 00:16:46,500 --> 00:16:47,790 We have four minutes left, 188 00:16:48,330 --> 00:16:56,430 okay, I will try to go fast, maybe I can skip this. So their hips too. Invisible is 189 00:16:56,430 --> 00:17:01,440 also a very important measurement because it cannot It allows you to probe 190 00:17:02,490 --> 00:17:05,040 directional Higgs to potentially a dark matter. 191 00:17:07,020 --> 00:17:09,750 And this was studied also in the context of the cdr. 192 00:17:11,250 --> 00:17:17,130 You have these very large sitting in your background, which you can constrain by by 193 00:17:17,130 --> 00:17:21,210 measuring the CW and gamma spectra and you can also actually measure it, you know, 194 00:17:21,210 --> 00:17:26,220 when you have high statistics from the past minus you control region. In fact, 195 00:17:26,220 --> 00:17:31,470 you have so much statistical data that you can actually do even better than FCC and 196 00:17:31,470 --> 00:17:36,690 you can actually even measure the standard model. It was easy to form a neutrino 197 00:17:38,460 --> 00:17:40,230 the level of 10% I believe, 198 00:17:43,650 --> 00:17:47,970 something else you can do of course, you know high energy collider as I mentioned 199 00:17:47,970 --> 00:17:51,780 at the beginning, and this is something is the first thing you look at if you wish 200 00:17:51,780 --> 00:17:56,250 when you start to assess these kind of options because you want to check whether 201 00:17:56,550 --> 00:18:05,280 you can fulfill the promise Increasing these Kaveri rich. And so the first thing 202 00:18:05,280 --> 00:18:13,170 to look at is resonances. So you can see primes to dialect on tops Graviton to W. 203 00:18:13,860 --> 00:18:18,450 Of course, this will make use of stars, Jetstar, certainly because we look at 204 00:18:18,450 --> 00:18:25,110 these in the Atlantic channel. So the two highly most tops, W's who educate 205 00:18:25,140 --> 00:18:30,990 chronically as well. And of course, you have constraints from the tech revolution 206 00:18:30,990 --> 00:18:35,790 because of the fact I mentioned earlier that is highly boost and jets will be 207 00:18:36,480 --> 00:18:40,530 severely collimated and eventually will emerge and you won't be able to 208 00:18:40,530 --> 00:18:43,770 distinguish them too much from QC digits. 209 00:18:46,770 --> 00:18:48,420 We also look at this flavor inspired 210 00:18:49,800 --> 00:18:55,770 model where you have DC prime coupling to DNS only. That could explain in a minimal 211 00:18:55,770 --> 00:19:02,670 way. The B to k star mimeo Family and we showed that we just checked you can 212 00:19:02,670 --> 00:19:10,200 basically exclude all the allowed parameter space suit stops again we use 213 00:19:10,200 --> 00:19:16,320 these very same boosted technique to construct these atomic jets. He came from 214 00:19:16,680 --> 00:19:21,720 a highly massive stops which we'll get into how he was the top and you can show 215 00:19:21,720 --> 00:19:28,530 that you can you can actually discover stops up to 10 TV more or less at the FCC 216 00:19:28,530 --> 00:19:36,030 ah Finally, something which is also very interesting is exotic signatures such as 217 00:19:36,360 --> 00:19:43,440 such as disappearing tax. So, you have this very simple with a type of dark 218 00:19:43,440 --> 00:19:49,830 matter scenario that emulate with a dark force. Xenon when a dark matter, which are 219 00:19:49,830 --> 00:19:55,140 favored in the range of one and three TV, it observes that Alec abundance, these are 220 00:19:55,140 --> 00:19:59,010 very typical compressed my my spectrum which are these very characteristic 221 00:19:59,010 --> 00:20:04,020 signatures Have a charged particle that will basically disappear in your detector 222 00:20:04,020 --> 00:20:08,250 because it will decay to a very soft biome and missing energy and you cannot 223 00:20:08,250 --> 00:20:12,630 reconstruct the soft pi and so, your your signal is basically this disappearing tax. 224 00:20:13,110 --> 00:20:18,090 And this group of people from doctrine is very nice studies shows that you can 225 00:20:18,090 --> 00:20:26,190 basically cover and actually discover both Xenon we know dark matter and Pshh should 226 00:20:26,490 --> 00:20:34,980 properly design your packet volume. And so, I come to the conclusion, I will just 227 00:20:34,980 --> 00:20:40,230 briefly summarize the bytes I went through. So, the large statistics are GCC 228 00:20:40,230 --> 00:20:45,390 h h in terms of Higgs physics, so, we typically produce 10 to the 10 Higgs boson 229 00:20:45,390 --> 00:20:50,160 open up a new range of possibilities, allowing both to measure or advocate 230 00:20:50,160 --> 00:20:54,750 channel and measure the Higgs in eukaryotic genome and he's really 231 00:20:54,750 --> 00:21:00,450 complimentary to that see. You can measure ratios of couplings or equivalent Key 232 00:21:00,450 --> 00:21:04,980 ratios of branching ratios concept both systematics and to allow you to normalize 233 00:21:06,030 --> 00:21:12,000 these measurement with respect to the SEC give you they're often the absolute 234 00:21:12,450 --> 00:21:17,880 counting measurement, you can measure the Higgs coupling to a precision of about 5% 235 00:21:17,880 --> 00:21:22,620 and the FC change which is among all proposed future options, they are the most 236 00:21:22,620 --> 00:21:33,510 precise measurement and you can directly excluded these very simple models of or or 237 00:21:33,510 --> 00:21:38,340 fine or discovered of for compatible with the first time that I took this position. 238 00:21:38,610 --> 00:21:43,890 And of course, you have unprecedented reach for direct searches, evidence 239 00:21:43,890 --> 00:21:48,060 associated searches. I hope I made it in time. 240 00:21:51,240 --> 00:21:53,100 Yes, you did. Thanks. Let me kill 241 00:21:55,290 --> 00:22:01,560 without warning open the panel for for questions or comments. So that's the usual 242 00:22:01,560 --> 00:22:05,850 procedure please raise your hand and then we will give me 243 00:22:07,230 --> 00:22:08,370 permission to speak 244 00:22:11,250 --> 00:22:12,330 any questions? 245 00:22:21,090 --> 00:22:28,140 If not maybe a naive one from from myself. I'm not an expert on on sushi but I always 246 00:22:28,140 --> 00:22:33,180 had the impression that already with Elysee databases very much under pressure 247 00:22:33,180 --> 00:22:34,020 to say the least. 248 00:22:35,700 --> 00:22:36,390 How much 249 00:22:37,800 --> 00:22:44,850 to do people actually still have hope to to find something yet at FCC or how much 250 00:22:44,850 --> 00:22:47,580 are these models constructed actually true? 251 00:22:47,790 --> 00:22:51,540 Well, I believe that Okay, these are these are modern, more fine tuned model, of 252 00:22:51,540 --> 00:22:58,140 course, but I think that rather than, you know, giving a hope measures to find Susie 253 00:22:58,140 --> 00:23:03,720 or not, Yes Ah, this is a way It's a well known and well studied model such that 254 00:23:03,720 --> 00:23:08,340 people can refer to when you evaluate to the benchmark country to the doctor. I 255 00:23:08,340 --> 00:23:10,200 mean, which is more the way I see this 256 00:23:14,519 --> 00:23:15,539 community maybe 257 00:23:15,839 --> 00:23:18,029 I can comment better on a 258 00:23:19,350 --> 00:23:20,880 wireless has 259 00:23:22,590 --> 00:23:30,540 been doing very bad Of course, but not that we we we have absolutely no no no 260 00:23:30,540 --> 00:23:36,450 reason to stop searching directly for new resonances. supersymmetry may still be 261 00:23:36,450 --> 00:23:39,150 there look a little bit different from what we thought and there are many there 262 00:23:39,150 --> 00:23:43,770 can be many more scenario. So I totally agree with what you said. The the idea of 263 00:23:43,770 --> 00:23:47,430 having these sushi benchmarks is simply because they are a lot of particles which 264 00:23:47,430 --> 00:23:52,230 has been studied already. And we want to know how well we can be ready to discover 265 00:23:52,350 --> 00:23:57,930 new particles of the broadest possible variety. So it's like a catalog. Okay, for 266 00:23:57,930 --> 00:24:06,540 me, and I think we get like these So, I had a question. Yes. Oh, if you want so my 267 00:24:06,540 --> 00:24:12,420 question was about this dispenser extra linear we always so you show that and you 268 00:24:12,420 --> 00:24:16,950 comment on slide 15 that actually in most actually, as far as I know, almost all the 269 00:24:17,040 --> 00:24:21,960 other Genesis models, the single leaks, it's enough right? Single leaks gathering 270 00:24:21,960 --> 00:24:26,970 measuring very well at some collider closes a bit the door to these these 271 00:24:26,970 --> 00:24:30,780 models. So what is actually left? I mean, we want to move to measure the cylinder 272 00:24:30,780 --> 00:24:31,860 But why? 273 00:24:32,610 --> 00:24:37,170 Well, I think this is a question for theorists like you but in from an 274 00:24:37,170 --> 00:24:40,920 experimental perspective, if you're completely naive, you have a new particle 275 00:24:40,920 --> 00:24:44,910 and you know, you have a unit you know, you have a predicted value for its 276 00:24:44,910 --> 00:24:49,500 coupling and a standard model. And even if you you know, even if you don't have 277 00:24:49,500 --> 00:24:55,860 anything in mind that you want measure is new, all its new couplings to death. And 278 00:24:56,130 --> 00:24:59,820 the history of coupling is one of them. I mean, this is at least my perspective on 279 00:24:59,820 --> 00:25:06,450 it. You're right. I mean, of course, it seems that measuring the zz and extra vv 280 00:25:06,450 --> 00:25:12,630 couplings and naptime colliders will be enough to constrain these models. You 281 00:25:12,630 --> 00:25:15,930 probably even know better than me. There might be even some models for Jewish this 282 00:25:15,930 --> 00:25:16,740 is not the case. 283 00:25:18,119 --> 00:25:22,199 It's difficult. It's difficult to find some there are corners of things. Now, 284 00:25:22,199 --> 00:25:25,649 maybe I don't agree with what you're saying, don't you think is maybe that 285 00:25:25,649 --> 00:25:31,379 measuring, I don't know, 10 times or 100 times better. The scalping to vector 286 00:25:31,379 --> 00:25:35,639 vector may be more productive than measuring the extra linear, which doesn't 287 00:25:35,639 --> 00:25:39,659 mean it is to say, we can put both things but yeah, 288 00:25:40,109 --> 00:25:42,509 okay, this might be true. And I think we shouldn't do both. 289 00:25:44,760 --> 00:25:49,560 In fact, I think probably the best way would be to start by measuring up to the 290 00:25:49,560 --> 00:25:52,620 highest possible position with a plus or minus collider and then 291 00:25:53,730 --> 00:25:55,110 then measure that the linear 292 00:25:55,680 --> 00:25:58,140 Thomasina procedure with a Hadron Collider. 293 00:26:00,810 --> 00:26:01,350 Okay, 294 00:26:02,760 --> 00:26:03,390 thank you. 295 00:26:05,009 --> 00:26:11,009 I don't see any further raised hands so let's think Michaela again. And then you