1 00:00:02,070 --> 00:00:07,500 In my house, talking about recent results on call activity and small systems from 2 00:00:07,500 --> 00:00:09,030 the Atlas collaboration. 3 00:00:11,670 --> 00:00:15,330 And let's see if we'll go forward. There we go. So there are a wealth of Atlas 4 00:00:15,330 --> 00:00:20,070 results on small systems and I listed a number of the recent ones down below. But 5 00:00:20,070 --> 00:00:24,510 in these 15 minutes, I want to focus on just one recent measurement. And that's 6 00:00:24,690 --> 00:00:29,100 the transverse momentum and process dependent azimuth and I saw trapeze in p 7 00:00:29,100 --> 00:00:33,840 lead collisions published recently in this article, and that's the thesis work of 8 00:00:33,840 --> 00:00:36,840 Kurt Hill which you can read in full detail linked here. 9 00:00:38,160 --> 00:00:44,310 So key features of heavy ion Coalition's we often think of the Hydra dynamically 10 00:00:44,310 --> 00:00:49,230 described collectivity of the bulk, you can argue about which PT separates that 11 00:00:49,230 --> 00:00:54,360 region, but you might think sort of below five six gv and the jet quenching 12 00:00:54,360 --> 00:00:59,850 phenomenon, the suppression of high Pt parkins jets and hey drones in the high PT 13 00:00:59,850 --> 00:01:00,000 region. 14 00:01:00,000 --> 00:01:06,630 Maybe above 10 to 12 GDP. And if you think of the hydrodynamics, you have the initial 15 00:01:06,630 --> 00:01:11,460 state where you have steeper density gradients along the x axis in this diagram 16 00:01:11,490 --> 00:01:16,740 on the left. And so, due to the steeper density gradients, when you couple that 17 00:01:16,740 --> 00:01:22,470 with hydrodynamics, you get more bulk particles along the x axis. In the case of 18 00:01:22,500 --> 00:01:27,390 jet quenching, you have that same geometry. But in this case, these high PT 19 00:01:27,390 --> 00:01:32,040 part cons and the resulting jets have a shorter path out of the medium along the x 20 00:01:32,040 --> 00:01:38,040 axis. And so, you expect more jets and protons at high PT to survive on the x 21 00:01:38,040 --> 00:01:46,050 axis and to be more suppressed in vertical or Y axis. And so that means that due to 22 00:01:46,050 --> 00:01:52,110 these two different phenomena, low PT bulk particles are asked to be fully correlated 23 00:01:52,110 --> 00:01:57,120 with high PT jet particles because they both result from the same underlying 24 00:01:57,120 --> 00:01:59,610 geometry that impacts them 25 00:02:00,810 --> 00:02:06,900 And that's exactly what's seen in lead lead collisions. Here is the vn for 26 00:02:06,900 --> 00:02:10,530 moments two through seven and the different colors versus transverse 27 00:02:10,530 --> 00:02:17,100 momentum. And in sort of the low PT region that's shaded in blue might think of this 28 00:02:17,100 --> 00:02:24,060 as being from hydrodynamics. In high PT region, you still see a significant v2, 29 00:02:24,390 --> 00:02:29,250 that's often interpreted as being again from jet quenching. Again, remember, it's 30 00:02:29,250 --> 00:02:34,410 a correlation between high PT and low PT is the way these VMs are measured. So just 31 00:02:34,410 --> 00:02:38,670 like I discussed in the last slide, and then in purple, this is some transition 32 00:02:38,670 --> 00:02:45,870 region where you have a mixture of these effects. And in p led Coalition's are the 33 00:02:45,900 --> 00:02:50,400 same plot over here. And as discussed in the previous talks, there's sort of 34 00:02:50,400 --> 00:02:56,700 similar anisotropy is in the low PT region in blue, maybe that's hydrodynamics at 35 00:02:56,700 --> 00:03:00,000 high PT from previous Atlas publication is really just 36 00:03:00,000 --> 00:03:05,790 one data point in this higher PT region. And maybe that's a hint about this 37 00:03:05,820 --> 00:03:10,320 question of jet quenching or some other phenomena and a large region of sort of 38 00:03:10,320 --> 00:03:16,830 purple in the middle. And so the goal was, how do we fill out that high PT region in 39 00:03:16,950 --> 00:03:18,060 led collections. 40 00:03:19,289 --> 00:03:26,369 And so this Atlas analysis uses the 2016 p loaded ATV data, we're going to use three 41 00:03:26,369 --> 00:03:29,489 different samples, I'm only going to show two of them in this talk, but all three 42 00:03:29,489 --> 00:03:33,359 are in the paper, there's a minimum bias triggered sample and there's a sample 43 00:03:33,359 --> 00:03:40,049 triggered by events that have jet with PT greater than 100 Gp, and I'll skip the 44 00:03:40,049 --> 00:03:45,689 detector details since they're pretty familiar. So what we're doing is a p led 45 00:03:45,719 --> 00:03:51,809 to particle correlation. And what's shown on the left is the two particle 46 00:03:51,809 --> 00:03:56,969 correlation and high multiplicity p light events in the case where it's the minimum 47 00:03:56,969 --> 00:03:59,909 bias event trigger and a standard 48 00:04:00,480 --> 00:04:06,450 template method is used to remove the non flow, and you see the dominance of the v2 49 00:04:06,450 --> 00:04:11,790 coefficient in the lower panel. However, if you look at events where there's a jet 50 00:04:11,820 --> 00:04:19,230 greater than 100, gv, you see that the non flow contribution is a lot bigger, right? 51 00:04:19,260 --> 00:04:24,720 sort of imagine, here's the blue flow coefficient potentially. And there's this 52 00:04:24,720 --> 00:04:29,640 very large jet correlation, which is expected because these are events from 53 00:04:29,640 --> 00:04:34,890 jets. And in fact, you can see that basically, there's a distortion here in 54 00:04:34,890 --> 00:04:38,970 the template subtracting procedure, because effectively the signal to 55 00:04:38,970 --> 00:04:44,160 background is so small. And so in order to do this kind of measurement reliably, we 56 00:04:44,160 --> 00:04:50,040 need to reduce that non flow background. And so the technique that's used is 57 00:04:50,070 --> 00:04:57,150 restricting associated particles in the events that have 100 gV jets. So we do the 58 00:04:57,150 --> 00:04:59,970 standard thing of the associated particle must be 59 00:05:00,480 --> 00:05:04,200 Have a delta theta greater than two from the trigger particle, as we've heard in 60 00:05:04,200 --> 00:05:10,230 previous talks. But now In addition, we're going to restrict the associated particle 61 00:05:10,440 --> 00:05:17,430 to be delta Ada greater than one relative to all jets greater than 15. gv in the 62 00:05:17,430 --> 00:05:21,420 event. So the trigger particle can come from a jet. That's what you might expect 63 00:05:21,420 --> 00:05:26,790 that high PT. But the associated particle, we want to reduce its contribution coming 64 00:05:26,790 --> 00:05:31,230 from jets. And that was has a large enough acceptance that even an event with 65 00:05:31,230 --> 00:05:35,880 multiple jets, there's still quite a bit of acceptance to get statistics for these 66 00:05:35,880 --> 00:05:36,900 correlations. 67 00:05:38,640 --> 00:05:43,380 And so this just displays how this works. The left plot is the one that I already 68 00:05:43,380 --> 00:05:49,410 showed you a couple slides ago. These are p led high multiplicity events with 100 gV 69 00:05:49,410 --> 00:05:57,060 jet, so that has a low flow signal to jet background, this big peak here, and then 70 00:05:57,150 --> 00:06:00,000 after we apply this jet restriction 71 00:06:00,000 --> 00:06:06,600 So we try to eliminate associated particles that are in jet cones, you see 72 00:06:06,600 --> 00:06:11,880 that a dramatic improvement in the signal to background. And we now have what looks 73 00:06:11,880 --> 00:06:17,850 like a pretty successful template fit to basically remove the non flow. And so the 74 00:06:17,850 --> 00:06:22,110 improvement in the signal to background really reduces the sensitivity to the 75 00:06:22,110 --> 00:06:25,590 template method assumptions. And that's a key in this measurement. 76 00:06:27,210 --> 00:06:34,800 And so here are the results. And so we're plotting v2 as a function of P t of the 77 00:06:34,800 --> 00:06:40,770 associated particle. And there are two different sets of points. So the black 78 00:06:40,770 --> 00:06:46,950 points are in minimum bias events where we do not have to apply this jet rejection. 79 00:06:47,370 --> 00:06:52,050 And we see this familiar pattern where the v2 is rising up. 80 00:06:53,130 --> 00:06:57,840 It's then falling and now we have enough statistics to actually have a couple of 81 00:06:57,840 --> 00:07:00,000 points at PT great 82 00:07:00,000 --> 00:07:06,420 Than 10, gv that seems to confirm a v2 of order a couple percent even in that 83 00:07:06,420 --> 00:07:12,480 region. And then what's really dramatically different is now we can look 84 00:07:12,480 --> 00:07:17,190 in these events with a jet trigger greater than 100, gv. And of course, this trigger 85 00:07:17,190 --> 00:07:24,540 sample, the full p lead, luminosity delivered. And so we get the rise the fall 86 00:07:24,540 --> 00:07:31,680 and now we have very, very good statistics all the way out to 50 gV in PT. And we see 87 00:07:31,680 --> 00:07:41,130 that that two to 3% v2 remains up to the highest pts that we measure. And so, in 88 00:07:41,130 --> 00:07:46,560 the blue region, you can think again of the low PT bulk we can confirm the rising 89 00:07:46,560 --> 00:07:47,340 v2. 90 00:07:48,360 --> 00:07:54,600 Now in the high PT region, getting all the way up to 50. We really see that there is 91 00:07:54,600 --> 00:08:00,000 a correlation and acid myth between the low PT bulk particles and the high p TP 92 00:08:00,000 --> 00:08:04,770 articles and in a Coalition's This is interpreted in terms of jet quenching. 93 00:08:06,299 --> 00:08:09,869 And then there's a transition region in purple in the middle. And there's a 94 00:08:09,869 --> 00:08:12,839 difference between the two trigger samples, which I'm not going to have time 95 00:08:12,839 --> 00:08:16,349 to talk about in this talk. But if people have questions, you can take a look in the 96 00:08:16,349 --> 00:08:17,729 paper or ask at the end. 97 00:08:19,980 --> 00:08:27,000 One thing that's quite striking is if you overlay the v two results versus PT with 98 00:08:27,030 --> 00:08:32,130 previously published Atlas led led data with the P led scale by a single factor of 99 00:08:32,130 --> 00:08:38,520 1.5, they actually look quite similar. And again, I think there's a lot of 100 00:08:38,520 --> 00:08:42,300 speculation that there's a common hydrodynamic explanation for sort of the 101 00:08:42,300 --> 00:08:47,400 lower PT. And I guess the question is, is that our common explanation for the high 102 00:08:47,400 --> 00:08:48,660 PT correlation? 103 00:08:51,630 --> 00:08:55,560 You know, in the last few minutes, talk about a couple of different pictures. So 104 00:08:55,560 --> 00:08:59,970 what if we think of it as jet quenching in pea lead? Well, in fact, this is 105 00:09:00,000 --> 00:09:07,200 Some old paper from Zhang and Lau, where they model a small q GP droplet in p led 106 00:09:07,200 --> 00:09:12,660 Coalition's and they actually calculated v2 and the two different dashed curves are 107 00:09:12,660 --> 00:09:18,000 two different size q GP droplets. And what you see is that actually, their 108 00:09:18,000 --> 00:09:25,290 description of the P lead v2 is qualitatively not so bad, but in the same 109 00:09:25,290 --> 00:09:32,490 paper in the same model. They also predict in the right hand plot the RP lead the 110 00:09:32,490 --> 00:09:38,250 nuclear suppression factor and P lead and they predicted nuclear suppression factor 111 00:09:38,430 --> 00:09:45,810 of almost a factor of point five at low PT rising very slowly up to 50 gV, but still 112 00:09:45,810 --> 00:09:50,970 being a 30% suppression. And even though there are, you know, challenges in 113 00:09:50,970 --> 00:09:58,260 measuring RP lead in central events, their results from Atlas and Elise, basically 114 00:09:58,260 --> 00:09:59,970 strongly disfavor that level. 115 00:10:00,000 --> 00:10:05,130 hole of suppression. And so just like in a collisions, you need a pretty large 116 00:10:05,130 --> 00:10:11,970 modification to the PT spectra in order to generate a differential jet quenching. And 117 00:10:11,970 --> 00:10:18,030 so this cannot describe both azimuthal and isotropy. And the lack of change in PT 118 00:10:18,030 --> 00:10:23,130 spectra. And that's a pretty fundamental challenge, I think, to any jet quenching 119 00:10:23,130 --> 00:10:25,230 model, not just this specific one. 120 00:10:27,180 --> 00:10:31,980 The other interpretation I want to walk through which was discussed in the paper 121 00:10:31,980 --> 00:10:36,990 is the initial state effect model. And I want to remind people that a key check for 122 00:10:36,990 --> 00:10:42,450 the original pee pee rich correlation observed by CMS was checking in pythia. 123 00:10:42,690 --> 00:10:48,150 And so here are a couple plots from the original sort of seminal CMS paper. The 124 00:10:48,180 --> 00:10:54,300 left was the pee pee rich in real data, and the right was the result from pythia 125 00:10:54,330 --> 00:10:56,460 where no Ridge was seen. 126 00:10:58,140 --> 00:11:00,000 But pythia sort of has a revival. 127 00:11:00,000 --> 00:11:06,390 ENTJ In fact, in the left plot, this is pythia, eight in soft to CD non 128 00:11:06,390 --> 00:11:10,980 diffractive mode. And as CMS observed in their paper, there's no long range ridge. 129 00:11:11,520 --> 00:11:17,550 But actually, if you run pythia, eight in Hart q CD mode with a PT hat men have 15, 130 00:11:17,550 --> 00:11:24,150 gv, and then basically requiring a jet in the event as we're sort of doing in our 131 00:11:24,150 --> 00:11:31,560 analysis. There's actually a long range rich in pythia. And actually, we've traced 132 00:11:31,560 --> 00:11:37,830 that down to an implementation and pythia of initial state radiation in space shower 133 00:11:37,830 --> 00:11:43,290 routine, and confirm that with the author's it's a radiation pattern from 134 00:11:43,290 --> 00:11:47,640 color coherence considerations. And just to emphasize, since some of you will be 135 00:11:47,640 --> 00:11:53,280 familiar, this is not the string shoving option described in this paper. This is 136 00:11:53,280 --> 00:12:00,000 really not due to interaction. It's due to a coherence effect. However, 137 00:12:00,539 --> 00:12:06,209 The effect is biggest in low multiplicity events, and is watered down in high 138 00:12:06,209 --> 00:12:11,879 multiplicity events. It's a correlation amongst only a subset of the particles 139 00:12:11,909 --> 00:12:17,159 from this radiation pattern. And so in fact, what happens is kind of interesting. 140 00:12:17,429 --> 00:12:22,589 If you run the pythia. In this case, it's argued inter. So it's p lead. If you 141 00:12:22,589 --> 00:12:27,869 actually run it through our full analysis procedure, what you get is there's 142 00:12:27,869 --> 00:12:30,839 actually a near side. 143 00:12:32,670 --> 00:12:39,420 Rich that comes out, but because it's stronger in low multiplicity events than 144 00:12:39,420 --> 00:12:44,910 in high multiplicity, when you apply the template subtraction procedure, it 145 00:12:44,910 --> 00:12:50,280 actually predicts a negative correlation and high multiplicity events. So of 146 00:12:50,280 --> 00:12:56,280 course, the V to two predicted due to this long range rich and pythia actually is 147 00:12:56,280 --> 00:13:00,000 negative. So we plotted this v two two because normally you 148 00:13:00,000 --> 00:13:05,340 You'd have to take a square root, so you'd get an imaginary vi to me. I mean, it's, 149 00:13:05,580 --> 00:13:09,990 yep, thank you. And I think this is a problem with any explanation in the 150 00:13:09,990 --> 00:13:17,280 initial state that involves lowercase n less than n total particles, which is that 151 00:13:17,280 --> 00:13:21,450 as you go to higher and higher multiplicity events, this kind of initial 152 00:13:21,450 --> 00:13:26,250 state effect gets watered down gets smaller and smaller. And that's the 153 00:13:26,280 --> 00:13:32,760 opposite of what we see in experimental data. So sort of both of these theoretical 154 00:13:32,760 --> 00:13:38,580 approaches face major challenges in describing experimental data. 155 00:13:40,560 --> 00:13:46,650 And so just sort of on my last slide here, want to show the result again, in p led 156 00:13:46,650 --> 00:13:52,830 collisions in black and then orange for the events with a jet greater than 100. gv 157 00:13:52,950 --> 00:14:00,000 overlaid with the lead lead events. And so this new Atlas results really extend 158 00:14:00,000 --> 00:14:08,580 These v2 measurements up to very high PT. The paper also shows v3. It's similar 159 00:14:08,580 --> 00:14:13,380 trend but statistically a little bit challenged at the highest PT. So I think 160 00:14:13,380 --> 00:14:18,330 this sets out that there's a definitive correlation of high and low PT particles 161 00:14:18,330 --> 00:14:23,820 and P lead events where low PTs and youth land isotropy is typically explained by 162 00:14:23,820 --> 00:14:29,430 hydrodynamics and geometry. So that implies if you follow that logic that 163 00:14:29,430 --> 00:14:35,010 these high PT particles are correlated with the geometry. But there are 164 00:14:35,010 --> 00:14:39,720 fundamental conflicts with that explanation in terms of jet quenching, and 165 00:14:39,720 --> 00:14:44,370 also in terms of initial state explanations. And so I think this is an 166 00:14:44,400 --> 00:14:49,050 excellent puzzle to be solved in the future. Thank you for your attention. 167 00:14:50,070 --> 00:14:54,840 Thank you, Jeremy, for this very interesting presentation. And yeah, so now 168 00:14:54,840 --> 00:14:59,970 we have time for questions. if people have questions, please 169 00:15:00,000 --> 00:15:02,280 force a raise hand button. 170 00:15:13,200 --> 00:15:15,510 I don't see any hands. 171 00:15:20,100 --> 00:15:26,430 Hi Ivana. This is Alina I cannot raise hand because in being host I cannot. But a 172 00:15:26,850 --> 00:15:27,600 Hello Jamie 173 00:15:29,160 --> 00:15:33,690 Hello is a when you mention the results from btn 174 00:15:34,830 --> 00:15:41,370 taking calm to a these radiation DC, a mentioning that has nothing to do with a 175 00:15:41,400 --> 00:15:49,140 string showing. Uh huh. What do you mean? I mean, it's just to mean domain that has 176 00:15:49,140 --> 00:15:55,710 nothing to do with color reconnection. Well, what I meant is there's a specific 177 00:15:55,740 --> 00:15:57,570 implementation of pythia 178 00:15:58,650 --> 00:15:59,970 from Christian beer Lucia. 179 00:16:00,000 --> 00:16:08,370 All that has strings shoving, and air, they do see a long range Ridge because 180 00:16:08,370 --> 00:16:13,020 they're basically coupling the string interactions to geometry. And I just 181 00:16:13,020 --> 00:16:19,170 wanted to make very clear that the effect that we're seeing here is not the string 182 00:16:19,170 --> 00:16:25,590 shoving, implementing. Okay, it's really from a different effect. Okay, yeah. Thank 183 00:16:25,590 --> 00:16:26,700 you. Thank you very much. 184 00:16:28,560 --> 00:16:32,310 Thank you, Elena. Do we have more questions to James? 185 00:16:37,980 --> 00:16:42,480 Okay, I don't see any but I have 111 186 00:16:43,680 --> 00:16:50,370 where you are discussing the this model for jet quenching in proton. So how do we 187 00:16:50,400 --> 00:16:55,170 how do they decide define sizes? So perhaps you said that but somehow I missed 188 00:16:55,170 --> 00:16:59,910 it. What's the difference between a and b? Yeah. So it's a rather old 189 00:17:00,000 --> 00:17:04,890 paper, I think they just are basically making different assumptions that relate 190 00:17:04,920 --> 00:17:12,630 the multiplicity of the event to the size and temperature of the DGP droplet. So 191 00:17:12,630 --> 00:17:16,920 they provided both predictions. I don't know whether one could sort of think of 192 00:17:16,920 --> 00:17:22,740 that as a systematic uncertainty in their picture on the size of the droplet. 193 00:17:24,450 --> 00:17:26,790 Okay, thank you. That explains. 194 00:17:27,930 --> 00:17:33,300 Okay, I don't see more questions to this specific presentation. But right now, 195 00:17:33,330 --> 00:17:40,170 given that we have a discussion with all speakers of the session, so first of all, 196 00:17:40,170 --> 00:17:45,930 I'd like to invite all speakers to be available to answer questions. And of 197 00:17:45,930 --> 00:17:51,090 course, I'd like to invite all participants to ask questions to either to 198 00:17:51,090 --> 00:17:56,820 specific speakers or to all of them. So please, if you have a question to add to 199 00:17:56,820 --> 00:17:59,640 our speakers of the session, please push 200 00:18:00,510 --> 00:18:01,530 And I can button. 201 00:18:19,140 --> 00:18:24,750 Hello Ivana. This is la nafa radio. Yeah. Hello, please go. Hello. I had a question 202 00:18:24,750 --> 00:18:35,910 for a Lexus. A concerning a Alex's. Can you hear me? Yes. Yeah. A I like very much 203 00:18:35,910 --> 00:18:42,300 your talk. I had a question when you were estimating the kinetic time 204 00:18:43,350 --> 00:18:50,100 a is proportional to the number of creative particles divided by the 205 00:18:50,100 --> 00:18:55,200 transverse transverse area. My question would be, how do you do you have an 206 00:18:55,200 --> 00:18:59,970 asymmetric Colosseum? Because your example I think was different is life saving 207 00:19:01,140 --> 00:19:05,610 A your examples were for proton proton or nucleus nucleus coalition. 208 00:19:07,109 --> 00:19:09,599 Yes. So in that case, it was 209 00:19:11,429 --> 00:19:18,869 of course a simplification, but we'll just take a typical area of the system. So, in 210 00:19:18,869 --> 00:19:25,229 a symmetric collisions of Ah sorry, you meant not peripheral, but yes, yes yeah, 211 00:19:25,229 --> 00:19:33,119 no, no no I mentioning a set for collisions that a proton nucleus Yeah. So, 212 00:19:33,629 --> 00:19:37,379 you have to consider the mid rapidity. 213 00:19:39,210 --> 00:19:47,310 Particle multiplicities and where I mean of course, lots of mismo participants will 214 00:19:47,310 --> 00:19:55,170 not not participate, you know. So, you can think of P let collisions also as with 215 00:19:55,170 --> 00:19:59,910 some transfer Syria, of course, it's very maybe crude approximation, but we didn't 216 00:19:59,940 --> 00:20:00,000 know 217 00:20:00,000 --> 00:20:04,230 Specific so the description I was 218 00:20:05,310 --> 00:20:10,200 talking about is well suited for, of course, symmetric, large system 219 00:20:10,200 --> 00:20:15,330 collisions. It's just a way of how you could, from that understanding try to make 220 00:20:15,330 --> 00:20:20,820 predictions. For smaller systems, it doesn't have inherently a symmetric 221 00:20:21,270 --> 00:20:26,040 symmetry. So it's just more a question of a, you know, once you have proton 222 00:20:26,040 --> 00:20:30,510 colliding on on on lead, can you also just assume that the system has a small 223 00:20:30,510 --> 00:20:37,080 transfers area and just forget about the rest of Yeah, so like, proton? A, okay. 224 00:20:37,080 --> 00:20:37,440 Yeah. 225 00:20:39,360 --> 00:20:42,210 Yeah. Okay. Okay. Thank you very much. Thank you. 226 00:20:44,280 --> 00:20:46,590 Thank you. Do we have more questions? 227 00:20:52,320 --> 00:20:57,540 Okay, so maybe I will start actually, I have a question to all experimental 228 00:20:58,740 --> 00:20:59,760 speakers. 229 00:21:00,000 --> 00:21:07,230 So, how low in drachma TP PCT do we see collectivity in proton proton collisions? 230 00:21:07,230 --> 00:21:10,140 So what's your current understanding? 231 00:21:12,360 --> 00:21:17,760 So can we start with Zana? Elise from Elise? I think actually, this was a 232 00:21:17,760 --> 00:21:23,940 question from, from your motivations like, yeah, this is actually well from if you 233 00:21:23,940 --> 00:21:28,590 remember the blog that I showed for VM coefficients, I can also share it again, 234 00:21:28,590 --> 00:21:34,590 but maybe you remember this points for BB collisions where we see even the results 235 00:21:34,590 --> 00:21:40,020 for higher full harmonics actually speed to six for example, staying there for up 236 00:21:40,020 --> 00:21:44,430 collisions up to the very down very low multiplicity sexually the lowest 237 00:21:44,430 --> 00:21:49,140 multiplicity that is possible there MVP. So what's the lowest multiplicity? I think 238 00:21:49,140 --> 00:21:52,560 it's around 10 tracks or so. And tracks. 239 00:21:54,540 --> 00:21:56,100 Yeah, okay. 240 00:21:59,640 --> 00:21:59,970 Can 241 00:22:00,359 --> 00:22:05,819 CMS? Yeah. A find that a very scary question. 242 00:22:06,839 --> 00:22:07,919 Okay, could you comment? 243 00:22:12,090 --> 00:22:12,900 Yeah, I 244 00:22:16,260 --> 00:22:20,190 think I think my honest answer is that I don't know. Hey, okay. A 245 00:22:21,870 --> 00:22:25,590 we can, you can. I'm confident above 100. And then 246 00:22:27,960 --> 00:22:32,880 hey, yeah, you were going to do a multivariate kind of look at this overall. 247 00:22:34,350 --> 00:22:40,380 And I, so I think it would be something to combine. I mean, it would be nice to 248 00:22:40,380 --> 00:22:44,550 combine the results of all the experiments and try to really nail this nail this 249 00:22:44,550 --> 00:22:44,880 down. 250 00:22:46,470 --> 00:22:50,910 I think that's a wonderful question. It's just I just find it very hard. 251 00:22:53,490 --> 00:22:59,940 Maybe just a comment from the Atlas side in the Atlas and CMS 252 00:23:00,269 --> 00:23:07,529 data down to the lowest multiplicities, you know, or 10 or even lower are in 253 00:23:07,529 --> 00:23:15,779 agreement. But in the Atlas paper, they extract the two that continues is pretty 254 00:23:15,779 --> 00:23:20,999 flat into that region. Whereas CMS extracts a v2 that's basically really 255 00:23:20,999 --> 00:23:27,959 dropping off. And that's just based on two different assumptions in the non flow 256 00:23:27,959 --> 00:23:33,239 subtraction method. And as far as I could, so it's not an experimental difference. 257 00:23:33,269 --> 00:23:39,179 It's a difference in the assumption used in the non flow subtraction. And as far as 258 00:23:39,179 --> 00:23:47,009 I know, no one has really figured out a way to validate or invalidate those 259 00:23:47,009 --> 00:23:52,289 particular assumptions. And I think that's a general problem at both Rick and the Lh 260 00:23:52,289 --> 00:23:59,969 see is when you have a very large non flow contribution, you're very susceptible 261 00:24:00,000 --> 00:24:05,910 To the assumptions of the non flow subtraction, if it's a pretty modest 262 00:24:05,910 --> 00:24:09,750 subtraction, then it's a small, systematic and it doesn't matter so much. So I think 263 00:24:09,750 --> 00:24:11,310 that's still quite open. 264 00:24:12,840 --> 00:24:17,760 That's Jimmy's right? That's part of why we were trying to do theism cumulants with 265 00:24:17,790 --> 00:24:23,460 with different sub event, but I certainly think we probably need theoretical health. 266 00:24:26,100 --> 00:24:29,670 Because the data is very good. And it's and it's not contradictory between the 267 00:24:29,670 --> 00:24:30,420 experiments. 268 00:24:33,030 --> 00:24:38,130 Okay, Alexa, has something to say. I'm wondering if it's related to this 269 00:24:38,130 --> 00:24:44,220 question, or is it a separate question, a different question. It's maybe related, 270 00:24:44,220 --> 00:24:52,080 but not exactly, um, is in order to provide more maybe fear understanding. So 271 00:24:52,110 --> 00:24:56,940 what were challenges of, you know, applying our typical models of heavy hand 272 00:24:56,940 --> 00:24:59,970 collisions into very small systems. Of course, we have 273 00:25:00,000 --> 00:25:05,280 Breaking manual of assumptions in many of these models. And there's one particular 274 00:25:05,340 --> 00:25:10,710 aspect that how we do conduct how do we produce particles at a final state from a 275 00:25:10,710 --> 00:25:14,760 fluid is by doing a Cooper fry freeze out. So, we do a 276 00:25:15,809 --> 00:25:20,819 particle ization and often it relies from you know, the fact that system is 277 00:25:20,849 --> 00:25:24,989 sufficiently close to thermal equilibrium that we know what kind of hardware 278 00:25:24,989 --> 00:25:31,409 distributions we should use. However, if a system is really freezing out without 279 00:25:31,409 --> 00:25:36,089 reaching equilibrium in very unusual traffic state, there is no general 280 00:25:36,089 --> 00:25:41,219 prescription how to convert such a matter into into particles. However, what we 281 00:25:41,219 --> 00:25:47,309 could maybe be better at constraining is what is the energy flow in respective law 282 00:25:47,309 --> 00:25:52,049 what is the conversion to matter, but that will require knowing the flow in terms of 283 00:25:52,079 --> 00:25:58,169 energies than particles. So, my question to experimental This is what is there any 284 00:25:58,169 --> 00:25:59,969 fundamental difference in our 285 00:26:00,480 --> 00:26:06,360 Calculating the particle of correlations and Particle Flow or energy correlation 286 00:26:06,360 --> 00:26:07,380 and energy flow. 287 00:26:11,580 --> 00:26:16,500 So you I think that's a very good point and he sounds like Mike Tannenbaum. 288 00:26:16,500 --> 00:26:20,670 They're always telling us to look at the flow of energy. I think experiments could 289 00:26:20,670 --> 00:26:24,150 certainly do that, which is a combination of energy. It's a good idea. 290 00:26:26,580 --> 00:26:31,140 I mean, I guess one thing is the the PT cutoff of the experiments, 291 00:26:32,250 --> 00:26:36,660 if you want the total energy, and isotropy is the limitation. 292 00:26:43,050 --> 00:26:46,380 But I think other than that, I don't see a particular 293 00:26:47,610 --> 00:26:53,580 limitation. I think it's the opposite because the energy is less sensitive to 294 00:26:53,670 --> 00:26:58,890 cut than particle yield, because you have an extra power of PT 295 00:27:00,599 --> 00:27:05,729 Right, but what we measure, like I showed in my talk, we're measuring, say v2 versus 296 00:27:05,729 --> 00:27:14,039 PT. So we show the v2 over the PT range that we measure. But if you wanted a v2, 297 00:27:14,729 --> 00:27:19,439 integrated overall PT or integrated overall energy, you have to integrate down 298 00:27:19,439 --> 00:27:23,459 to zero. So there's a region where all experiments at some point don't measure. 299 00:27:24,630 --> 00:27:27,510 I don't know how large an effect that would would be 300 00:27:28,800 --> 00:27:30,570 in terms of an uncertainty. 301 00:27:32,940 --> 00:27:39,270 Mitchell, I haven't seen such a such measurement. Is it correct or 302 00:27:40,560 --> 00:27:45,750 it seems I'm not the first one to have suggested? I think if you have the like 303 00:27:45,750 --> 00:27:52,140 from a least the particle spectra and the v2 versus PT, for the different p IDs, you 304 00:27:52,140 --> 00:27:56,310 can calculate it from that this Yeah, you should be able to just just 305 00:28:01,949 --> 00:28:05,669 I think it's implicit in those two. 306 00:28:09,000 --> 00:28:09,660 parabolas. Yeah. 307 00:28:17,250 --> 00:28:23,550 All right. Okay. Do we have do you do you have other questions? I think there was a 308 00:28:23,550 --> 00:28:30,390 question from a Christian before. I'm wondering if he still wants to 309 00:28:33,060 --> 00:28:34,530 ask his question. 310 00:28:39,630 --> 00:28:45,120 It was pretty much settled previously. Thank you. Okay. Thank you. 311 00:28:46,680 --> 00:28:50,160 Anyone else wants to ask a question. 312 00:28:57,210 --> 00:28:58,980 Okay, there's a question from you. 313 00:29:01,290 --> 00:29:05,130 Instead of questions more like a common rule will be discussed, which is very 314 00:29:05,130 --> 00:29:11,460 nice. And for the how low democracy we can go to may flow collectivity. But I'm 315 00:29:11,460 --> 00:29:15,360 really afraid already for the ongoing discussion forum for these templates 316 00:29:15,360 --> 00:29:17,820 versus the prefer subtraction which is unclear as 317 00:29:18,840 --> 00:29:24,870 was already mentioned by Jimmy, but by I varied is the method of the peripheral 318 00:29:24,870 --> 00:29:29,820 subject in itself, because, if you mean this method already assume there's no flow 319 00:29:30,120 --> 00:29:34,860 at the lower symmetries of the region. So, if you apply this method depends on how 320 00:29:34,860 --> 00:29:40,770 low and you treat as no flow region and then you will not get flow by default. So 321 00:29:40,770 --> 00:29:46,080 for CMS, if you treat authenticity below 20 as lowest democracy division and you 322 00:29:46,080 --> 00:29:50,400 don't expect any flow you will get zero. So I am afraid the conclusion might 323 00:29:50,400 --> 00:29:52,350 depends on the method you are applying. 324 00:29:54,600 --> 00:29:57,090 Yes, we're definitely trying to go beyond that. 325 00:29:59,280 --> 00:29:59,970 With with 326 00:30:00,659 --> 00:30:02,429 Essentially multiple observables 327 00:30:04,710 --> 00:30:05,940 as a function multiplicity 328 00:30:08,820 --> 00:30:13,680 we will we will keep trying to, to hack at this, look at this. 329 00:30:14,790 --> 00:30:20,580 But I agree, you kind of just say that there's no flow by default to you. It's 330 00:30:20,580 --> 00:30:21,120 better to 331 00:30:25,950 --> 00:30:29,070 measure up measure all your variables as a function of multiplicity and then look at 332 00:30:29,070 --> 00:30:29,760 the total picture. 333 00:30:35,460 --> 00:30:40,950 Okay, thank you any federal question or input to the discussion, comment? 334 00:30:49,080 --> 00:30:58,530 Okay, I don't see any raised hands. So I think it's time to conclude. Okay, so I'd 335 00:30:58,530 --> 00:31:00,000 like to thank you 336 00:31:00,000 --> 00:31:06,600 speakers for inspiring talks given in this session, and I'd like to thank everyone 337 00:31:06,600 --> 00:31:12,060 who has contributed to our discussions. Also, I'd like to remind you that 338 00:31:14,429 --> 00:31:20,669 tomorrow there is dedicated john session between the heavier loads and the QC D on 339 00:31:20,789 --> 00:31:25,499 initial state nuclear PDFs and other topics. So if you are interested, please 340 00:31:25,499 --> 00:31:34,379 join Friday at 1230 same time. Okay, I think we are done. So thank you everyone, 341 00:31:34,469 --> 00:31:39,509 and the session is closed. Thank you to the organizers. Thank you organizers 342 00:31:39,629 --> 00:31:42,419 Alison Lena aunty Thank you much