1 00:00:02,129 --> 00:00:08,129 Which will be an overview of ALICE status from Andrea Dainese. 2 00:00:10,439 --> 00:00:13,949 So whenever you're ready to share your screen, go ahead and you can start 3 00:00:14,189 --> 00:00:14,999 whenever you like. 4 00:00:15,810 --> 00:00:19,320 Hello, good afternoon. I'm sharing my screen. 5 00:00:20,130 --> 00:00:24,960 So I tried to open my camera but didn't manage to so I flash here a picture of 6 00:00:24,960 --> 00:00:27,840 myself so that you know who I am. 7 00:00:29,310 --> 00:00:33,780 And could you please confirm that you can see my screen? Yes. 8 00:00:34,830 --> 00:00:40,770 Okay. So good morning, everyone. It is my pleasure to present the highlights and 9 00:00:40,770 --> 00:00:45,420 perspectives from ALICE. And of course, we thank the organizers for the 10 00:00:45,420 --> 00:00:46,350 invitation. And I 11 00:00:46,350 --> 00:00:48,900 also thank the collaboration for preparing so many 12 00:00:48,900 --> 00:00:54,720 nice results that I can show you today. So we have in ALICE, more than 1000 signing 13 00:00:54,720 --> 00:01:02,640 authors from over 39 countries and in terms of papers we reached around 300 today with 14 00:01:02,670 --> 00:01:07,470 eight new papers and we have seven more in the pipeline. So in total 15 papers for 15 00:01:07,470 --> 00:01:13,350 this conference and hard probes next week. The table shows our harvest from run 16 00:01:13,350 --> 00:01:17,280 one and two. And of course, we are grateful to the LHC team for always 17 00:01:17,280 --> 00:01:25,320 providing high success run. So I don't have to introduce too much our detector to 18 00:01:25,320 --> 00:01:30,570 this audience I guess. We have a central barrel with tracking hadron electron 19 00:01:30,570 --> 00:01:37,740 photon and jet reconstruction and the forward muon spectrometer and this is how 20 00:01:38,010 --> 00:01:41,910 the central barrel looked like when we opened the magnet doors at the beginning of 21 00:01:41,910 --> 00:01:49,080 LS two to start our major upgrade. Now, I will start now by presenting our 22 00:01:49,080 --> 00:01:54,840 recent highlights, so I start from our core business so to speak, lead lead collisions 23 00:01:54,870 --> 00:02:00,450 and the study of the deconfined phase of QCD matter, the quark gluon plasma, which forms 24 00:02:00,450 --> 00:02:05,070 when the energy density is larger than oh point five GeV per fermi cube. So in LHC 25 00:02:08,520 --> 00:02:14,340 in LHC lead lead collisions we reach well eyond that over a large volume. 26 00:02:15,210 --> 00:02:20,310 So I will present the results following a bit the time evolution of the 27 00:02:20,340 --> 00:02:25,620 collision. I start with a macroscopic property, vorticity, that we started 28 00:02:25,620 --> 00:02:30,780 recently to study. So in case of non central collisions, the system has a large 29 00:02:30,810 --> 00:02:37,500 angular momentum, and spin orbit interactions may polarize the quarks and 30 00:02:37,500 --> 00:02:43,380 lead to a visible spin alignment for the vector mesons. And if you see here, in 31 00:02:43,380 --> 00:02:48,780 red, we show an effect at low pT in non centralKcollisions for the k star which is 32 00:02:48,780 --> 00:02:54,000 a spin one, and this is the deviation with respect to the one third the value of this 33 00:02:54,030 --> 00:03:00,480 row 00 variable, which we find as a good cross check in pp collisions, and for the K 34 00:03:00,480 --> 00:03:07,140 zero, which is spin one. Now, moving ahead, one of the characterizing features of the 35 00:03:07,200 --> 00:03:13,530 QGP is of course color deconfinement and there the prime tool to study are 36 00:03:13,950 --> 00:03:21,810 quarkonia, so, heavy quark bound states. So, at the LHC, we are in a regime in 37 00:03:21,810 --> 00:03:27,870 which the melting due to color screening, color dissociation which is pictured 38 00:03:27,870 --> 00:03:28,380 here 39 00:03:28,710 --> 00:03:35,970 on the left is in part compensated by regeneration in case of charm because 40 00:03:35,970 --> 00:03:42,000 there is a high density of charm quarks in the system. So, here I show our latest 41 00:03:42,000 --> 00:03:46,170 results for the nuclear modification factor of the J/psi in central lead lead 42 00:03:46,170 --> 00:03:51,570 collisions. So, this is the lead lead yield over the pp yield the scaled by the number 43 00:03:51,570 --> 00:03:56,730 of binary nuclear nuclear collisions. So, at high pT you see we have a suppression 44 00:03:56,730 --> 00:04:02,010 of a factor five which is described by models in terms of color screening or 45 00:04:02,010 --> 00:04:06,990 energy loss of the J/psi. And then when we go to low pT, and this is something 46 00:04:06,990 --> 00:04:11,670 that has been seen only at the LHC and not at lot lower energies, we see that the 47 00:04:11,670 --> 00:04:19,590 suppression is is lifted, there is an increase. And this is the effect of 48 00:04:19,590 --> 00:04:24,900 regeneration that I mentioned, it is described by models, and it is also 49 00:04:25,050 --> 00:04:30,900 supported by the fact that that when we go to central rapidity, so from red to black, 50 00:04:31,170 --> 00:04:35,610 we see more of that, and this is consistent with a higher density of 51 00:04:35,640 --> 00:04:42,210 C quarks at central rapidity. So moving on parton interactions in the system are a 52 00:04:42,210 --> 00:04:48,210 powerful tool to understand its properties. And also to understand how 53 00:04:48,240 --> 00:04:54,390 parton dynamics works in a high density deconfined system. So there the main 54 00:04:54,390 --> 00:05:00,840 tools are jets. I start by showing the jet quenching in terms of nuclear modification 55 00:05:00,840 --> 00:05:04,680 factor of the jet yield, So how much is the jet yield 56 00:05:05,460 --> 00:05:06,210 reduced 57 00:05:06,390 --> 00:05:11,970 and this is again central lead lead collisions divided by proton proton. So in 58 00:05:11,970 --> 00:05:17,760 the central plot I show our recently published result for R equal Oh point 59 00:05:17,760 --> 00:05:27,030 two where we started from 40 GeV. And in the right hand side plot, I show a new 60 00:05:27,030 --> 00:05:33,510 result where we explore machine learning techniques to separate the larger 61 00:05:33,510 --> 00:05:39,360 underlying event energy fluctuations from the jet components. And this allows us to 62 00:05:39,360 --> 00:05:46,980 go down to 40 GeV also for a larger resolution parameter of 0.4 with a caveat 63 00:05:46,980 --> 00:05:56,340 that this may be somehow biased because we train on Pythia. But overall, we see a 64 00:05:56,340 --> 00:06:02,700 reduction of a factor three to four of the jet yield down to 40 GeV, so this suggests 65 00:06:02,700 --> 00:06:08,970 that the lost energy when we have medium induced gluon radiation is not 66 00:06:08,970 --> 00:06:14,280 recovered in the jet cone. So, this radiation occurs predominantly at larger 67 00:06:14,700 --> 00:06:21,870 angles. Now to study more the dynamics of jet interactions in the medium, we 68 00:06:21,870 --> 00:06:26,940 have started a broad set of jet substructure measurements. Here I will 69 00:06:26,940 --> 00:06:33,150 just show one example. So, we use the grooming technique to go and look for the 70 00:06:33,150 --> 00:06:37,860 first hard splitting. And essentially we measure the angular 71 00:06:37,860 --> 00:06:43,620 distribution between the two prongs. And in the figure you see at large angles 72 00:06:43,620 --> 00:06:49,410 close to one we see a suppression in central dijet with respect to pp collisions, 73 00:06:50,070 --> 00:06:57,150 which suggests that the jet core is more collimated in lead lead collisions with 74 00:06:57,150 --> 00:07:03,870 respect to pp. Now, let me make a small QCD interlude where I will show a couple 75 00:07:03,870 --> 00:07:08,250 of proton proton results. So, we use this substructure 76 00:07:09,780 --> 00:07:11,370 technology so to speak, 77 00:07:11,700 --> 00:07:17,160 to carry out measure many measurements. And in particular here I show how we 78 00:07:17,400 --> 00:07:23,760 dissect the soft charm jets using the grooming technique again and we count 79 00:07:23,760 --> 00:07:29,670 the number of hard splittings in the jet fragmentation with momentum radiation 80 00:07:29,670 --> 00:07:35,610 larger than 10% and here in the figure so here we use jets tagged with the 81 00:07:35,610 --> 00:07:41,250 D mesons with pT larger than five GeV and here we plot the number of these 82 00:07:41,250 --> 00:07:47,580 splittings and we see that for charm jets this is shifted towards lower 83 00:07:47,580 --> 00:07:52,320 splittings by about one unit with respect to inclusive jets. And this is 84 00:07:52,320 --> 00:07:57,000 connected to the harder fragmentation of heavy with respect to light quarks and 85 00:07:57,000 --> 00:08:03,180 gluons. In pp collisions we have also recently exposed for the first 86 00:08:03,180 --> 00:08:10,920 time the dead cone effect in in for heavy quarks. So this effects is predicted to 87 00:08:10,920 --> 00:08:18,570 reduce gluon radiation at small angles from heavy quarks and here we use iterative 88 00:08:18,600 --> 00:08:25,800 declustering and the Lund plane analysis to compare the D0 jets and the inclusive 89 00:08:25,800 --> 00:08:32,490 jets as you see here in the smaller plots. And when we translate this into a 90 00:08:32,490 --> 00:08:37,500 measurement as a function of radiation angle, and we make a ratio of charm over 91 00:08:37,500 --> 00:08:43,170 inclusive, we see a suppression at small angles which is what is predicted by by 92 00:08:43,170 --> 00:08:48,840 the jet cone mechanisms and it is actually well described by Pythia for example. So the 93 00:08:48,840 --> 00:08:55,560 jet cone in the case of lead lead collisions and medium induced gluon radiation has been 94 00:08:55,560 --> 00:09:04,020 predicted almost 20 years ago to lead the to a reduction of energy loss from 95 00:09:04,020 --> 00:09:09,480 b works with respect to c quarks, due to the larger mass, and now we have a 96 00:09:09,480 --> 00:09:14,250 measurement that is sensitive to that. We measured the nuclear modification 97 00:09:14,250 --> 00:09:21,090 factor of non prompt D0 mesons in blue compared to that of prompt 98 00:09:21,090 --> 00:09:26,640 D0 mesons. So, they probe b and c quarks respectively. And we see that for, 99 00:09:26,640 --> 00:09:31,170 for the case of b quarks there is less suppression, which is well described by 100 00:09:31,170 --> 00:09:34,350 the models that implement radiative energy loss 101 00:09:34,380 --> 00:09:36,390 with the dead cone effect. 102 00:09:37,980 --> 00:09:43,830 Now, moving ahead with the evolution of the system, it is extremely interesting to 103 00:09:43,830 --> 00:09:54,270 study the expansion dynamics, which is well described by hydrodynamic simulations and 104 00:09:54,270 --> 00:10:01,110 also allow us to extract characterizing processes of the QGP. So, here it is 105 00:10:01,110 --> 00:10:05,880 useful to consider non central collisions, in which there is an elongated 106 00:10:05,880 --> 00:10:10,800 geometry from the beginning. And then during the expansion via pressure 107 00:10:10,800 --> 00:10:15,960 gradients, this maps into an azimuthal modulation in momentum space that we 108 00:10:15,960 --> 00:10:20,880 analyzed with Fourier decomposition and the second coefficient, the v2, 109 00:10:20,880 --> 00:10:26,160 is called elliptic flow, it quantifies the dominant elliptic modulation. So, here 110 00:10:26,160 --> 00:10:32,400 you see our latest results on the left for six different hadron species, 111 00:10:33,269 --> 00:10:39,839 we see at low momentum circled in yellow an ordering the mass, and that if you look 112 00:10:39,839 --> 00:10:46,019 on the right we even see when we take light nuclear with A equals two and A equals 113 00:10:46,019 --> 00:10:53,129 three that we measured recently. So, this suggests that particles participate in the 114 00:10:53,129 --> 00:10:58,349 collective expansion. There is a common flow velocity that imparts to hadrons 115 00:10:58,349 --> 00:11:03,269 an additional momentum, a momentum shift, which is proportional to their 116 00:11:03,269 --> 00:11:08,399 mass. Now instead at intermediate momenta here in green, we see a clear 117 00:11:08,399 --> 00:11:16,919 separation between baryons and mesons. And this suggests that in this 118 00:11:16,919 --> 00:11:23,609 momentum range, the flow is carried by quarks and it is then propagated to 119 00:11:23,609 --> 00:11:30,389 hadrons via an hadronisation process, at least in part by recombination similar 120 00:11:30,389 --> 00:11:37,379 to what I mentioned for the J/psi. So, now these very high precise data are used 121 00:11:37,409 --> 00:11:44,549 by theory groups with sophisticated statistical techniques like Bayesian 122 00:11:44,549 --> 00:11:52,169 procedures to really extract the properties of the system. And this, for 123 00:11:52,169 --> 00:11:57,629 example, uses the hydrodynamic simulation that I showed at the beginning. So, 124 00:11:57,629 --> 00:12:02,429 here I focus on one of the really characterising properties of the QGP, the 125 00:12:02,429 --> 00:12:07,109 shear viscosity versus temperature. And you see it is now determined with the 126 00:12:07,109 --> 00:12:11,939 precision of 20% and it is found to be 10 times 127 00:12:12,630 --> 00:12:15,240 smaller than for any other form of matter. 128 00:12:17,190 --> 00:12:25,260 So, today we put out our final full run two results for also flow measurements 129 00:12:25,260 --> 00:12:33,150 involving heavy works, both charm and beauty. So, these are compiled in this in this 130 00:12:33,150 --> 00:12:39,270 figure, that you see, and we see that D mesons, in orange, and J/psi, in red, 131 00:12:39,300 --> 00:12:41,070 exhibit a large flow. 132 00:12:42,660 --> 00:12:45,060 They are, they are ordered and both are both 133 00:12:45,480 --> 00:12:52,260 both are lower than that of pions in in black. So, this is consistent with a 134 00:12:52,260 --> 00:12:57,990 scenario which is implemented in model calculations that describe the data in 135 00:12:57,990 --> 00:13:05,130 which both light and charm quarks participate in the expansion of the system, 136 00:13:05,130 --> 00:13:11,160 they carry some some flow, and that by the charm quarks to a smaller extent than 137 00:13:11,160 --> 00:13:16,470 light quarks. And then at least in this momentum range they form these hadrons 138 00:13:16,890 --> 00:13:22,980 via recombination. So we also see that B mesons are sensitive to the 139 00:13:22,980 --> 00:13:28,080 elongated shape of the system. These are the purple points, while the very heavy 140 00:13:28,110 --> 00:13:34,290 Upsilon 1S doesn't show a significant flow signal in blue. And this 141 00:13:34,290 --> 00:13:40,500 is consistent with its very large mass and also with a small regeneration probability 142 00:13:40,860 --> 00:13:47,610 in case of beauty. Now, in the second part of the highlights, I will show a selection 143 00:13:47,610 --> 00:13:53,070 of results that give you an idea of the very comprehensive QCD program that we 144 00:13:53,070 --> 00:14:00,720 have beyond QGP studies. So this really sparked with LHC surprises and 145 00:14:00,840 --> 00:14:07,350 new findings and especially with the high luminosity pp and p lead samples of run two 146 00:14:09,480 --> 00:14:16,080 this this these measurements have been developed very significantly. So, I 147 00:14:16,080 --> 00:14:24,240 start from small systems and it is already well known since some time that we 148 00:14:24,240 --> 00:14:31,740 see in pp and p lead collisions at high particle multiplicity effects that look 149 00:14:31,740 --> 00:14:38,670 like what we see in lead lead collisions. So, here I show some updates. On the left, 150 00:14:39,210 --> 00:14:39,960 you see 151 00:14:41,340 --> 00:14:43,290 the strangeness over pion 152 00:14:44,610 --> 00:14:50,460 plot as a function of multiplicity which we published for pp collisions in Nature 153 00:14:50,460 --> 00:14:57,240 Physics in 2017. Now, it contains four different colliding systems including 154 00:14:57,240 --> 00:15:02,430 xenon xenon, and also different center of mass energies and we see a 155 00:15:02,430 --> 00:15:08,580 smooth path across the systems. So it seems to be driven by multiplicity and 156 00:15:08,580 --> 00:15:15,180 also independent of square root of s and there is a steeper rise in within the small 157 00:15:15,180 --> 00:15:20,250 systems for increased strangeness content and at high multiplicity in small 158 00:15:20,250 --> 00:15:27,240 systems values similar to those in lead lead are reached. On the right, I show 159 00:15:27,240 --> 00:15:34,200 also a plot that we published last year in which we compiled elliptic flow 160 00:15:34,200 --> 00:15:40,320 measurements in the four colliding systems that we had. And also in this case, we see 161 00:15:40,320 --> 00:15:47,490 in high multiplicity pp and p lead collisions, clear elliptic flow signal, so v2 larger 162 00:15:47,490 --> 00:15:53,880 than zero, and similar to lead lead at the same multiplicity. So now, here I show a new 163 00:15:53,880 --> 00:15:55,470 result that we have just 164 00:15:55,710 --> 00:15:57,540 prepared for this conference, 165 00:15:57,990 --> 00:16:03,360 which is related to elliptic flow in pp collisions, we have measured it over the 166 00:16:03,390 --> 00:16:11,340 maximum possible delta eta separation. So, we use hadron pairs separated by six units in 167 00:16:11,610 --> 00:16:17,250 in eta, as you see in the sketch. And in high multiplicity collisions we 168 00:16:17,250 --> 00:16:19,950 clearly see up to this high separation, 169 00:16:21,090 --> 00:16:23,250 the so called near side, 170 00:16:26,010 --> 00:16:35,130 near side ridge, which is a characteristic of this flow modulation. And we see it up to 171 00:16:35,130 --> 00:16:41,520 this delta eta which supports the idea that this is truly collective correlations between 172 00:16:41,580 --> 00:16:47,730 between hadrones and when we represent the v2 parameter for different colliding 173 00:16:47,730 --> 00:16:53,100 systems as you see here, on the right at similar multiplicity, we find that that it 174 00:16:53,100 --> 00:16:59,790 has a similar magnitude. Now, in pp collisions, it is also interesting to look 175 00:16:59,790 --> 00:17:07,800 for low mass dielectron production and this we have done using our samples 176 00:17:07,800 --> 00:17:11,910 that we collected with lower magnetic field in the central barrel to have higher 177 00:17:11,910 --> 00:17:18,060 acceptance at very low momentum. And we see a hint of an excess here over the 178 00:17:18,060 --> 00:17:23,640 hadron cocktail at low mass and low pT. And this is quite interesting because it 179 00:17:23,640 --> 00:17:30,870 is reminiscent of an effect an excess that was seen for real and virtual photons in 180 00:17:30,870 --> 00:17:37,590 the 80s. And also interestingly this cannot be described by calculations either 181 00:17:37,590 --> 00:17:43,830 using hadronic bremsstrahlung or even radiation from a mini QGP. So this 182 00:17:44,279 --> 00:17:46,469 clearly deserves some more investigation. 183 00:17:46,890 --> 00:17:50,790 Andrea, just slightly less than three minutes. Thank you. 184 00:17:51,599 --> 00:17:57,569 So, in proton proton we have also several measurements concerning hadronization of 185 00:17:57,569 --> 00:18:03,989 charm. Here I show baryon over meson ratios. So, on the left the lambda c was 186 00:18:03,989 --> 00:18:09,059 already shown to be increased with respect to e+ e- expectations and 187 00:18:09,059 --> 00:18:14,129 now we see that this increase depends on multiplicity in pp. And we also measure 188 00:18:14,129 --> 00:18:21,539 the sigma c and xi c which also exhibit large increases. And for example, the 189 00:18:21,539 --> 00:18:29,489 sigma c is not described by any tune of Pythia even with the color reconnection. Now, 190 00:18:29,909 --> 00:18:35,849 the LHC is not only a nucleus collider but also an anti nuclear nuclear factory. We 191 00:18:35,849 --> 00:18:42,509 measured them by using our TPC and time of flight. The production mechanism is not 192 00:18:42,509 --> 00:18:42,749 yet 193 00:18:42,750 --> 00:18:43,830 fully understood. 194 00:18:44,160 --> 00:18:47,850 It can be described in terms of nucleon coalescence or statistical 195 00:18:47,850 --> 00:18:52,740 hadronisatino. But today I want to focus on an aspect that is 196 00:18:52,770 --> 00:18:55,380 a strong implication on the dark matter searches 197 00:18:55,380 --> 00:19:01,740 in space, for example, from a neutralino annihilation to anti deuteron anti helium 198 00:19:01,740 --> 00:19:07,410 three. Now these searches are affected by large uncertainties due to the limited 199 00:19:07,410 --> 00:19:13,590 knowledge of the ordinary hadron production by cosmic, so anti nuclei, and also their 200 00:19:13,590 --> 00:19:20,640 absorption in space. And so today we provide new measurements that give 201 00:19:20,640 --> 00:19:27,600 insights in both directions. On the left, you see our deuteron over proton ratio as a 202 00:19:27,600 --> 00:19:33,600 function of multiplicity and we just published the data in yellow, pp at 13 TeV. 203 00:19:33,870 --> 00:19:38,820 So, this clearly constraints the production models. And on the right, we 204 00:19:38,820 --> 00:19:43,080 measured for the first time at low momentum, the anti deuteron absorption 205 00:19:43,080 --> 00:19:47,640 cross section in the ALICE material. And this is very interesting because at 206 00:19:47,640 --> 00:19:53,460 low momentum this is larger than the state of the art modelling. So the last result 207 00:19:53,490 --> 00:20:02,280 that I want to highlight is a study of QCD interactionos among hadrons using 208 00:20:02,490 --> 00:20:10,140 essentially proton hyperon pairs, and their momentum correlation is sensitive to the 209 00:20:10,170 --> 00:20:11,430 strong interaction 210 00:20:11,460 --> 00:20:14,340 potential. This is a field that, an 211 00:20:16,170 --> 00:20:23,160 interaction potential that is not well measured and high statistics data from the LHC 212 00:20:23,160 --> 00:20:29,520 are really a breakthrough. So, here we present the proton xi minus and proton 213 00:20:29,550 --> 00:20:36,120 omega minus correlation, which now precisely show an attractive strong 214 00:20:36,120 --> 00:20:42,120 interaction in addition to the Coulomb interaction. So, in the last couple of 215 00:20:42,120 --> 00:20:47,430 minutes, I will show the perspectives, we are preparing for run three and run four. 216 00:20:47,430 --> 00:20:53,910 Our major upgrade is taking shape, it will be discussed in detail later by 217 00:20:53,910 --> 00:20:59,790 Piotr. So, overall, we aim at improving the tracking resolution at low pT and 218 00:21:00,510 --> 00:21:07,260 increasing by a factor of 50 the readout capabilities. So the impact of the 219 00:21:07,260 --> 00:21:13,680 COVID-19 at present is quantified into a delay of 4.5 months, which means that we 220 00:21:13,680 --> 00:21:19,350 will be ready for begin commissioning at the end of August of next year. So here I 221 00:21:19,350 --> 00:21:25,650 just flash a couple of major highlights. The TPC is already instrumented with 222 00:21:25,650 --> 00:21:32,850 GEM chambers, and, while the old ITS is serving in the ALICE exhibition, the new 223 00:21:32,850 --> 00:21:38,370 one together with the muon forward tracker fully made of pixels are ready for 224 00:21:38,490 --> 00:21:44,520 installation. So we are also proposing upgrades for LS three. On the left, a 225 00:21:44,520 --> 00:21:50,100 forward electromagnetic calorimeter with high granularity readout to 226 00:21:50,100 --> 00:21:55,530 measure photons in p lead, down to 10 to the minus five in x which are sensitive 227 00:21:55,530 --> 00:22:00,300 to the gluon density in a region where it is essentially unconstrained and where 228 00:22:00,300 --> 00:22:08,010 gluon saturation may set in, and at central rapidity, we are considering and proposing 229 00:22:08,010 --> 00:22:14,070 to replace the inner barrel of the ITS with three truly cylindrical maps layers 230 00:22:14,340 --> 00:22:18,960 with much better performance. And you see we are already testing the curved 231 00:22:18,990 --> 00:22:25,650 sensors. Now pushing farther this idea of ultra thin filling silicon detectors we 232 00:22:25,650 --> 00:22:32,040 are preparing a proposal for a silicon only, so to speak, heavy ion experiment for 233 00:22:32,040 --> 00:22:38,190 beyond run four, which would be fast, ultra thin and provide essentially 234 00:22:38,220 --> 00:22:43,830 ultimate performance for several probes like multi heavy flavor, thermal radiation, and 235 00:22:43,830 --> 00:22:50,070 soft, very soft hadron production. And those who could exploit the higher LHC 236 00:22:50,070 --> 00:22:56,880 luminosity that the LHC could be provided with nuclei lighter than lead. 237 00:22:58,050 --> 00:23:02,490 So to conclude we have a large number of results based on full run two samples. 238 00:23:03,060 --> 00:23:09,510 Not only they provide insight on the QGP workings and properties but also on a much 239 00:23:09,510 --> 00:23:16,770 broader QCD research program. Our major upgrade is on track to be ready for pp 240 00:23:16,770 --> 00:23:22,170 collisions at the end of August next year. And we are getting up for LS three 241 00:23:22,230 --> 00:23:31,050 upgrades and planning for run five and beyond. So in thanking you I inviting you 242 00:23:31,080 --> 00:23:36,840 to enjoy the 29 talks and posters with ALICE presenters that we have at the 243 00:23:36,840 --> 00:23:38,940 conference. Thank you. 244 00:23:40,470 --> 00:23:41,610 Okay, thank you, Andrea. 245 00:23:42,869 --> 00:23:46,769 This nice summary. And we have a question. 246 00:23:48,240 --> 00:23:50,760 Marek. Hold on. 247 00:23:52,529 --> 00:23:55,019 I can allow. Okay, Marek should be able to unmute. 248 00:23:57,180 --> 00:24:06,600 Ah, so two questions. One is, is there any data about pT, transverse momentum 249 00:24:06,600 --> 00:24:14,160 dependence, of the anti deuteron production? This is very relevant for some 250 00:24:14,160 --> 00:24:21,270 issues regarding exotic hadrons where the deuteron is a well understood system. 251 00:24:23,700 --> 00:24:29,370 Yes, yes, we have also measurement of transverse momentum spectra of deuteron, and 252 00:24:29,370 --> 00:24:37,620 anti deuteron and even more light nuclei. So, I don't have backup figures here, but 253 00:24:37,860 --> 00:24:44,580 you can find them in our papers, for example the one that I linked here. 254 00:24:45,599 --> 00:24:51,689 Okay, thank you. And the second question is, you mentioned measuring interactions 255 00:24:51,689 --> 00:24:52,109 between, 256 00:24:57,720 --> 00:24:59,550 interactions between hadrons 257 00:25:01,500 --> 00:25:03,390 by measuring correlations. 258 00:25:05,220 --> 00:25:09,870 Can you look at correlations between protons and sigma c baryons? 259 00:25:14,730 --> 00:25:20,970 Well not with the statistics that we have from run two, we we have been able to 260 00:25:20,970 --> 00:25:26,910 measure sigma c production but likely there is not enough statistics to study 261 00:25:26,910 --> 00:25:31,530 correlations, but definitely this is something that we could consider 262 00:25:32,910 --> 00:25:33,690 for run three. 263 00:25:34,230 --> 00:25:43,440 It's highly relevant for understanding the nature of the hidden charm pentaquark 264 00:25:43,470 --> 00:25:45,660 that was discovered by LHCb. 265 00:25:49,349 --> 00:25:54,779 Okay, thank you. Thank you. Thank you for the suggestion. We will, we will look into 266 00:25:54,779 --> 00:25:55,139 it. 267 00:25:55,380 --> 00:25:59,520 Thank you. Okay. 268 00:26:01,140 --> 00:26:07,800 So I think if there are no other questions, we can thank Andrea again. Thank 269 00:26:07,800 --> 00:26:09,840 you. Thank you