1 00:00:01,230 --> 00:00:02,340 Yep, we see that's good. 2 00:00:02,460 --> 00:00:08,010 All right, very good. Okay, so I'll give you some selected highlights from the CMS 3 00:00:09,510 --> 00:00:16,590 HLS HCM program. Now of course, the aim of all this is to enable the full program for 4 00:00:16,590 --> 00:00:20,940 both precision measurements as well as direct searches for rare processes and 5 00:00:21,330 --> 00:00:25,980 subtle and or exotic signatures in the search for beyond the Standard Model 6 00:00:25,980 --> 00:00:34,680 physics in the pure environment of the HL hc. So you face three challenges, so the 7 00:00:34,680 --> 00:00:38,400 high radiation environment which necessitates the complete replacement of 8 00:00:38,400 --> 00:00:43,980 the tracker and then cap calorimeter systems, as well as the gold operation of 9 00:00:43,980 --> 00:00:49,530 the barrel decal to mitigate for increased noise in the PDS and also, of course, a 10 00:00:49,530 --> 00:00:54,210 major program of electronics overhaul and consolidation of the barrel counter 11 00:00:54,210 --> 00:01:00,720 emitters and systems behind pileup motivates improved granularity Wherever, 12 00:01:00,990 --> 00:01:06,840 wherever possible, as well as novel approaches to in time pilot mitigation, 13 00:01:06,930 --> 00:01:12,360 and in particular the use of precision timing detectors. And finally, the high 14 00:01:12,360 --> 00:01:16,950 luminosity requires substantially improved the level one trigger performances to 15 00:01:16,950 --> 00:01:22,860 offer better selectiveness despite because of the high rate of new physics or physics 16 00:01:22,860 --> 00:01:28,380 events, rather despite the high pileup environment, and a complete overhaul of 17 00:01:28,380 --> 00:01:33,480 the trigger and the ACU systems. And so it's these challenges that define the 18 00:01:33,480 --> 00:01:40,080 scope of the CMS HL will exceed upgrade program. Well, this is summarized in this 19 00:01:40,110 --> 00:01:47,610 somewhat busy slide, you see starting from the top right hand corner in blue. A 20 00:01:47,610 --> 00:01:53,580 summary of what I summarized as major electronics upgrade and consolidation for 21 00:01:53,580 --> 00:01:59,430 the barrel color amateurs and your systems on the left hand side and green the 22 00:01:59,430 --> 00:02:05,880 complete room placement of the tracker calorimeter endcap, as well as the level 23 00:02:05,880 --> 00:02:13,440 one trigger hltv cue chain. And finally on the bottom right hand side and purple new 24 00:02:13,440 --> 00:02:18,030 detector systems, of course, the most notable of these being the timing 25 00:02:18,030 --> 00:02:25,650 detector, but also a new gem and new generation RPC Yon chambers to augment the 26 00:02:25,890 --> 00:02:34,680 system. So, the scope of both for all this was set up in the conceptual design report 27 00:02:34,680 --> 00:02:40,500 and since then we have completed a series of TDR that detailed each of the different 28 00:02:40,500 --> 00:02:45,870 projects, the most recent of which being the trigger TDR, which is currently under 29 00:02:45,870 --> 00:02:52,560 review by the FCC. And we look forward to the remaining TDRS with the aq h lt and 30 00:02:52,560 --> 00:02:58,290 more specialized systems that's a Brill PPP PPS And finally, a computing TDR 31 00:03:00,420 --> 00:03:02,760 one slide is a teaser for the 32 00:03:04,020 --> 00:03:05,100 trigger TDR. 33 00:03:06,420 --> 00:03:13,560 On the top left hand side, you see a schema of the the level one trigger of 34 00:03:13,560 --> 00:03:19,500 CMS. And I've highlighted here two notable new ingredients of this. So there is a 35 00:03:19,500 --> 00:03:24,660 level one tracking trigger. And I'll have more about that in a moment. And then in 36 00:03:24,660 --> 00:03:29,280 yellow, you see that of course, having tracks available at the level one together 37 00:03:29,280 --> 00:03:35,130 with calorimeter. And new on primitives enables the use of Particle Flow that 38 00:03:35,610 --> 00:03:43,290 level one something that was previously deployed at the high level trigger. Moving 39 00:03:43,380 --> 00:03:48,810 on then to the starting, if you like from the inside out and looking now at the 40 00:03:49,200 --> 00:03:55,770 tracker with phase two tracker. On the top left hand side, you have the usual quarter 41 00:03:55,770 --> 00:04:01,200 layout view and you see and there are six tracking layers. Other tracking layers in 42 00:04:01,200 --> 00:04:06,900 the central region followed by a number of end caps and a substantially extended in 43 00:04:06,930 --> 00:04:11,610 pixel system. The goal of this is to provide an extended either coverage going 44 00:04:11,610 --> 00:04:18,780 beyond the previous coverage or beta 2.4 result. And all the way up to eat up for 45 00:04:18,780 --> 00:04:23,790 you see, do you see that and the plot at the top right hand side where the tracking 46 00:04:23,790 --> 00:04:30,480 points are shown. This of course is intended both to extend the acceptance but 47 00:04:30,480 --> 00:04:37,140 also to for pilot mitigation. For example, in terms of BPF, generally construction 48 00:04:37,980 --> 00:04:43,920 meant and so on. Now, one way we set up very aggressive target in terms of 49 00:04:43,920 --> 00:04:48,930 reducing the material budget on the top, the bottom right hand corner rather, you 50 00:04:48,930 --> 00:04:54,750 see a comparison between the material budget of the current tracker and that on 51 00:04:54,780 --> 00:04:59,340 the phase two tracker, it's a very dramatic change. You see that to the Pico 52 00:04:59,340 --> 00:05:05,400 material In the face to tracker is about 70% of the radiation length and that's 53 00:05:05,400 --> 00:05:12,120 half the material that's present in the current tracker. That was done in a number 54 00:05:12,120 --> 00:05:18,300 of ways. One of them is illustrated here in the bottom left hand corner, where as 55 00:05:18,300 --> 00:05:24,210 you can see in the overall layout we have for the entire three tracking layers. We 56 00:05:24,210 --> 00:05:28,920 have tilted sensors that are brought in to complement the standard the barrel and 57 00:05:28,920 --> 00:05:36,180 endcap sensor configurations. And on the next slide, you see that this has gone now 58 00:05:36,180 --> 00:05:44,970 from detailed design to quite advanced thermal mechanical mock ups. And here on 59 00:05:44,970 --> 00:05:49,950 the bottom right hand side we demonstrate Another feature of the design that is 60 00:05:49,950 --> 00:05:54,540 again used in this aggressive reduction and material budget and that is the 61 00:05:54,540 --> 00:05:59,820 deployment of co2 cooling. So these are cooling tests for one of these rather 62 00:05:59,820 --> 00:06:07,950 reasons Arctic tilted barrel sections and showing the excellent performance of the 63 00:06:07,950 --> 00:06:10,080 co2 cooling. And those structures 64 00:06:11,910 --> 00:06:13,470 are a key conceptual 65 00:06:14,880 --> 00:06:21,900 novelty of this phase two tracker was the introduction of so called for PT modules. 66 00:06:21,930 --> 00:06:29,160 So these are modules that integrate to closely spaced silicon layers. And as you 67 00:06:29,160 --> 00:06:33,930 can see by the diagram on the top left hand side, this allows to measure not only 68 00:06:33,930 --> 00:06:38,700 the position but actually the direction vector and the pipeline of particles that 69 00:06:38,700 --> 00:06:44,400 lets you combine in pairs of these hits into stop vectors if you like, let's see 70 00:06:44,400 --> 00:06:49,860 discriminate vectors, according to their curvature and the four Tesla field of the 71 00:06:49,890 --> 00:06:56,370 CMS, a superconducting magnet, and that lets you locally discriminate. vectors are 72 00:06:56,370 --> 00:07:03,960 stops that are associated to tracks to the PT above or below to GDP. And so those 73 00:07:03,960 --> 00:07:09,420 stubs above two gv can then be sent to the level one trigger for further processing. 74 00:07:09,900 --> 00:07:15,180 That's illustrated on this slide, where you see that the tracker is organized into 75 00:07:15,180 --> 00:07:22,980 five slices, those five slices are time multiplexed in such a way that one trigger 76 00:07:23,010 --> 00:07:29,970 box if you like, level one trigger box has visibility over an entire fi slice. And 77 00:07:29,970 --> 00:07:35,730 then there is a search, there's a seeded search. For tracks. It's illustrated in 78 00:07:35,730 --> 00:07:40,920 three little plots on the top right hand side that lets you generate level one 79 00:07:40,920 --> 00:07:47,250 trigger primitives. down on the bottom you see the efficiency versus a function of P 80 00:07:47,250 --> 00:07:54,210 t and then as a function of eater over the full range of eat up to close to 2.5 for 81 00:07:54,210 --> 00:08:02,010 nuance and it's flattened at about 100% and the electrons and goes above 80% for 82 00:08:02,010 --> 00:08:08,580 bt above 10 gV over most of the acceptance region. And you see on the bottom right 83 00:08:08,580 --> 00:08:14,820 hand side, this is now the track rate that sent to the generated by the level one 84 00:08:14,820 --> 00:08:20,550 trigger, applying the threshold, in this case, three GB and you see that the 85 00:08:21,270 --> 00:08:28,860 average number of tracks for zero pylon 23 goes up by a factor of three or so to 86 00:08:28,920 --> 00:08:36,990 somewhere between 70 and 80 and a pileup of 200. So, this is the, of course 87 00:08:36,990 --> 00:08:43,350 reflects the hard nature of the of the hard interaction compared to the soft 88 00:08:43,350 --> 00:08:48,570 nature of the violent vertices. So, this is going to be a qualitatively new 89 00:08:48,570 --> 00:08:55,200 instrument for CMS. I show here the present state of development of these PT 90 00:08:55,200 --> 00:09:00,000 module. So, on the left hand side you have a rather lovely photo of one of these 91 00:09:00,000 --> 00:09:04,620 modules you see that it comprises two sensors are split down the middle, so the 92 00:09:04,620 --> 00:09:11,910 strips are five centimeters long. On each side, our readout hybrids with eight front 93 00:09:11,910 --> 00:09:18,150 end chips or CB sees you have a zoom in on one of these rather sophisticated hybrids 94 00:09:18,150 --> 00:09:24,900 on the top right hand side. On the bottom left hand side is a cut view of this 95 00:09:24,930 --> 00:09:31,380 object that shows the flex circuit. There are bands not shown in this diagram and 96 00:09:31,410 --> 00:09:35,850 realize on top and bottom that let you bring signals from the top and bottom 97 00:09:35,850 --> 00:09:41,970 sensors to a single row of chips where they can be combined into the stocks that 98 00:09:41,970 --> 00:09:47,460 I mentioned in the previous slide. And you see that there's some compensator layers 99 00:09:47,460 --> 00:09:53,130 introduced here in yellow, which addressed one of the thorny problems we had with the 100 00:09:53,130 --> 00:09:59,130 structure which was due to bullying and deformation and during fabrication and 101 00:09:59,130 --> 00:10:05,010 also of course, Have an operated cold and you see here now we're over a large span 102 00:10:05,010 --> 00:10:12,570 of temperature that the deviations are within 10 microns from from flat. also 103 00:10:12,570 --> 00:10:18,750 shown here is the that the low voltage is brought in at 10 volts and there is then 104 00:10:18,780 --> 00:10:24,000 DC DC converter, you see the coils associated to that DC DC converter. And of 105 00:10:24,000 --> 00:10:27,420 course, this is another one of the strategies that has been adopted for this 106 00:10:27,420 --> 00:10:33,450 aggressive material budget reduction. I'm bringing in the low voltage, rather high 107 00:10:33,450 --> 00:10:37,680 voltage if you like and stepping down locally so as to reduce currents and the 108 00:10:37,680 --> 00:10:42,990 required copper cross section. Moving on now to a few slides for a new detector 109 00:10:42,990 --> 00:10:49,290 subsystem. So, the MIP timing detector, which surrounds the tracker is the barrel 110 00:10:49,290 --> 00:10:55,560 layer and the end cap layers. On the top right hand side is a table that reflects 111 00:10:55,560 --> 00:10:59,970 the impact of this in terms of physics gains. So the song 112 00:11:02,669 --> 00:11:07,559 Either increases at signal yields that are pointed out or else decreases in the 113 00:11:07,559 --> 00:11:13,079 background. On the bottom left hand side is by now I think the well known plot for 114 00:11:13,079 --> 00:11:18,449 that was a key part of the physics case for this device, introducing the so called 115 00:11:18,479 --> 00:11:23,069 4d reconstructed vertex where you reconstruct the vertex and both the Z 116 00:11:23,069 --> 00:11:28,199 shown here as well as x and y, but also in the additional dimension on the vertical 117 00:11:28,199 --> 00:11:34,649 axis of timing that lets you disentangle vertices that otherwise overlap spatially. 118 00:11:35,429 --> 00:11:39,389 On the bottom right hand corner is an example of how that can be used to 119 00:11:39,389 --> 00:11:44,039 mitigate the rate of the pilot jets in the forward region that has an immediate 120 00:11:44,039 --> 00:11:50,099 impact on the quality who pbf tagging which, for example, translates to this 30% 121 00:11:50,099 --> 00:11:57,749 improve statistical precision on the cross section for VFX to data. You can do more 122 00:11:57,749 --> 00:12:03,989 exotic things such as looking for Long live stable charged particles that's shown 123 00:12:03,989 --> 00:12:08,459 in this plot. And then you can do all sorts of opportunistic things. It turns 124 00:12:08,459 --> 00:12:14,909 out that this is a very nice particle detector Of course, it's the most precise 125 00:12:14,999 --> 00:12:20,909 time of flight detector ever realized. And this is actually a simulation of the 126 00:12:20,909 --> 00:12:26,279 particle a the performance in the context of heavy ion. So this can be used not only 127 00:12:26,279 --> 00:12:30,989 for beach physics and the standard proton program, but also as a very exciting you 128 00:12:30,989 --> 00:12:39,569 handle for heavy iron colleagues and CMS. Finally shown here is by combining the 129 00:12:39,599 --> 00:12:46,169 timing information for the upgraded, will be used in the upgraded electronics of the 130 00:12:46,169 --> 00:12:54,689 eagle barrel. You can shown in green on the left hand side plots are hypotheses 131 00:12:54,749 --> 00:12:58,979 for the vertex of the leading and subleasing photons and where they 132 00:12:58,979 --> 00:13:02,909 intersect is where presumed primary vertexes and you can see that you can 133 00:13:02,909 --> 00:13:09,269 associate these to a reduced number of primary vertices and that results in a 20% 134 00:13:09,269 --> 00:13:14,129 improvement on the statistical precision for the extra gamma gamma measurement. So 135 00:13:14,129 --> 00:13:20,039 a broad range of impacts over the full range of physics of the CMS experiment in 136 00:13:20,039 --> 00:13:25,799 the high pilot environment as well as this new feature of particle lighting. I 137 00:13:25,799 --> 00:13:29,699 mentioned previously that this thing is organized in both the barrel and end cap 138 00:13:29,699 --> 00:13:37,889 the barrel uses a way so crystals with sip and read up, whereas the end cap uses the 139 00:13:37,919 --> 00:13:44,459 new Elgato silicon sensor technology in the barrel are shown. On the top 140 00:13:44,729 --> 00:13:49,889 photograph you see the arrangement so we have bars of EL wire, so crystals arranged 141 00:13:49,889 --> 00:13:55,589 in a 16 by one array, where the bars are read out at each end. On the right hand 142 00:13:55,619 --> 00:14:01,679 corner you see a plot to blue and red of the responsive The readout that for each 143 00:14:01,679 --> 00:14:06,479 of the two ends and black, the combined response to the better than 30 picosecond 144 00:14:06,479 --> 00:14:10,829 timing response, there's a photo here of the array of weapons that's used for the 145 00:14:10,829 --> 00:14:15,599 readout and on the bottom the test being set up from which these measurements were 146 00:14:15,599 --> 00:14:24,749 extracted. So, here we move now beyond the basic detector unit towards the 147 00:14:24,749 --> 00:14:30,149 qualification of crystals from a number of commercial vendors. And we are also well 148 00:14:30,149 --> 00:14:38,159 advanced in the design of the module and for the we've gone through a thorough 149 00:14:38,159 --> 00:14:43,049 study in the prototyping on the integration aspects and single signal 150 00:14:43,049 --> 00:14:49,559 routings from Crystal to set them to basic various photographs here which illustrate 151 00:14:50,099 --> 00:14:57,449 the present state of play. In the end cap as I mentioned, Bill Gates logon avalanche 152 00:14:57,479 --> 00:15:05,549 diode sensors are used Again here we have moved to beyond the prototyping phase and 153 00:15:05,549 --> 00:15:15,059 we are now in the process of qualifying vendors and developing the tools that will 154 00:15:15,059 --> 00:15:21,929 allow us to monitor the quality of these devices during production. and here also 155 00:15:22,319 --> 00:15:26,879 looking beyond the sensor to the modules that represent the hardware till 156 00:15:26,880 --> 00:15:27,870 about five minutes. 157 00:15:29,370 --> 00:15:34,860 You see the state of play for these modules, a few slides on the CMS a Chico 158 00:15:35,610 --> 00:15:40,830 This is about 1000 square meters of instrumented surface with over 600 square 159 00:15:40,830 --> 00:15:49,320 meters and 6 million channels with silicon sensors and the 300 square meters of 160 00:15:49,320 --> 00:15:56,910 simulators. I read up with 240 organizers 240,000 scintillator files with individual 161 00:15:56,910 --> 00:16:02,220 separate read up there are some well thanks for the adoption of a 10 sensors is 162 00:16:02,220 --> 00:16:08,610 600 and some square meters can be covered with 30,000 silicon modules. On this slide 163 00:16:08,610 --> 00:16:12,990 I'll show you the upper left hand corner schematic of the silicon module stack up, 164 00:16:13,560 --> 00:16:19,410 which is a silicon sensor sandwiched between the base plate and the PCB. And 165 00:16:19,410 --> 00:16:24,810 Shown here are various photos of the automated versus automated assembly steps 166 00:16:24,870 --> 00:16:31,170 of these modules. The bottom right hand side, the finished product. A similar 167 00:16:31,170 --> 00:16:36,930 slide for the CIP Amman tile and module development. So you see individual tiles 168 00:16:36,930 --> 00:16:43,470 and symptoms. You see them then grouped together onto the tile module. And on the 169 00:16:43,470 --> 00:16:49,500 backside of that tire module is an electronic sport that houses various 170 00:16:49,530 --> 00:16:56,430 support in the tronics as well as the readout basics and the dc dc convertors. 171 00:16:57,840 --> 00:17:05,520 Both the silicon and The Superman tile use substantially the same front end chip hc 172 00:17:05,520 --> 00:17:13,470 rock with a slightly modified front end. One of the defining features of this chip 173 00:17:14,190 --> 00:17:19,500 is the architecture which allows us to achieve an effective 16 bit dynamic range 174 00:17:19,980 --> 00:17:25,440 by combining an ADC over the range where the front end amplifier remains linear, 175 00:17:25,800 --> 00:17:30,780 and the time of a threshold measure the length of time during which preamplifier 176 00:17:30,780 --> 00:17:36,030 is actually in saturation. And the chip features then a third ADC which provides 177 00:17:36,030 --> 00:17:42,960 the time of arrival signal with a resolution of 25 picoseconds. The Sheikah 178 00:17:42,960 --> 00:17:49,710 will feature in Purcell high resolution tiny measurement, which remember correctly 179 00:17:49,710 --> 00:17:56,160 I have a slide later on to illustrate is a slide that looks at the architecture the 180 00:17:56,160 --> 00:18:00,330 electronics architecture so not only are the rocks substantially common to The 181 00:18:00,330 --> 00:18:06,150 silicon and scintillator sections, but so is the architecture signals from a number 182 00:18:06,150 --> 00:18:11,550 of rocks are collected through. So called concentrated trips there is a concentrated 183 00:18:11,550 --> 00:18:17,040 trip the trigger path, separate concentrated trip for the data path. The 184 00:18:17,040 --> 00:18:23,070 signals are bused from modules to the concentrator trips over so called wagon 185 00:18:23,340 --> 00:18:32,250 motherboards. And then the two minutes, two minutes and there are so called 186 00:18:32,250 --> 00:18:37,650 engines that provide the interface to the LPG VTX shown here on the bottom left hand 187 00:18:37,650 --> 00:18:42,780 side is something that gives you an idea of how tightly packed hold these are, in 188 00:18:42,780 --> 00:18:46,380 order to maintain the compactness of the email section of the calorimeter where we 189 00:18:46,380 --> 00:18:53,400 allow for a gap of all this electronics of about five millimeters. This is a similar 190 00:18:53,400 --> 00:18:58,590 diagram for so called mixed cassettes we have silicon modules on the inside and 191 00:18:58,590 --> 00:19:04,080 central later on the outside. This is a slider was alluding to previously, which 192 00:19:04,080 --> 00:19:10,110 shows the time in response to the photons, it's worth 20 picoseconds. But it shows 193 00:19:10,110 --> 00:19:15,990 that you also get a border 20 picosecond. The response approaching 20 picoseconds to 194 00:19:15,990 --> 00:19:20,550 neutral had rods and the bottom two plots to show what happens when you turn the 195 00:19:20,550 --> 00:19:25,860 knob and reject the pilot within a single bunch crossing with the timing code of 90 196 00:19:25,860 --> 00:19:31,470 picoseconds for a Higgs the gamma gamma event in a pileup of 200 and the resulting 197 00:19:31,470 --> 00:19:37,200 cleanup this is just to say that the data from this calorimeter generates a great 198 00:19:37,200 --> 00:19:42,960 deal of excitement and exercising novel reconstruction techniques, in particular 199 00:19:42,990 --> 00:19:46,560 machine learning and various types of graph networks. 200 00:19:48,150 --> 00:19:49,830 Coming out to the immune system. 201 00:19:51,570 --> 00:19:55,920 There are a number of new chambers that have been added to the neon system g one 202 00:19:55,920 --> 00:19:59,970 one whose goal is to improve the trigger performance at level one that says 203 00:20:00,000 --> 00:20:04,500 straighted in the plots on the right hand side, or you have an improved efficiency 204 00:20:04,500 --> 00:20:10,380 with a reduction of order over an order of magnitude and the trigger rate. This is 205 00:20:10,380 --> 00:20:16,050 actually the first of our phase two upgrades. So the minus side view on one 206 00:20:16,050 --> 00:20:22,020 disk has been was installed before the end of last year. On the bottom you see a 207 00:20:22,020 --> 00:20:25,980 photograph from that installation and on the bottom right hand side you see a photo 208 00:20:25,980 --> 00:20:31,680 of the chambers for the second disc and test track awaiting installation has coded 209 00:20:31,680 --> 00:20:32,430 well allow 210 00:20:33,900 --> 00:20:37,020 we're down to zero minutes Can you come to wrap up 211 00:20:37,380 --> 00:20:43,230 slides now I'm about to wrap up. We also will extend the neon coverage in order to 212 00:20:43,290 --> 00:20:49,290 prove acceptance with the zero chambers and take advantage of the denser and more 213 00:20:49,290 --> 00:20:55,470 compacted Sheikha which allows for a slot behind it. And also leveraging the fact 214 00:20:55,470 --> 00:21:00,000 that the tracker acceptance of course extends now beyond data three and finally 215 00:21:00,840 --> 00:21:05,100 We will both add new rpcs and upgrade electronics to make full use of the 216 00:21:05,100 --> 00:21:09,360 intrinsic timing capability of the rpcs. And among other things that will improve 217 00:21:09,360 --> 00:21:14,190 our well that will provide a trigger for heavy stable charged particles as shown 218 00:21:14,190 --> 00:21:21,600 here on the right. Just a word about the extremely ambitious set of ethics that are 219 00:21:21,600 --> 00:21:26,220 required to support these upgrades. That's, I think, a defining theme in our 220 00:21:26,220 --> 00:21:31,470 field the importance of these electronics and the continued access to expertise and 221 00:21:31,470 --> 00:21:36,510 foundries. I think I'll skip the slide on the overall schedule unless there are 222 00:21:36,510 --> 00:21:41,340 questions about it and I come to the conclusions. So responding to the 223 00:21:41,340 --> 00:21:46,980 challenges of the nature illiteracy environment. The CMS upgrade program 224 00:21:46,980 --> 00:21:52,050 introduces new paradigms in the form of PT modules for level one trigger tracking 225 00:21:52,080 --> 00:21:56,550 ishika precision timing for pilot mitigation. It breaks new ground and the 226 00:21:56,550 --> 00:22:00,810 type of technology for example, with a low very large scale the deployment of eighth 227 00:22:00,810 --> 00:22:06,570 inch. So the consensus radiation heart systems, elk, cats gems, as well as 228 00:22:06,780 --> 00:22:12,840 computing. Well this is underpinned that I mentioned by a broad program of a six 229 00:22:12,840 --> 00:22:17,340 development, which are both for common applications. In fact, not only within CMS 230 00:22:17,340 --> 00:22:23,700 but also for Atlas, as well as the tech the specific designs. It's an ambitious 231 00:22:23,700 --> 00:22:30,450 program, we make good progress, but many challenges still lie ahead. we're 232 00:22:30,450 --> 00:22:35,610 advancing through TDRS towards production. There is an additional year now which is 233 00:22:35,610 --> 00:22:39,630 allowed by the November 17 certain schedule and provides the both the 234 00:22:39,630 --> 00:22:43,650 opportunity to get more time as necessary to mitigate technical risks, make sure 235 00:22:43,650 --> 00:22:48,360 that everything that goes ahead is actually technically sound while also 236 00:22:48,360 --> 00:22:53,640 restoring a 12 month master for contingency and that together Of course, 237 00:22:53,640 --> 00:22:58,230 with the commitment and support of CERN, but in particular, also the collaborative 238 00:22:58,230 --> 00:23:02,280 funding agencies and Institute's provides a healthy footing for the successful 239 00:23:02,280 --> 00:23:05,460 completion of this upgrade and physics programs. That's it. 240 00:23:06,509 --> 00:23:11,729 Thank you very much, Marcelo. That was really fascinating talk. And there's a 241 00:23:11,729 --> 00:23:18,389 moment now for questions, please raise your hand using the feature. Yes. So v 242 00:23:18,389 --> 00:23:21,809 tech, please state your name and institutes and go ahead. 243 00:23:24,450 --> 00:23:32,460 Returns because I'm at ski Sara cyclic on page 19. Your egg God for the end cap 244 00:23:32,490 --> 00:23:38,010 timing detector on the surface would very much like the Atlas ganz if only because 245 00:23:38,010 --> 00:23:44,610 you say it's going to be a joint order. Now why is it that they will tolerate the 246 00:23:44,610 --> 00:23:53,250 radiation for the entire lifetime of the HL hc while Atlas plans to replace the 247 00:23:53,280 --> 00:23:58,290 innermost parts of the foreword this at least once if not prize during the 248 00:23:58,290 --> 00:23:59,550 attributed lifetime? 249 00:24:02,220 --> 00:24:10,710 Yes, I think so there's a great deal of synergy in this in this development 250 00:24:10,740 --> 00:24:15,510 between the two collaborations. I think that's been very positive on both sides. I 251 00:24:15,510 --> 00:24:20,310 believe the rapidity coverage of the Atlas timing detector is different from that to 252 00:24:20,310 --> 00:24:25,110 the CMS detector. And I believe that therefore, you integrate more fluids for a 253 00:24:25,110 --> 00:24:26,160 given luminosity. 254 00:24:28,200 --> 00:24:32,370 At any rate, you see here measurements that show that the 255 00:24:35,580 --> 00:24:40,650 so there's a plot in the center plot on the bottom rows, rather nice plot which 256 00:24:40,650 --> 00:24:47,310 shows that if you look at the timing resolution in terms of of gain, 257 00:24:48,630 --> 00:24:51,900 that you see most points of fall on on a given 258 00:24:55,260 --> 00:25:01,560 line, there is some hint of degradation of that with with radiation. But main trend 259 00:25:02,010 --> 00:25:06,840 is that as long as you can Is that really the timing of the solution as determined 260 00:25:06,840 --> 00:25:10,620 by the game, which is essentially the amplitude of the signal that's generated. 261 00:25:11,490 --> 00:25:17,610 Now what happens is, if you look very carefully at the symbols is that if you 262 00:25:17,610 --> 00:25:23,310 look at the little red crosses, so those are in the red boxes, those are four 310 263 00:25:23,310 --> 00:25:28,560 to the 15 610 to the 15 neutrons per square centimeter. And you see that at 264 00:25:28,560 --> 00:25:33,930 these high influences, you're no longer able to achieve the highest gains, you see 265 00:25:33,930 --> 00:25:39,570 actually gain versus bias voltage. On the left hand side what happens as we approach 266 00:25:39,570 --> 00:25:46,140 for answers of five or 610 to the 15, which is what we expect over the lifetime 267 00:25:46,140 --> 00:25:54,270 of the device is the achievable gain decreases, the resolution degrades. So we 268 00:25:54,270 --> 00:25:59,070 will start with 30 picoseconds, we will end up with something like 60 and we will 269 00:25:59,070 --> 00:26:02,970 average about 40 45 Pico seconds over the lifetime of the device. 270 00:26:05,130 --> 00:26:10,830 Okay, we have time for one quick question from Andreas flicker. 271 00:26:12,330 --> 00:26:13,980 Please again identify yourself. 272 00:26:15,900 --> 00:26:16,860 Go ahead, Andreas. 273 00:26:21,000 --> 00:26:25,500 Okay, so yes. So I got my son Jessica from son I, my child, this was a beautiful 274 00:26:25,500 --> 00:26:30,000 Talk. Thank you very much. Very quick question. Actually two quick ones. I was 275 00:26:30,030 --> 00:26:36,150 Can you remind me the impact parameter resolution you have 400 for the level one 276 00:26:36,150 --> 00:26:41,160 tracks, basically TGV tracks, the ones who reconstruct, and then I had one more 277 00:26:41,160 --> 00:26:46,710 question, which is on page 14, where you show the beautiful dy dx plot, so tight 278 00:26:46,710 --> 00:26:51,870 timing dependent plot, but you show it for eta larger than 1.6 is the performance 279 00:26:51,870 --> 00:26:55,050 similar for central tracks. Thank you very much. 280 00:27:00,690 --> 00:27:05,130 So yes, that's shown for the end cap. 281 00:27:07,259 --> 00:27:12,359 There's no reason why the performance will be different for central tracks. Okay. 282 00:27:13,109 --> 00:27:14,759 Now coming to your 283 00:27:16,800 --> 00:27:19,140 actually, Can you remind me what your first question was? 284 00:27:19,740 --> 00:27:21,900 This was the impact parameter is dilution. 285 00:27:23,040 --> 00:27:28,200 Yes, I don't remember that off the top of my mind. But the impact parameter itself, 286 00:27:28,260 --> 00:27:31,650 the inner pixel layers don't form part of level one trigger. 287 00:27:33,390 --> 00:27:35,520 If we go to two 288 00:27:36,840 --> 00:27:38,730 main effects that zero actually 289 00:27:38,850 --> 00:27:45,510 exactly so So, if you see the the inner three blue layers 290 00:27:47,040 --> 00:27:51,900 there the sensors the PT modules are comprised of one layer which is a strip 291 00:27:51,900 --> 00:27:58,590 sensor, and a second layer, which is pixelated with the pixel lines if you like 292 00:27:58,590 --> 00:28:07,530 of the leaflets 1.3 millimeters finally. And so, you have a lever arm of the 293 00:28:07,560 --> 00:28:14,310 between the first and the third such layer which is longer than comparable to the 294 00:28:14,310 --> 00:28:18,840 distance from the first layer to the to the vertex. And so from that you could 295 00:28:18,840 --> 00:28:21,690 conclude that you will have zero resolution of order a couple of 296 00:28:21,690 --> 00:28:25,140 millimeters, but I don't remember the exact number off the top of my head, but 297 00:28:25,170 --> 00:28:26,220 that's about the scale. 298 00:28:27,600 --> 00:28:28,200 Thank you. 299 00:28:29,100 --> 00:28:34,440 Okay, thank you very much, Marcelo. And if people have questions, they can contact 300 00:28:34,440 --> 00:28:40,380 you offline. Now, we would like to go on to the concluding talk today by Mark 301 00:28:40,380 --> 00:28:49,320 Tobin. So if we can stop sharing from Marcelo and Mark when you're ready, if you 302 00:28:49,320 --> 00:28:50,220 can start sharing