WEBVTT 1 00:00:04.481 --> 00:00:10.150 WH11NE- Sunrise: Good afternoon. Thanks a lot for coming for the what's called. 2 00:00:10.370 --> 00:00:14.460 WH11NE- Sunrise: I'll present the next results for the 3 00:00:14.840 --> 00:00:17.699 WH11NE- Sunrise: for the lovely particle Search immism case. 4 00:00:17.810 --> 00:00:20.649 WH11NE- Sunrise: you'll see Ms beyond vector showers. 5 00:00:21.060 --> 00:00:22.070 WH11NE- Sunrise: And 6 00:00:22.260 --> 00:00:33.950 WH11NE- Sunrise: I'm from initial science laboratory in Armenia. I'm a 5th year. Phd student. And I've been to for about 2 years. 7 00:00:34.550 --> 00:00:41.960 WH11NE- Sunrise: I've been involved in some of the. These are some of my activities that I've been involved in formula. 8 00:00:42.110 --> 00:00:45.810 WH11NE- Sunrise: So the physical analysis itself, the 9 00:00:45.920 --> 00:00:53.740 WH11NE- Sunrise: have been working on the development of system test for the Cms. And timing pair modules 10 00:00:54.160 --> 00:01:10.599 WH11NE- Sunrise: for this, for the for testing them, and having involved in testing of pixel and strip Acl sensors at the testing facility and and then contributed in the design and performance of the screen racing 11 00:01:11.130 --> 00:01:14.590 WH11NE- Sunrise: of so and currently, I'm working on the 12 00:01:14.730 --> 00:01:20.340 WH11NE- Sunrise: development of a testing set up for the modules with cost improvitation. 13 00:01:23.380 --> 00:01:28.010 WH11NE- Sunrise: So yeah, we'll start with the production test. 14 00:01:28.150 --> 00:01:32.570 WH11NE- Sunrise: You know, that standard model has a short codes, some of them. 15 00:01:32.860 --> 00:01:42.719 WH11NE- Sunrise: Some of the phenomena cannot be explained. With this other model, for example, the Guy hierarchy problem, the existence of the dark matter, the very in a symmetry and the 16 00:01:42.860 --> 00:01:51.230 WH11NE- Sunrise: interacting, the universe. The origin of the neutrino messes the universe expansion with acceleration. So 17 00:01:51.460 --> 00:01:58.239 WH11NE- Sunrise: the gravity, gravity signature itself. So there are some pictures here. 18 00:01:58.480 --> 00:01:59.840 WH11NE- Sunrise: Also. 19 00:02:00.330 --> 00:02:01.580 WH11NE- Sunrise: There's like 20 00:02:02.180 --> 00:02:14.039 WH11NE- Sunrise: the 1st page I'm showing. The bullet cluster. Galaxy cluster. It consists of. This is this observation consists of. 21 00:02:14.260 --> 00:02:14.960 WH11NE- Sunrise: So 22 00:02:15.180 --> 00:02:21.660 WH11NE- Sunrise: the there are 2 parts of the image, the the blue regions which correspond to the locations of the 23 00:02:21.960 --> 00:02:23.460 WH11NE- Sunrise: the 2 Busters. 24 00:02:23.600 --> 00:02:37.599 WH11NE- Sunrise: and the the pink region is the X-ray X-ray. The observation of the X-ray radiation in this region which shows that these 2 galaxy clusters have collided. 25 00:02:37.760 --> 00:02:44.979 WH11NE- Sunrise: How do we know that? Because well, 1st of all, by the shape of the of the second 26 00:02:45.120 --> 00:02:47.350 WH11NE- Sunrise: of the second part of the 27 00:02:51.250 --> 00:02:59.909 WH11NE- Sunrise: that's the second region. So which means that this this galaxy has been deploying through with the higher speed, and 28 00:03:00.060 --> 00:03:09.249 WH11NE- Sunrise: by seeing that by observing the the lens effect, the cosmic lens effect, we can say that 29 00:03:09.992 --> 00:03:17.227 WH11NE- Sunrise: the masses are still concentrated in this in these regions, even after the collision. And 30 00:03:17.970 --> 00:03:26.780 WH11NE- Sunrise: I think the radiating matter is the gases which have stolen down after the collision, which 31 00:03:26.990 --> 00:03:38.280 WH11NE- Sunrise: yes, and as a result, we can see the radiation from here. But these parts of the matter they didn't interact. If they didn't slow down. They moved faster than the gas, so 32 00:03:38.500 --> 00:03:44.350 WH11NE- Sunrise: a new type of matter has been introduced, called called Dark Matter. 33 00:03:44.630 --> 00:03:48.381 WH11NE- Sunrise: Oh, and for the various symmetry 34 00:03:49.200 --> 00:03:58.849 WH11NE- Sunrise: So that's the question. Why is the universe consists of only matter, one of the one of the indirect 35 00:03:59.560 --> 00:04:03.749 WH11NE- Sunrise: indirect? Let's say confirmation, that. 36 00:04:04.350 --> 00:04:20.779 WH11NE- Sunrise: or just a observation of that phenomenon can be the the microwave map of the universe. Simply, it's showing the temperature in different locations. 37 00:04:22.280 --> 00:04:43.540 WH11NE- Sunrise: the universe. It's of the universe. If the Z axis is the temperatures. So since there are dark areas, which means that since since the map is not uniform, it means that there wasn't a known uniformity initially in the early universe of matter in that matter. So once it expanded, the dark 38 00:04:43.650 --> 00:04:51.380 WH11NE- Sunrise: regions also the less dense in matter. Regions have also expand, and the 39 00:04:51.540 --> 00:04:58.719 WH11NE- Sunrise: yes, and the map of the app universe is evolution. 40 00:04:58.910 --> 00:05:04.240 WH11NE- Sunrise: Yes, the universe is expanding, expanding with an acceleration. 41 00:05:04.420 --> 00:05:10.369 WH11NE- Sunrise: And well, to to explain that the dark energy concept testing. 42 00:05:11.700 --> 00:05:12.520 WH11NE- Sunrise: Let's see. 43 00:05:13.400 --> 00:05:14.500 WH11NE- Sunrise: So 44 00:05:15.300 --> 00:05:25.039 WH11NE- Sunrise: some of the some of the phenomenon that cannot be explained with with the standard model theories or beyond standard model theories are introduced. 45 00:05:25.866 --> 00:05:26.473 WH11NE- Sunrise: They 46 00:05:27.450 --> 00:05:38.890 WH11NE- Sunrise: So they sent the standard model with new predicted particles and and the searches for hey? 47 00:05:39.110 --> 00:05:45.150 WH11NE- Sunrise: The the search for Bsn particles is mostly inspired by the standard model 48 00:05:46.071 --> 00:05:53.500 WH11NE- Sunrise: problems. So the detectors that are built today the modern detectors are stuff. 49 00:05:54.270 --> 00:06:00.449 WH11NE- Sunrise: They expect the particles to be prompt. So so they so the 50 00:06:01.700 --> 00:06:07.599 WH11NE- Sunrise: so. So this this expectation has been has been the cause of development 51 00:06:07.760 --> 00:06:11.159 WH11NE- Sunrise: of the nowadays. Design of the detectors. 52 00:06:11.270 --> 00:06:12.180 WH11NE- Sunrise: Oh. 53 00:06:12.470 --> 00:06:24.660 WH11NE- Sunrise: yes, but but there are cases in the Bsm. In the models that the particles can have significantly larger decay time. 54 00:06:24.890 --> 00:06:27.409 WH11NE- Sunrise: vk, distance. 55 00:06:28.370 --> 00:06:31.681 WH11NE- Sunrise: And that's when the log net particles come in. 56 00:06:32.380 --> 00:06:48.169 WH11NE- Sunrise: so the requirements for the particle to be long lived. This is the decay. This is the lifetime of the particle. It depends on 2 major components is the matrix element and the phase space of the decay. 57 00:06:48.540 --> 00:07:02.770 WH11NE- Sunrise: So it either either to be to be for the particle to be long lived either the map matrix element should be small, small or or and the space space for SDK should be 58 00:07:03.554 --> 00:07:05.519 WH11NE- Sunrise: should be limited. 59 00:07:05.890 --> 00:07:15.659 WH11NE- Sunrise: So in many theoretical model there are many theoretical models. These are some examples of those that predict the existence of the Ops. 60 00:07:15.840 --> 00:07:29.069 WH11NE- Sunrise: the Suzy model, the seesaw model that predicts the steril-steromes and the hex portal model which will be discussed in this. In this talk, hidden values 61 00:07:29.190 --> 00:07:39.620 WH11NE- Sunrise: and for the detection they challenge the ordinary methods of detecting particles and some new detection techniques and 62 00:07:40.660 --> 00:07:43.129 WH11NE- Sunrise: Tree bank methods should be developed. 63 00:07:44.880 --> 00:07:56.990 WH11NE- Sunrise: So, oh, so to to detect. We expect a different signature from them than from standard model particles. 64 00:07:57.180 --> 00:08:02.470 WH11NE- Sunrise: We expect an anomalous organization which is 65 00:08:02.810 --> 00:08:13.000 WH11NE- Sunrise: different different amount of ionization that can be predicted from the box equation. We expect the the waves vector signals. 66 00:08:13.806 --> 00:08:24.520 WH11NE- Sunrise: and so- so after. So since then we can separate the searches into 2 categories 67 00:08:24.630 --> 00:08:29.580 WH11NE- Sunrise: into direct detection. And for charge Llps and Neutral Llps. 68 00:08:29.760 --> 00:08:39.260 WH11NE- Sunrise: In case of charge we can observe. Observe tracks. If we discuss the design of Cms. We can. 69 00:08:39.950 --> 00:08:48.200 WH11NE- Sunrise: We'll we'll observe some some disappearing tracks or anomous trajectory tracks. 70 00:08:48.390 --> 00:09:00.110 WH11NE- Sunrise: What is it? Disappearing track is the if the indicates somewhere in the tracker system, it's at least a track behind it behind it, and at some point 71 00:09:00.210 --> 00:09:03.799 WH11NE- Sunrise: the the track just interrupts. 72 00:09:04.130 --> 00:09:06.110 WH11NE- Sunrise: If a. 73 00:09:06.210 --> 00:09:15.699 WH11NE- Sunrise: the other cases, the displaced track, when when it the case before the tracking system, and we can see all the 74 00:09:15.810 --> 00:09:19.260 WH11NE- Sunrise: the track of the reference. 75 00:09:19.620 --> 00:09:20.500 WH11NE- Sunrise: Oh. 76 00:09:20.810 --> 00:09:28.039 WH11NE- Sunrise: in case of any direct detection with the neutral piece of the case for this for this talk. 77 00:09:28.220 --> 00:09:34.650 WH11NE- Sunrise: Oh, we expect a decay, displace, decay, vertex. 78 00:09:35.110 --> 00:09:41.350 WH11NE- Sunrise: It's placed somewhere because calorimeters or the internal system phone. 79 00:09:42.650 --> 00:09:47.180 WH11NE- Sunrise: So into more in detail of 80 00:09:47.970 --> 00:09:51.020 WH11NE- Sunrise: discuss the case with the, you know system. 81 00:09:51.280 --> 00:09:52.270 WH11NE- Sunrise: So 82 00:09:52.620 --> 00:10:00.341 WH11NE- Sunrise: why do we perform searches and immune systems? Because it has a high coverage and high coverage? 83 00:10:01.760 --> 00:10:05.390 WH11NE- Sunrise: well, it's it's it's completely covering the 84 00:10:05.870 --> 00:10:15.789 WH11NE- Sunrise: Cms. It has a far. It is far from the interaction point, so we can cover a large decay decay distances. 85 00:10:15.920 --> 00:10:28.549 WH11NE- Sunrise: It's excellent for background suppression, because it has steel layers, and this steel and detector layered structure can be used as a sampling. 86 00:10:29.280 --> 00:10:39.750 WH11NE- Sunrise: And this is the this images from a simulation. We have to play with example of a pair of an and beyond. 87 00:10:40.110 --> 00:10:49.190 WH11NE- Sunrise: we can obviously see that these yellow dots are. It's in the so gas chambers. 88 00:10:49.600 --> 00:10:52.840 WH11NE- Sunrise: cattle, strip chambers. And we can. 89 00:10:53.130 --> 00:11:09.670 WH11NE- Sunrise: We can see that the signature of the differs a lot, and I will explain how the Llps became, and how does how does it produce showers? And therefore it produces more hits than the muon. 90 00:11:09.930 --> 00:11:16.260 WH11NE- Sunrise: Also it's more compact because passes through and leaves very few hits. 91 00:11:19.790 --> 00:11:27.410 WH11NE- Sunrise: So the- the analysis that I will show is using the- the following mechanism to 92 00:11:27.520 --> 00:11:31.710 WH11NE- Sunrise: to detect their own piece, oh, Whoa! 93 00:11:32.730 --> 00:11:40.869 WH11NE- Sunrise: Once- once the produce, the showers. We use a scan. 94 00:11:41.090 --> 00:11:46.410 WH11NE- Sunrise: an algorithm called dB scan to reconstruct those heads into clusters. 95 00:11:46.740 --> 00:11:59.420 WH11NE- Sunrise: Oh, there's something. There's a diagram that shows 2 parameters distance parameter, from the, from the from the 96 00:11:59.520 --> 00:12:16.159 WH11NE- Sunrise: perfect, for the, for the, from the mean of the closer from being distance from the closer and the the end of this, the mean, the main position, and the distance from the from the other from the other end. So it's 97 00:12:16.380 --> 00:12:21.950 WH11NE- Sunrise: continuously looking over tickets and collecting them into a cluster. 98 00:12:22.410 --> 00:12:23.055 WH11NE- Sunrise: And 99 00:12:23.840 --> 00:12:37.569 WH11NE- Sunrise: yes, as we've seen, the do not create. And eventually the number of hits is one of the important parameters that we'll use. It's not going for the mules is going to be 100 00:12:37.690 --> 00:12:42.289 WH11NE- Sunrise: there, there will be much less. It's neglected. Cluster. 101 00:12:44.340 --> 00:12:50.750 WH11NE- Sunrise: So this is the 1st analysis that has been done in the 102 00:12:51.300 --> 00:12:54.050 WH11NE- Sunrise: just, an search in their own chambers 103 00:12:54.320 --> 00:13:03.199 WH11NE- Sunrise: in. Yes, this is the. This is the signal process that has been discussed. So 104 00:13:03.810 --> 00:13:14.469 WH11NE- Sunrise: that became still happens in the system, and because because it's happening in the immune system, and 105 00:13:14.720 --> 00:13:19.800 WH11NE- Sunrise: the energies are high because of the because it's produced by 106 00:13:19.930 --> 00:13:26.300 WH11NE- Sunrise: 5 decay on the Higgs also the Lp. Is a scalar-scalar. So 107 00:13:26.830 --> 00:13:31.649 WH11NE- Sunrise: so, therefore, since it passes the colorimeters, it produces a high net. 108 00:13:31.790 --> 00:13:52.790 WH11NE- Sunrise: and in the selections you know, find selections we use. Pt. Greater than 200 Gb. Of missing. We require at least one at least one chat of greater than 50 gb. Pt. And we require at least 109 00:13:52.900 --> 00:14:03.589 WH11NE- Sunrise: least one cluster, or one or 2 clusters passing the top cluster. Id cluster id is a set of requirements for the cluster. 110 00:14:04.823 --> 00:14:12.180 WH11NE- Sunrise: and so, after. So, after these selections and estimation limit of the limit. 111 00:14:12.480 --> 00:14:24.669 WH11NE- Sunrise: these are some of the these are the curves of the estimated limit. Different curves correspond to different masses. For the there are 3 Gb. 7, 1514, 112 00:14:24.770 --> 00:14:31.339 WH11NE- Sunrise: 65, and the most stringent limit that could be applied. In this case. 113 00:14:32.120 --> 00:14:37.270 WH11NE- Sunrise: it can be estimated is at one meter of a Dk length. 114 00:14:41.190 --> 00:14:41.940 WH11NE- Sunrise: So 115 00:14:44.090 --> 00:14:55.450 WH11NE- Sunrise: yeah. So the Higgs portal model is the one that we have that we're discussing, because it's a, it's a minimum extension model. It extends to center model by a single scalar. 116 00:14:56.125 --> 00:14:57.820 WH11NE- Sunrise: Which is so. 117 00:14:58.100 --> 00:15:10.730 WH11NE- Sunrise: Yes, noted by this. So the-, the-, the extension of the standard model consists of 2 parts, and the the first-, the 1st part is the one that we just we'll discuss 118 00:15:10.940 --> 00:15:16.557 WH11NE- Sunrise: on this talk, and the second one is the one, the one that we have just looked at. 119 00:15:17.010 --> 00:15:24.870 WH11NE- Sunrise: and yes, and the yes, the second scenario, I mean the second scenario will trigger it with Matt. And it's a 120 00:15:25.420 --> 00:15:32.139 WH11NE- Sunrise: it has been excluded. It's the selections developed for it. Very sensitive. 121 00:15:32.570 --> 00:15:37.380 WH11NE- Sunrise: Yes, and the the 1st case that we will discuss. 122 00:15:37.620 --> 00:15:44.669 WH11NE- Sunrise: we observed, observe a direct OP. The production of the OP. 123 00:15:44.810 --> 00:15:49.430 WH11NE- Sunrise: From the from decay of the V Renaissance. 124 00:15:49.790 --> 00:15:58.139 WH11NE- Sunrise: So so the into a We cloud that's decay to a mess and 125 00:16:02.470 --> 00:16:03.390 WH11NE- Sunrise: 36. 126 00:16:05.580 --> 00:16:10.517 WH11NE- Sunrise: So since so- so since we 127 00:16:12.230 --> 00:16:20.090 WH11NE- Sunrise: there is the, there is a requirement on the mess of the OP, since it's going to be smaller than the venison mass. 128 00:16:20.190 --> 00:16:24.900 WH11NE- Sunrise: the 1st diagram will be dominant in the fixed portal. 129 00:16:25.200 --> 00:16:29.146 WH11NE- Sunrise: So we are using the yeah sounds. 130 00:16:29.750 --> 00:16:34.840 WH11NE- Sunrise: And and we're using the be parking data set to overcome the limitations from 5 min. 131 00:16:35.170 --> 00:16:44.831 WH11NE- Sunrise: because well, I didn't include the kinematics of the. But for the for the for this case, the 132 00:16:45.650 --> 00:16:51.250 WH11NE- Sunrise: very soft, that's very little peaky and 133 00:16:52.580 --> 00:16:58.320 WH11NE- Sunrise: yes, and this is the single signal process that we're discussing. 134 00:16:58.730 --> 00:17:03.700 WH11NE- Sunrise: So the way that we trigger. This process is with the with the neon. 135 00:17:03.810 --> 00:17:14.749 WH11NE- Sunrise: As I said, we have 2. 1 of them decays into an the other, one decays into a decays into a new one, and 136 00:17:15.349 --> 00:17:17.160 WH11NE- Sunrise: then we all just use the 137 00:17:17.510 --> 00:17:23.489 WH11NE- Sunrise: to trigger the events that will selections for the new ones you want to 138 00:17:25.609 --> 00:17:27.632 WH11NE- Sunrise: for the view parking data sets. 139 00:17:28.450 --> 00:17:37.659 WH11NE- Sunrise: so- so the- the data set was collected in 2018 with 14 1.6 140 00:17:37.870 --> 00:17:45.530 WH11NE- Sunrise: in our city. It consists of 10 billion events. It each of them has 141 00:17:46.270 --> 00:17:48.709 WH11NE- Sunrise: as a decay of 2 in essence. 142 00:17:49.010 --> 00:17:59.879 WH11NE- Sunrise: And so during the data acquisition, the drop in the the drop in the luminosity has been considered. 143 00:18:00.000 --> 00:18:12.640 WH11NE- Sunrise: and in 2017 we can see that was dropping. So in 2018, periodically, to maintain the same 144 00:18:12.970 --> 00:18:18.870 WH11NE- Sunrise: data rate. New Hlt triggers we're adding 145 00:18:19.250 --> 00:18:26.160 WH11NE- Sunrise: were being added in order to in order to maintain the same event, collection number of events. 146 00:18:27.345 --> 00:18:28.895 WH11NE- Sunrise: So eventually, 147 00:18:29.780 --> 00:18:37.090 WH11NE- Sunrise: eventually, by the end of the collect data acquisition, about 70 to 80% security. It's been 148 00:18:37.220 --> 00:18:40.969 WH11NE- Sunrise: has been achieved for preparing data set. 149 00:18:43.770 --> 00:18:48.779 WH11NE- Sunrise: Also, we apply trigger scale factors for the events 150 00:18:48.920 --> 00:19:02.530 WH11NE- Sunrise: which has been collecting, which has been calculated using the simulated events of J side to process with the parking data set. 151 00:19:03.030 --> 00:19:21.006 WH11NE- Sunrise: So in order to calculate it. The mass mass has been reconstructed of the J side process. The same was done for the parking data set. The peaks have been calculated, reconstructed for different. 152 00:19:21.690 --> 00:19:25.439 WH11NE- Sunrise: Oh, so the new ones already constructed with the tag and probe method 153 00:19:25.610 --> 00:19:37.000 WH11NE- Sunrise: and the probe method probe probe muon has been used to select different regions of the Muon Pt and the displacement significance 154 00:19:37.150 --> 00:19:39.799 WH11NE- Sunrise: in different regions. 155 00:19:40.420 --> 00:19:48.100 WH11NE- Sunrise: The the mass peak has been constructed and fitted with the Gaussian plus cherish 1st order, phase, function. 156 00:19:48.670 --> 00:19:54.992 WH11NE- Sunrise: oh, and and yes, and the the integral of the 157 00:19:56.660 --> 00:20:02.290 WH11NE- Sunrise: of the differences calculated as a as a as the yield. 158 00:20:02.440 --> 00:20:06.799 WH11NE- Sunrise: And and then the efficiency has been calculated for the. 159 00:20:07.010 --> 00:20:15.590 WH11NE- Sunrise: for the events where the probe, you know, is passing the parking agility triggers for not the following data. 160 00:20:15.750 --> 00:20:24.490 WH11NE- Sunrise: and the ratio is take of signal over background is taken as a trigger, as a trigger scale factor. 161 00:20:24.920 --> 00:20:25.690 WH11NE- Sunrise: Oh. 162 00:20:30.480 --> 00:20:39.010 WH11NE- Sunrise: so in the process that I've described, we discuss the decay of the of the OP. Into 2 ions. 163 00:20:39.140 --> 00:20:48.290 WH11NE- Sunrise: either positive, either positive or neutral or positive, to oppositely charged or to neutral items. 164 00:20:48.620 --> 00:20:58.386 WH11NE- Sunrise: Yeah, so, and once we construct the clusters, and we require them to match their own piece. Gen, level. 165 00:20:59.720 --> 00:21:08.630 WH11NE- Sunrise: Yeah, so and we calculate the efficiency for those for those cases, for for the for different decay positions. 166 00:21:08.790 --> 00:21:19.250 WH11NE- Sunrise: And yes, we can see that we observe about 50 to 60% efficiency in the in the reconstruction of the of these clusters. 167 00:21:21.730 --> 00:21:27.040 WH11NE- Sunrise: Yes, and yes, the upper row is for 5 0 5 0, and for the 168 00:21:34.280 --> 00:21:40.489 WH11NE- Sunrise: so this is a so now I'll describe the analysis strategy that we've implemented we. 169 00:21:41.400 --> 00:21:50.979 WH11NE- Sunrise: So these are the requirements for triggering on. We require to be on to greater than sub G energy. Less than 1.5. 170 00:21:51.190 --> 00:21:56.259 WH11NE- Sunrise: We're required to buy one of the departing Hlt triggers, which are the following, 171 00:21:58.190 --> 00:22:07.210 WH11NE- Sunrise: the ones that we have used and the and the we require. It passes off, screwed 172 00:22:08.390 --> 00:22:18.660 WH11NE- Sunrise: and and yes, and and of course, we apply selections on the clusters. We apply quality cuts on those, and 173 00:22:19.880 --> 00:22:32.990 WH11NE- Sunrise: the 1st one is the the rejection of the clusters that are coming from the 1st layers. So since We-we are discussing the we performed analysis in the couple strip chambers 174 00:22:33.230 --> 00:22:35.509 WH11NE- Sunrise: we require. 175 00:22:35.840 --> 00:22:37.840 WH11NE- Sunrise: We we checked the first.st 176 00:22:37.990 --> 00:22:44.880 WH11NE- Sunrise: Oh, the the cluster is coming from the 1st layers of the of the Clc. 177 00:22:45.110 --> 00:22:49.660 WH11NE- Sunrise: Any 1, 1, 2 regions, and also 178 00:22:50.500 --> 00:22:56.689 WH11NE- Sunrise: we apply additional veto on the clusters that are matched to his in re, 1, 2. 179 00:22:58.430 --> 00:23:00.180 WH11NE- Sunrise: Yes, and are you talking to? 180 00:23:00.650 --> 00:23:01.540 WH11NE- Sunrise: Oh. 181 00:23:01.670 --> 00:23:13.440 WH11NE- Sunrise: because this is done because it does. Those layers don't. Don't, don't have any any shielding compared to other other chambers. 182 00:23:13.640 --> 00:23:21.230 WH11NE- Sunrise: and can kind of clusters in them can be produced by the functional jets that are passing through the parameters. 183 00:23:21.520 --> 00:23:24.679 WH11NE- Sunrise: Yes, it contributes to the background 184 00:23:26.690 --> 00:23:45.169 WH11NE- Sunrise: and to mitigate the branch stolen. Coming from the from the neurons we reject. We reject the clusters that are coming from by rejecting the between the clusters that are matching to the segments in the 1st parallel layer. 185 00:23:46.495 --> 00:23:50.170 WH11NE- Sunrise: one or in Rb. One. 186 00:23:54.150 --> 00:24:03.120 WH11NE- Sunrise: Also we reject this region of of Csc's, because in earlier study dub 187 00:24:03.440 --> 00:24:13.300 WH11NE- Sunrise: the theme on reconstruction has been performed poorly in this region. So yes, We-we checked the 188 00:24:13.500 --> 00:24:19.499 WH11NE- Sunrise: reject the events that are coming, or reject the events. Where then, the events were triggered by 189 00:24:20.040 --> 00:24:21.870 WH11NE- Sunrise: 5 new 1. 0, Sandy! 190 00:24:26.100 --> 00:24:38.500 WH11NE- Sunrise: So, after all these selections, these are the backgrounds that we expect to have very useful background, which comes from the from the particles which are 191 00:24:40.160 --> 00:24:48.830 WH11NE- Sunrise: which are coming from the cosmics that they can be detailed, and 192 00:24:48.930 --> 00:24:54.190 WH11NE- Sunrise: once they are vetoed, the rest of them will be estimated with the with the data trimming method 193 00:24:55.068 --> 00:24:58.481 WH11NE- Sunrise: and the irreducible background which is 194 00:24:59.430 --> 00:25:12.269 WH11NE- Sunrise: produced by the standard model articles which are long lived by themselves, and the study shows that they are dominating in the background. 195 00:25:12.580 --> 00:25:21.700 WH11NE- Sunrise: Yes, and and it's going to be estimated with the with the fake rate method, this one. 196 00:25:22.870 --> 00:25:28.240 WH11NE- Sunrise: yes, and the Abcd method is some- so 197 00:25:28.530 --> 00:25:38.470 WH11NE- Sunrise: in a Ucd method, 2 main variables are chosen to distinguish the signal region of our data, and 198 00:25:38.730 --> 00:25:44.400 WH11NE- Sunrise: yes, once- once they are determined, they must be independent. And so 199 00:25:45.230 --> 00:26:02.429 WH11NE- Sunrise: it must not be correlated. So we apply cuts on them. So so we can select precisely our single region, and once a signal region is selected. We use the other regions in order to predict the background. Since these are all these are 200 00:26:03.120 --> 00:26:10.490 WH11NE- Sunrise: required as background. We use them to estimate the background in Region A, 201 00:26:10.770 --> 00:26:15.799 WH11NE- Sunrise: and this is the way we do it. So BCOT. A. R. 10. 202 00:26:16.060 --> 00:26:16.850 WH11NE- Sunrise: Problem. 203 00:26:16.990 --> 00:26:19.260 WH11NE- Sunrise: Yes, A is the the background 204 00:26:19.580 --> 00:26:22.249 WH11NE- Sunrise: estimated background in the signal reading. 205 00:26:22.470 --> 00:26:27.940 WH11NE- Sunrise: So, yes, these are the number of events in each region. 206 00:26:30.710 --> 00:26:41.080 WH11NE- Sunrise: So here's what we did. We selected the as as our 2 main variables that we've chosen, the number of hits in each cluster. 207 00:26:42.550 --> 00:26:46.319 WH11NE- Sunrise: The the Delta Phi between the cluster and the trigger millenn. 208 00:26:46.800 --> 00:27:01.729 WH11NE- Sunrise: and we can clearly see that for the background and for the different. Therefore, Delta Pi is more uniform for the for the parking data set. And so the number of kids in the parking data set is smaller. 209 00:27:01.920 --> 00:27:06.199 WH11NE- Sunrise: Also, we can see that they are not correlated so they can be used. 210 00:27:06.630 --> 00:27:15.540 WH11NE- Sunrise: And we did a scan of different. We can apply the signal over background of. 211 00:27:15.710 --> 00:27:19.060 WH11NE- Sunrise: and yes, and on X axis is the 212 00:27:20.430 --> 00:27:27.040 WH11NE- Sunrise: the Delta py cuts the Y axis, the cluster size cuts, and the axis is the signal over by cuts 213 00:27:27.340 --> 00:27:28.680 WH11NE- Sunrise: definitely absurd. 214 00:27:31.190 --> 00:27:32.410 WH11NE- Sunrise: So I know. 215 00:27:35.680 --> 00:27:55.649 WH11NE- Sunrise: So to- to validate the ABC method. We use the out of time events. These are these are the variables that we use to distinguish whether the event is from at the cost rates from the in time, domain, interaction, or from the pilot. 216 00:27:57.100 --> 00:28:12.989 WH11NE- Sunrise: These are between the regular cluster. Time is the-the mean time of the bus cluster which the mean is taken from the hit static campaigns and the regular cluster time spread is the standard deviation of the of the time. 217 00:28:13.280 --> 00:28:17.655 WH11NE- Sunrise: Oh, okay, of the time of the holidays 218 00:28:18.270 --> 00:28:23.690 WH11NE- Sunrise: closer. Okay, if you pull up the distribution. We'll see. You can calculate this. 219 00:28:24.220 --> 00:28:25.540 WH11NE- Sunrise: And so 220 00:28:26.080 --> 00:28:39.209 WH11NE- Sunrise: yes, and we simply. And if we throw the the cluster time we can see the main that the signal is coming from the main fraction points, mostly speaking. 221 00:28:39.370 --> 00:28:45.669 WH11NE- Sunrise: So this region is used for the method. The rest is used for this validation. 222 00:28:46.750 --> 00:28:47.620 WH11NE- Sunrise: Hello! 223 00:28:48.010 --> 00:28:59.220 WH11NE- Sunrise: And by yes, by validation. We're estimating the background in Region 8, and we're comparing it to the number that we have in region. 224 00:28:59.490 --> 00:29:02.989 WH11NE- Sunrise: and we see that they match. 225 00:29:04.509 --> 00:29:13.090 WH11NE- Sunrise: Yes, and the this value these values for the cuts are selected by tuning. We wait 226 00:29:13.760 --> 00:29:20.978 WH11NE- Sunrise: initially, we're basing on the signal of our background. But later we began to tune the values 227 00:29:22.720 --> 00:29:31.799 WH11NE- Sunrise: and we have, after several attempts to find the most sensitive cuts that we can apply we have paid to 228 00:29:32.170 --> 00:29:42.200 WH11NE- Sunrise: into just oh, so here's how we estimate the favorites. 229 00:29:42.580 --> 00:29:46.700 WH11NE- Sunrise: the contribution of the irreducible background. 230 00:29:47.030 --> 00:29:54.689 WH11NE- Sunrise: Oh, so we we create sample w plus chats events using full ROM to data set. 231 00:29:55.090 --> 00:30:09.490 WH11NE- Sunrise: We require type, id isolated laptop in the events we rebuild. The jets that are matching to the laptop with Delta R is a 0 point 4, and we require an enterprise. 232 00:30:10.510 --> 00:30:20.990 WH11NE- Sunrise: We yes, we- we calculate the the fake rates applied to the chat and 233 00:30:22.040 --> 00:30:25.190 WH11NE- Sunrise: that that this matches to the clusters 234 00:30:25.450 --> 00:30:33.430 WH11NE- Sunrise: to see. Yes, to- to- to see how much, how how much, how how many, oh. 235 00:30:34.200 --> 00:30:42.297 WH11NE- Sunrise: to see how many events will be, events would be, see what we see. Depending on the 236 00:30:44.596 --> 00:30:46.369 WH11NE- Sunrise: so the 237 00:30:47.730 --> 00:31:00.920 WH11NE- Sunrise: yeah. So we eventually we observe 156 events that can be considered to be fake clusters in the selected events 238 00:31:01.590 --> 00:31:04.900 WH11NE- Sunrise: and still validates this. 239 00:31:05.260 --> 00:31:08.919 WH11NE- Sunrise: This method we select. 240 00:31:09.280 --> 00:31:13.390 WH11NE- Sunrise: We select 2 validation regions anyway. 241 00:31:14.180 --> 00:31:16.179 WH11NE- Sunrise: and then the same A/C plane. 242 00:31:16.400 --> 00:31:24.250 WH11NE- Sunrise: Oh, yes, and the with the blue regions are the-, the control regions that we select. 243 00:31:25.372 --> 00:31:27.510 WH11NE- Sunrise: Until we observe. 244 00:31:28.170 --> 00:31:36.669 WH11NE- Sunrise: And we we observed the number of events in those, and we they match to the and the predictions match to the, to the observation. 245 00:31:42.190 --> 00:31:53.549 WH11NE- Sunrise: So the so we have. We perform the systematic. We performed the calculation, but calculated the systematic effects 246 00:31:53.740 --> 00:32:05.140 WH11NE- Sunrise: we have used. This is not answering these. We have used the Z 2 essentials, proudness and policy, and 247 00:32:05.960 --> 00:32:12.629 WH11NE- Sunrise: and the single single beyond data set as a as a experimental data. 248 00:32:12.930 --> 00:32:21.920 WH11NE- Sunrise: And we performed the measurement of the systematic uncertainty. Seeing a large team or give me on this. Oh. 249 00:32:22.270 --> 00:32:27.730 WH11NE- Sunrise: at large, in the in the region with large team on us values. 250 00:32:28.070 --> 00:32:29.040 WH11NE- Sunrise: Oh, okay. 251 00:32:29.360 --> 00:32:35.519 WH11NE- Sunrise: So there are some. These are the requirements that we apply on data 252 00:32:36.242 --> 00:32:42.069 WH11NE- Sunrise: is only on 27th for her to be fired. 253 00:32:43.910 --> 00:32:47.290 WH11NE- Sunrise: Yeah. So the kinematic selections on the new ones. 254 00:32:47.410 --> 00:32:53.419 WH11NE- Sunrise: the tag and probe method was used in this case as well, and 255 00:32:53.760 --> 00:32:59.750 WH11NE- Sunrise: the Yes. As I said, the is restricted in which 256 00:33:01.490 --> 00:33:07.699 WH11NE- Sunrise: and this is one of the one of the plots for the uncertainty 257 00:33:08.010 --> 00:33:18.235 WH11NE- Sunrise: for the of one of the vetoes particularly, this is the 1, 1, 2 veto which rejects the 1st layer of the 258 00:33:18.790 --> 00:33:23.610 WH11NE- Sunrise: oh versus the number of primary vertices. 259 00:33:26.708 --> 00:33:29.380 WH11NE- Sunrise: Sorry this is the 260 00:33:29.570 --> 00:33:37.000 WH11NE- Sunrise: for for Z, for the, for the multiparlor data. These are the efficiencies, and the ratio of those is taken to consider. 261 00:33:41.540 --> 00:33:47.840 WH11NE- Sunrise: So so these are the uncertainties that we have estimated. 262 00:33:48.190 --> 00:33:49.250 WH11NE- Sunrise: Not all. 263 00:33:50.290 --> 00:33:55.581 WH11NE- Sunrise: So the there-. There is no certainty on the cross section of the process. 264 00:33:56.080 --> 00:34:03.410 WH11NE- Sunrise: There's a There's us, and and on the integrated 265 00:34:03.740 --> 00:34:08.270 WH11NE- Sunrise: for the rest of the cluster and for the rest of the cluster selections 266 00:34:09.088 --> 00:34:13.980 WH11NE- Sunrise: estimate for all of those. So 267 00:34:14.750 --> 00:34:19.569 WH11NE- Sunrise: so for the for the ABC. Prediction, we don't apply any uncertainties. 268 00:34:19.940 --> 00:34:26.050 WH11NE- Sunrise: Oh, so statistical uncertainties assigned to the 269 00:34:26.199 --> 00:34:33.540 WH11NE- Sunrise: chance. Thank you. Chance. Oh, sorry fake Rains this one, I think. 270 00:34:34.670 --> 00:34:38.719 WH11NE- Sunrise: And for Monte Carlo, yeah, so. And 271 00:34:38.909 --> 00:34:47.120 WH11NE- Sunrise: for Monte Carlo, yes, these are the uncertainties that we that we considered enter. 272 00:34:47.710 --> 00:34:48.550 WH11NE- Sunrise: Yes. 273 00:34:48.929 --> 00:34:58.329 WH11NE- Sunrise: what is it here? And plus the trigger scale factors, uncertainties, the and the statistical uncertainties for the multi parallel. 274 00:35:02.210 --> 00:35:04.779 WH11NE- Sunrise: So these are our state limits. 275 00:35:05.020 --> 00:35:12.960 WH11NE- Sunrise: The first.st These are these are the 1st Cms results for these for- for this kind of signature. 276 00:35:14.740 --> 00:35:29.926 WH11NE- Sunrise: and yes, we can see. These are the limit first, st for different masses, you know these, but in particular, for that's particularly for 5 plus 5 minus decay. Mode. 277 00:35:32.450 --> 00:35:43.670 WH11NE- Sunrise: yes, and we're able to get about 6 to 10 to negative 5 branching fractions limit on the branching fraction. 278 00:35:44.380 --> 00:35:52.359 WH11NE- Sunrise: Oh, yes, and these are the signal yields that we have that we have calculated in different regions. 279 00:35:53.160 --> 00:35:58.409 WH11NE- Sunrise: So yes, the total background is so sorry. 280 00:35:58.780 --> 00:36:09.760 WH11NE- Sunrise: so sorry. These are. These are the the number of the background events and and total observed events. 281 00:36:14.560 --> 00:36:21.360 WH11NE- Sunrise: and we we interpolate the these curves for different mass, for different masses. 282 00:36:21.560 --> 00:36:26.750 WH11NE- Sunrise: And this is the yes, and this is actually called for 283 00:36:28.860 --> 00:36:37.430 WH11NE- Sunrise: And so as a as a summary, and say that this is the second search for in the using department data set. 284 00:36:37.700 --> 00:36:45.490 WH11NE- Sunrise: it's particularly sensitive for lowness at the low Ptl piece with longer lifetimes. 285 00:36:46.971 --> 00:36:54.330 WH11NE- Sunrise: This one else is going to be and virtual affection. So, okay. 286 00:36:59.290 --> 00:37:03.270 WH11NE- Sunrise: okay, do we have questions for 287 00:37:04.298 --> 00:37:11.870 WH11NE- Sunrise: can you actually go to slide 29. Your limits live 288 00:37:12.970 --> 00:37:26.350 WH11NE- Sunrise: so it could be that I can't tell the colors. So if that's the case, let me know. But it looks like I would naively expect there to be some trend as you go up in mass like 1, 2, 3 would be some sort of smooth. 289 00:37:26.810 --> 00:37:30.580 WH11NE- Sunrise: you know transition, but you actually have your one. 290 00:37:30.950 --> 00:37:38.950 WH11NE- Sunrise: and then the 3 is the next one, the next lowest, and then you go to the 2. So do you understand why you have this sort of complicated mass dependence. 291 00:37:39.850 --> 00:38:07.279 WH11NE- Sunrise: like, if the one like, if you're 100 like, you're 100 or like 5 proper decay length. You have your 0 point 3, and is the lowest limit. You're most stringent, and then you have one that I would kind of expect it to be 2. But instead of your your 3 mass point is actually better, and then the 2 1 is above it. Do you know why you're less sensitive to your 5 mass of 2 versus your 5 mass of 3 or 5 mass of one. 292 00:38:07.940 --> 00:38:12.420 WH11NE- Sunrise: Oh, right? 293 00:38:13.990 --> 00:38:21.049 WH11NE- Sunrise: So I think it's a good yeah, to be honest. 294 00:38:21.230 --> 00:38:22.920 WH11NE- Sunrise: So some 295 00:38:23.060 --> 00:38:48.009 WH11NE- Sunrise: this could account. I don't have a certain answer to it. Why, why is that happening? No, this is this is part of. Maybe I can help. This is why you've been working on extra signal samples. Generation. Oh, yeah. So this is part of the question. Why, you would ask during approval. We don't expect this kind of behavior. That's the 296 00:38:48.110 --> 00:38:57.900 WH11NE- Sunrise: from what we see previously, all the Mds limits are pretty much mass independent. And we are. I think this is 297 00:38:58.840 --> 00:39:06.429 WH11NE- Sunrise: what we've checked internally is also the case. What we running here is really low set, because there is 298 00:39:06.650 --> 00:39:28.750 WH11NE- Sunrise: using direct simulation to get the branching region of 10 to minus 5. So and then we put place a high android cuts to to get rid of the that cuts down statistics and also around is working on getting new private samples 299 00:39:29.190 --> 00:39:44.850 WH11NE- Sunrise: hopefully better simulators. It means there's also a physics reason? Right? This it's a b mass is basically, it's something on your face-face. If you is that coming into play? No, I think it does take that into account. 300 00:39:45.260 --> 00:39:49.119 WH11NE- Sunrise: Okay, thank you. Steve has some answer as well. 301 00:39:51.680 --> 00:39:57.259 Stephen Mrenna: Hi, yeah, I I don't wanna be on this. How? How does your limit change? If 5 goes to Kk. 302 00:40:00.250 --> 00:40:02.759 WH11NE- Sunrise: When the file goes to kick in. 303 00:40:02.760 --> 00:40:05.660 Stephen Mrenna: Yes, if if 5 doesn't go to pi pi, if it goes to Kk. 304 00:40:10.009 --> 00:40:10.869 WH11NE- Sunrise: I guess. 305 00:40:11.660 --> 00:40:18.070 WH11NE- Sunrise: Well, we we don't, we don't. Well, we didn't measure the we didn't consider that the. 306 00:40:18.830 --> 00:40:22.340 WH11NE- Sunrise: And then consider the application of Yeah. 307 00:40:22.340 --> 00:40:26.340 Stephen Mrenna: Do you? Do you think your analysis is is going to depend upon the mass of the tracks or. 308 00:40:28.010 --> 00:40:31.229 WH11NE- Sunrise: Pretty much. No, yeah. 309 00:40:31.940 --> 00:40:36.439 Stephen Mrenna: It. Just if if you're sitting at one gev, and if it's anything like. 310 00:40:36.980 --> 00:40:43.550 Stephen Mrenna: you know, A. A. Qcd. And you have some, it's gonna see the file, the the the Qcd file 311 00:40:44.800 --> 00:40:48.354 Stephen Mrenna: which decays. Dek, so so if you look at the 312 00:40:50.244 --> 00:40:57.479 Stephen Mrenna: the meson probability as a function of mass around one gev. That that Phi is going to go mainly to Kk. 313 00:41:01.550 --> 00:41:02.730 Stephen Mrenna: Instead of pipeline. 314 00:41:03.090 --> 00:41:05.139 Stephen Mrenna: But I don't think it changes your limit, but. 315 00:41:09.530 --> 00:41:16.429 WH11NE- Sunrise: Yeah, I I think they're not reconstructing it right? Because it. This is this, the decay happens in the in the 316 00:41:16.780 --> 00:41:18.349 WH11NE- Sunrise: neuron system. Right? 317 00:41:18.530 --> 00:41:20.979 WH11NE- Sunrise: Right? So it's it's not that they have a track 318 00:41:21.320 --> 00:41:32.360 WH11NE- Sunrise: or K or pi, it's it's called pi to say there's a signal, I think. But yeah, awesome. 319 00:41:33.990 --> 00:41:43.609 Stephen Mrenna: As you go up in mass. It's gonna you know. It'll probably decay to rho pi or Rho or something, and you're gonna get, then distribute. You'll have more electromagnetic energy. 320 00:41:46.080 --> 00:41:49.140 WH11NE- Sunrise: Oh, you say, for looking at the the Monte Carlo itself? 321 00:41:49.850 --> 00:41:51.850 WH11NE- Sunrise: Yeah, not the signature. 322 00:41:52.060 --> 00:41:53.250 Stephen Mrenna: For the signature. Yes. 323 00:41:53.250 --> 00:41:53.850 WH11NE- Sunrise: Yeah. 324 00:41:53.990 --> 00:41:58.250 Stephen Mrenna: You as you go up in mass, you you expect this fire to decay. Something like. 325 00:41:58.490 --> 00:42:01.147 Stephen Mrenna: you know, standard model corks coupled to to 326 00:42:02.840 --> 00:42:05.089 Stephen Mrenna: to a strong to the Qcd acceptance. 327 00:42:06.650 --> 00:42:09.340 Stephen Mrenna: So so it should decay in a standard model, like way. 328 00:42:10.190 --> 00:42:28.229 WH11NE- Sunrise: Yeah. So in search, we simply assume the 100% branching ratio for the final state. At some point we would like to have a more realistic branching ratio of how these 5 would go what we're going to in the 329 00:42:28.460 --> 00:42:34.099 WH11NE- Sunrise: different. As as you pointed out, the mass of the 5 differs. 330 00:42:34.150 --> 00:42:53.909 WH11NE- Sunrise: But I think the power of this search really comes from the fact that it doesn't really matter what the Hadrons indicates into. I don't expect the limit to change if it's 100% to Kk or pi pi, because that's what we've seen in the previous analysis, because the Hadron will create a shower 331 00:42:53.910 --> 00:43:05.790 WH11NE- Sunrise: as long as it creates enough showers not. It's not just a couple of tracks. It only matters if you if you have sufficient em or electronic energy. 332 00:43:06.020 --> 00:43:22.139 WH11NE- Sunrise: So we are also working on 5 to 5 plus pi, 0 5 0, which will be predominantly managing. So those will be weaker because the steel stop more em shower than hydronic ones. 333 00:43:22.280 --> 00:43:32.065 WH11NE- Sunrise: but other than that it will. I would expect the the search will still be sensitive to a different demo. 334 00:43:33.270 --> 00:43:33.740 Stephen Mrenna: I agree. 335 00:43:33.740 --> 00:43:39.139 WH11NE- Sunrise: Harder to harder to assimilate all the branching ratio as a function of mass. 336 00:43:39.140 --> 00:43:42.720 Stephen Mrenna: Right. I I agree with you 100, but I think we want to make that 337 00:43:42.940 --> 00:43:45.260 Stephen Mrenna: be able to make that independent statement 338 00:43:46.170 --> 00:43:47.689 Stephen Mrenna: because it to me. It looks bad 339 00:43:48.020 --> 00:43:53.070 Stephen Mrenna: that you're you're you're assuming something that isn't what you expect. 340 00:43:55.200 --> 00:43:58.540 WH11NE- Sunrise: Oh, you mean the mass dependency in the- in the limit. 341 00:43:59.080 --> 00:44:02.500 Stephen Mrenna: Or just the defy 3 Gv. Would decay. Main. 342 00:44:03.092 --> 00:44:07.239 WH11NE- Sunrise: Is an odd assumption that you're saying. 343 00:44:07.240 --> 00:44:08.320 Stephen Mrenna: Yeah, that's all. 344 00:44:08.320 --> 00:44:10.810 WH11NE- Sunrise: Okay, okay. I'll take it. 345 00:44:11.170 --> 00:44:13.050 Stephen Mrenna: Yeah, I don't. I don't want you to get grief. I think 346 00:44:13.860 --> 00:44:19.439 Stephen Mrenna: I think the limits robust. I think it's a great analysis. I'm sorry I usually start off by saying those sort of things. I apologize. This is, Thank you. 347 00:44:19.975 --> 00:44:25.870 WH11NE- Sunrise: We did not have that intuition built it. But yeah. 348 00:44:28.990 --> 00:44:29.729 WH11NE- Sunrise: thank you. 349 00:44:30.690 --> 00:44:44.399 WH11NE- Sunrise: So I had a question about the the events that you observe, since they're only 181. Did you actually look at all of them like one by one, because this is like close to when when you do some. 350 00:44:44.850 --> 00:44:50.230 WH11NE- Sunrise: you know, search, or whatever, and the number is in depends. 351 00:44:50.500 --> 00:45:05.319 WH11NE- Sunrise: You really tempted? I'm gonna look at each of them and understand it. You know. I tried to see if I did matches my irreducible background. I expected. What? What is over there on the other side? Besides, whatever you cut right, just did you do any of this 352 00:45:05.600 --> 00:45:12.890 WH11NE- Sunrise: exploration of event displays? No, no, we haven't. Let me check that. 353 00:45:13.050 --> 00:45:14.769 WH11NE- Sunrise: Okay, one by one. 354 00:45:18.630 --> 00:45:26.690 WH11NE- Sunrise: I also was confused. I didn't want to stop you as something that is really a detail, I guess. But it was a lot earlier, like a slide 11 or something 355 00:45:27.257 --> 00:45:50.950 WH11NE- Sunrise: when you mentioned the something about the bee parking data set saying, Purity, yeah, at the very bottom said, you know, purity of 70 to 80% of the data set was cheap. What does it mean? Purity purity means that in the collected data, in 70 to 80% 356 00:45:51.050 --> 00:45:58.530 WH11NE- Sunrise: of the events actually could contain 2 emails I see. 357 00:46:00.450 --> 00:46:01.343 WH11NE- Sunrise: Accepted, too. 358 00:46:07.610 --> 00:46:11.170 WH11NE- Sunrise: Is this trigger also present in 1 3? 359 00:46:12.060 --> 00:46:14.359 WH11NE- Sunrise: Oh, it's so much. 360 00:46:16.540 --> 00:46:17.360 WH11NE- Sunrise: Yeah. 361 00:46:18.250 --> 00:46:33.030 WH11NE- Sunrise: And like, do you have an idea how this result will improve the main difference from run 2 to run 3. For this is the run. 2. It's only 2018, the 2018 one, a single muon based seat 362 00:46:33.200 --> 00:46:45.404 WH11NE- Sunrise: in run 3 until 2024. This is replaced with and dialectron, I mean dielectron seeds. It's not exactly single neon, but it's mostly hoping to catch 363 00:46:46.080 --> 00:46:52.270 WH11NE- Sunrise: A beam is on deaking to 2 muons within an eta range of like 1.6 364 00:46:52.530 --> 00:47:00.249 WH11NE- Sunrise: for if you're looking for any bdk's and stuff, it's still quite a bit efficient. And 365 00:47:01.166 --> 00:47:21.440 WH11NE- Sunrise: yeah, and there's a lot more data collected. Yeah. But if you have, I don't know. We haven't thought about repeating this with one free parking, because if you have time to monitor you, you already use the 2 sides and prop and tab, and we really the signal comes from the prop side, where you have only a jet and not new one. 366 00:47:21.580 --> 00:47:26.690 WH11NE- Sunrise: the some Lpdk longer into the immune system. 367 00:47:26.860 --> 00:47:38.119 WH11NE- Sunrise: But sync, yeah, it's not trivial to just use the diving on parking. 368 00:47:38.470 --> 00:47:40.549 WH11NE- Sunrise: and there's no muon on that side. 369 00:47:41.290 --> 00:47:45.060 WH11NE- Sunrise: So you really need the unbiased row. 370 00:47:49.240 --> 00:47:57.049 WH11NE- Sunrise: I also had another question on slide. I think it was 22, or 23, but anyway, so in general it's just about 371 00:47:57.220 --> 00:48:17.329 WH11NE- Sunrise: the choice, for the cuts, say the Delta phi between the cluster and the mu, for example, right? That it was like 2.2. Is it just from, you know like these, because I I had that sorry when you were talking about this. I was just looking somewhere somewhere. So it just comes from this distribution there on top that. 372 00:48:17.510 --> 00:48:29.170 WH11NE- Sunrise: So so, as I, as I said initially, so, the initial focus was to get as much signal over by ground ratio as we can, but 373 00:48:29.340 --> 00:48:38.439 WH11NE- Sunrise: but but that- that- that is observed when the cuts are very tight and we're just running out of that. So so we have. 374 00:48:38.700 --> 00:48:46.049 WH11NE- Sunrise: So we decided to tune the parameters so we can get as as much as possible. 375 00:48:46.930 --> 00:48:52.069 WH11NE- Sunrise: So I think the yeah. So we did several trials. 376 00:48:52.390 --> 00:48:58.319 WH11NE- Sunrise: We- we tried several pairs of the cuts, and yes, and we end up- ended up in these ones. 377 00:49:06.480 --> 00:49:11.429 WH11NE- Sunrise: And is there any measurement of the the in the analysis, or or do you 378 00:49:11.930 --> 00:49:15.350 WH11NE- Sunrise: need at all to look at the measuring which both 379 00:49:15.630 --> 00:49:21.999 WH11NE- Sunrise: masons are, you know, like Standard Mouse instead of the Phi into I. But you know not long lived. But 380 00:49:22.140 --> 00:49:25.339 WH11NE- Sunrise: you get the 2 J size. 381 00:49:26.190 --> 00:49:36.030 WH11NE- Sunrise: Yeah, right? Do you? Do you even care at all about like that to be a denominator of something or or of 382 00:49:38.070 --> 00:49:50.017 WH11NE- Sunrise: right because it. That's I don't know. Like if you I guess that it doesn't really help. I mean the branching ratio that limit that we set for Long live is 10 to minus 5. So 383 00:49:50.680 --> 00:49:52.880 WH11NE- Sunrise: I think there, there are rooms 384 00:49:53.220 --> 00:50:02.349 WH11NE- Sunrise: for for these such decades. Ju-just by looking at pure ratios. I think those are still allowed. 385 00:50:03.310 --> 00:50:06.090 WH11NE- Sunrise: or it's ready case to happen absolutely. 386 00:50:14.930 --> 00:50:29.780 WH11NE- Sunrise: I had a reality on the clustering that you described at the beginning. How, if understood correctly, you must have some seed to which you are the other particles. 387 00:50:30.230 --> 00:50:37.205 WH11NE- Sunrise: How do you? So? What? How do you start the cluster? So the clustering starts. 388 00:50:38.400 --> 00:50:40.680 WH11NE- Sunrise: so there is a 3.rd 389 00:50:40.980 --> 00:50:43.609 WH11NE- Sunrise: So it starts from the 390 00:50:44.920 --> 00:50:53.960 WH11NE- Sunrise: from what- what I mean. You can't start from a from a random one and start looking over the others, and 391 00:50:54.130 --> 00:51:06.679 WH11NE- Sunrise: yes, by simply applying the this calculating business from it and checking if it if it's within the given business parameter. 392 00:51:06.940 --> 00:51:13.930 WH11NE- Sunrise: It is considered to be in that cluster that though 393 00:51:14.210 --> 00:51:18.340 WH11NE- Sunrise: the way the way it's evolving. 394 00:51:20.550 --> 00:51:31.130 WH11NE- Sunrise: yeah, apologize like it's either the mean or the-, the- the last of the the last development that is being added to the cluster. It's 395 00:51:32.760 --> 00:51:33.840 WH11NE- Sunrise: refresh token 396 00:51:34.240 --> 00:51:47.969 WH11NE- Sunrise: to say. But yeah, if I can add some more details. So it's like this is A, that's the base microphone. So it doesn't really matter where you started. It's the configuration. 397 00:51:48.300 --> 00:51:56.569 WH11NE- Sunrise: You can start at any point, and then you reach the same stuff. It's really it's really trying to capture the over density 398 00:51:56.740 --> 00:52:03.310 WH11NE- Sunrise: right? So you start from one and then start adding, and it will move to where there are more point. 399 00:52:03.630 --> 00:52:15.919 WH11NE- Sunrise: No, it's basically. So you start from any point, and you draw the circle and see which are, is it to classify if it's call point a noise point or boundary point. And then 400 00:52:16.070 --> 00:52:24.809 WH11NE- Sunrise: from that is a basically global. So if you can, you zoom over all the points and and try to custom. 401 00:52:24.950 --> 00:52:28.619 WH11NE- Sunrise: If you draw this, draw the circle on each point, and then you will see 402 00:52:28.890 --> 00:52:44.909 WH11NE- Sunrise: where you can decide on how many cups have been done in the whole thing. It doesn't matter how you where, which one you start from. Unlike jet algo phone, where you have a physical picture of. Yeah. 403 00:52:46.800 --> 00:52:52.040 WH11NE- Sunrise: don't need that fancy, but it didn't work. Yeah, thank you. 404 00:52:53.490 --> 00:52:56.340 WH11NE- Sunrise: Do we have more questions? 405 00:52:57.510 --> 00:52:59.952 WH11NE- Sunrise: If not, we can. It's like.