1 E T miss measurement E T miss is an important signal for - new physics (e.g. SUSY, H  ZZ  ll ) - reconstruction of a narrow invariant mass distribution.

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Presentation transcript:

1 E T miss measurement E T miss is an important signal for - new physics (e.g. SUSY, H  ZZ  ll ) - reconstruction of a narrow invariant mass distribution for new (heavy) particles involving neutrinos (e.g. A  ) E T miss resolution - The detector performance in terms of E T miss resolution was studied by using fully-simulated H/A  events in the H/A mass range 100–500 GeV. - Typical E T miss values for these events are in the range GeV. [Simulation] A  - At low luminosity - With minimum-bias events |  | < 3 : full simulation 3 < |  | < 5 : not fully simulated, but the particle energies were smeared according to the expected resolution -the contribution of the calorimeter resolution to  ( E T miss ) is small - CPU time 第6回 KEK 解析会合 HI

2 ATLAS Calorimeters 13.3 m 6.9 m 8.5 m 12.2 m 4.5 m 2.3 m Hadron calorimeter requirements - Energy resolution

3 Liq Ar EM Calorimeter Liq Ar FCAL

4 [Calorimeter coverage] - Calorimetric coverage up to |  |= 5 is essential the resolution of the E T miss vector, as calculated at particle level for A  events with m A = 150 GeV, degrades from 2.3 GeV to 8.3 GeV if the calorimeter coverage is reduced from |  |< 5 to |  |< 3. - On the other hand, the contribution of the forward region to the E T miss resolution is small. The resolution of the E T miss vector, as obtained with full simulation of A  events with m A = 150 GeV, was found to be about 7 GeV (to be compared with 2.3 GeV at particle level). the main contribution coming from - the barrel region (about 5 GeV), - followed by the end-cap region (about 4 GeV), and - the forward region (about 3 GeV) -The dead material in the transition region between the barrel and the end-cap calorimeters has no significant effect on the width of the core of the E T miss distribution. The impact of these regions on the high- E T miss tails is not the case. Resoulution of  (p xy miss ) of each component of the E T miss vector is defined as  the sum of the x (y) components of the momenta of all generated particles (neutrinos and muons excluded) without any pseudorapidity restriction the sum of the x (y) momenta as reconstructed from the calorimeters

5  “full simulation in |  | < 3” |  | < 3 : full simulation 3 < |  | < 5 : not fully simulated, but the particle energies were smeared according to the expected resolution The electronic noise of the EM Calorimeter was included, and a low-energy cut-off at 1.5  was applied to the transverse energy deposited in each cell. The resolution of the E T miss components varies between about 5 and 10 GeV when m A varies between 100 and 500 GeV. The points shown in Figure 9-34 can be fitted with the form where E T is expressed in GeV. If the contribution of the limited coverage is unfolded, Then the resolution becomes  in case of the perfect coverage ?

6 -with minimum-bias events (up to 48 events) - full simulation in the region |  | < 5 - the parametrisations obtained for both physics samples are the same E T miss resolution scales like with k ~ 0.46 E T miss resolution v.s. total transverse energy

7 The contribution of the pile-up in the forward region was neglected, because it is small after a tower energy cut-off is applied. The E T miss resolution is degraded by the presence of pile-up. The impact can be reduced by applying a cut-off on the energy content of the calorimeter towers. The resolution is best for a cut-off of ~1 GeV, which corresponds to about 2.5  of the quadratic sum of the electronic noise and pile-up. High-luminosity case

8 The contribution to  (p xy miss ) coming from the pile-up and electronic noise alone, as obtained by applying the optimum tower cut-off of 1 GeV. The contribution of the pile-up in the FCAL is small if a cut-off is applied, which justifies the choice of simulating the pile-up up to |  |= 3 only.

9 E T miss tails Consider a heavy Standard Model Higgs boson with a mass in the range GeV in the decay mode H  ZZ  ll one of the potentially dangerous backgrounds comes from Z+jet(s) events, where a badly measured jet could fake large E T miss. The rejection factor needed is of the order of 1,000 in the region of E T miss larger than 200 GeV. [Event sample] - 4,667 Z+jet(s) events - full simulation - p T > 200 Gev for Z at the generator level - Z   to see effects of - calorimeter cracks and dead material Particle level muon momentum was used in the E T miss calculation, correcting simply for the average energy loss in the calorimeter. To eliminate radiative muons, events with a jet reconstructed within  R = 1 of the direction of the muon were rejected.

10 E T miss tails (cont’d) 3,826 events passed the selection Result is the dotted line in Fig events with E T miss above 200 GeV Those events contain a high-p T neutrino  genuine E T miss The full line represents the E T miss reconstructed in the event if the jet balancing the p T of the Z would go completely undetected. the rejection factor of 1,000 needed above 200 GeV is achieved

11 the pseudorapidity of the jet with the highest pT for the events that have a E T miss larger than 50 GeV around |  |= 1 the region of the vertical crack between the barrel and extended barrel calorimeters around |  |= 0 particles from the jets are parallel to the orientation of the scintillator tiles of the tile barrel calorimeter. In this configuration, the sampling fraction of the calorimeter is less uniform E T miss tails (cont’d)

12 [sample] 4,554 Z+jet(s) events p T (Z) > 40 Gev (The range of energies of the jets that are contributing to this sample is very large: from 20 GeV to about 800 GeV.) p xy calo : reconstructed in the calorimeter p xy  : the p T components of the two muons from the Z decay - muon momentum is reconstructed in the Muon System - no cut to reject radiative muons has been applied - the two components p xy calo and p xy  should be equal and opposite (since there is no true E T miss in these events, except for the few events that may contain a neutrino) - the distribution of their difference can be fitted by a Gaussian whose sigma gives the resolution on the measurement of the components of the E T miss vector in the event  (p xy miss ) vs.  E T in the calorimeter

13 [In the full simulation] - the E T miss is calculated from the sum of the energy of all cells of the calorimeters, applying to each calorimeter a single constant factor that corrects on average for the effect of the non-compensation of the calorimeter. - these coefficients have been fitted to minimise the resolution for the overall sample. [In ATLFAST] - the p xy calo is calculated from the energy of the reconstructed jets at particle level (cone  R = 0.4) smeared with a resolution given by where cells unused in clusters are also taken into account. [Note] The best jet energy resolution is obtained when the calibration coefficients depend on the jet energy and pseudorapidity and when correction terms taking into account the energy loss in dead material are added. Therefore the resolution obtained here with the simple algorithm used in this study is not optimum.  (p xy miss ) vs.  E T calo (cont’d)

14 Results are shown in Fig The full simulation gives a resolution about 20% worse than ATLFAST. - The resolution presented is larger than the experimental resolution  (p xy miss ) given in Fig and Fig 9-35 wich is fitted with -The above expression does not include the fluctuation of the fragmentation process -That contributes to the overall p T balance of the event which is shown in here. e.g. the rms of the sum of the p T of the particles resulting from the fragmentation of a 200 GeV quark (resp.1000 GeV) at |  |= 0.3 is 5.5 GeV (resp. 16 GeV). - In addition, in the sample of events considered here, the transverse energy is deposited essentially by a single high-p T jet. - When an equivalent amount of transverse energy is deposited by various jets, the most common physics case, then the resolution is dominated by the statistical term.  (p xy miss ) vs.  E T calo (cont’d)

15 Z   final states Z   reconstruction from all decay products Full simulation samples of Z    jet + lepton Z    jet  l l   can be reconstructed under the assumptions  - m   = 0  - the direction of the neutrino system from each   decay (   , 2 = l +  ) coincides with that  of the detected products of the  decay  - the  decay products are not back-to-back then  E T miss Z  l jet  2 = l + 

16 The mass resolution obtained is proportional to  (E T miss )/|sin  | (  azimuthal angle between the jet and the lepton) The variable  depends on the p T of the parent particle (e.g. a Z), and it is oncentrated around  if the p T is small. If  is close to  (back-to-back events), the neutrino system yields bad solutions giving rise to tails at high values of the reconstructed mass.

17 [1 st step] the mass distribution as generated by PYTHIA [2 nd step] the particle level information, that is using the generated energies and directions. In particular, the components of the E T miss vector were calculated without any restriction on the pseudorapidity coverage of the detector. At this stage, the event loss and the deterioration of the mass resolution were due to the assumption on the directions of the  decay products. [3 rd step] the same way as in the 2 nd step but using a cut |  |< 5 for the E T miss reconstruction. The resulting event loss and deterioration of the mass reconstruction were due to the limited pseudorapidity coverage of the detector. [4 th step] px miss and py miss as obtained from full simulation were used. The deterioration of the performance was due to the E T miss experimental resolution. [5 th step] the reconstructed energies and directions of the jet and the lepton were used. It can be seen that the event losses and the deterioration of the mass reconstruction and resolution are mainly due to the assumption on the particle directions, to the limited pseudorapidity coverage of the detector and to the E T miss resolution.

18 An analysis to extract a clean sample of Z events Cuts: The  -jet should be identified according to the criteria described in Section (isolated narrow jet & N tr =1 (or 3)) p T jet > 30 GeV, |  | jet < 2.5. p T lepton > 16 GeV and |  | lepton < 2.5 for the lepton produced in the leptonic  decay. No tagged b-jet in the event. Transverse mass m T (lepton-E T miss ) < 50 GeV. 1.8 <  < 2.7 or 3.6 <  < GeV < m  < 116 GeV.

19 - About 3,500 signal events satisfying the above cuts are expected with 10 fb The background is about 20% (Table 9-9). - The background can be further reduced by applying a more stringent cuts on thetransverse mass (m T < 25 GeV), which removes W+jet events, and on the missing transverse momentum (E T miss > 18 GeV), which rejects bb final states. With this set of cuts, the background in the mass window is reduced to ~6% and about 1,300 signal events are expected for 10 fb The reconstructed Z mass obtained in this way (Figure 9-54) is well centered at the nominal value and has a resolution of about 9 GeV. [Note] -the results shown in the last row of Table 9-8 were obtained without applying any cuts. - In particular the  cut improves significantly both the mass resolution and the correct reconstruction of the mass peak.

20 H/A   - The same method for reconstructing the  invariant mass as described for  final states. - The fully-simulated sample of events from direct A production described was used for this study. Events with 2.9 <  < 3.4 were rejected in order to improve the quality of the mass reconstruction. m A = 150 GeV  ~ 20 GeV m A = 450 GeV  ~ 40 GeV Low luminosity

21 High luminosity -The pile-up has a large impact on the E T miss resolution and therefore on the A mass resolution. - A cut-off on the minimum transverse energy in each calorimeter tower was applied to improve the E T miss resolution. - This cut affects the energy scale. - Therefore, prior to the mass reconstruction, the reconstructed  -jet energy was corrected by a factor obtained by comparing the reconstructed and the generated  -jet energy. - The tower cut-off (~1 GeV) which optimizes the E T miss resolution was applied at high luminosity. m A = 150 GeV  ~ 30 GeV

22 Tower cut-off m A = 150 GeV - The ratio of the standard deviations of the reconstructed  mass spectrum high luminosity and low luminosity, as a function of the tower E T cut-off - For the optimum cut-off, this ratio is about two. - The event acceptances in the mass window ± 1.5  (m  ) at low and high luminosity - The signal acceptance was 60% of the acceptance at low luminosity. - This is due to the fact that in the presence of pile-up, the fraction of events for which the neutrino system has unphysical solutions is larger.

23 -To minimize the effect of the pile-up, multiple-sampling and digital-filtering techniques for the calorimeter signals will be used. - Preliminary results obtained by performing digital filtering or simple weighted combinations of multiple samplings look promising and show some improvement in the performance. In conclusion, the impact of pile-up on the physics sensitivity is that the significance of a possible  signal will most likely be a factor smaller at high luminosity than it would be naively expected from the increase by a factor of ten in luminosity.