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DESY1 Particle Flow Calorimetry At ILC Experiment DESY May 29 th -June 4 rd, 2007 Tamaki Yoshioka ICEPP, Univ. of Tokyo Contents.

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Presentation on theme: "DESY1 Particle Flow Calorimetry At ILC Experiment DESY May 29 th -June 4 rd, 2007 Tamaki Yoshioka ICEPP, Univ. of Tokyo Contents."— Presentation transcript:

1 5/30/2007LCWS07 @ DESY1 Particle Flow Calorimetry At ILC Experiment LCWS07 @ DESY May 29 th -June 4 rd, 2007 Tamaki Yoshioka ICEPP, Univ. of Tokyo Contents 1. Introduction 2. Particle Flow Algorithm 3. Current Performance 4. Summary

2 5/30/2007LCWS07 @ DESY2 Introduction - Most of the important physics processes to be studied in the ILC experiment have multi-jets in the final state. → Jet energy resolution is the key in the ILC physics.

3 5/30/2007LCWS07 @ DESY3 Introduction - Most of the important physics processes to be studied in the ILC experiment have multi-jets in the final state. → Jet energy resolution is the key in the ILC physics. Precision studies of the Higgs boson will be ILC bread and butter. e + e - → ZH → qqbb @ 350GeV, 500fb -1 Invariant mass of two b-quark jets for different jet energy resolution. → 40% luminosity gain H → WW* 40% lum. gain e + e - → ZHH 40% lum. gain WW scattering, 30~40% lum. gain

4 5/30/2007LCWS07 @ DESY4 Introduction - Most of the important physics processes to be studied in the ILC experiment have multi-jets in the final state. → Jet energy resolution is the key in the ILC physics. Precision studies of the Higgs boson will be ILC bread and butter. e + e - → ZH → qqbb @ 350GeV, 500fb -1 Invariant mass of two b-quark jets for different jet energy resolution. → 40% luminosity gain H → WW* 40% lum. gain e + e - → ZHH 40% lum. gain WW scattering, 30~40% lum. gain Precise jet energy resolution for typical ILC jet energies, say σ E /E ~ 30%/√E, would be an essential tool for identifying and distinguishing W’s, Z’s, H’s, and top, and discovering new states or decay modes.

5 5/30/2007LCWS07 @ DESY5 Jet Reconstruction @ ILC - Q. How to achieve the best attainable jet energy resolution? - A. Since the momentum resolution for the charged particle measured by trackers is much better than the energy resolution of calorimeters, the best energy resolution is obtained by reconstructing momenta of individual particles avoiding double counting among Trackers and Calorimeters. - Charged particles (~60%) measured by Tracker. - Photons (~30%) by electromagnetic CAL (ECAL). - Neutral hadrons (~10%) by ECAL + hadron CAL (HCAL). E TOT = p e + p  + p charged hadron + E  + E neutral hadron [ tracks only] [calorimeter only] Particle Flow Algorithm (PFA)

6 5/30/2007LCWS07 @ DESY6 Jet Reconstruction @ ILC - Q. How to achieve the best attainable jet energy resolution? - A. Since the momentum resolution for the charged particle measured by trackers is much better than the energy resolution of calorimeters, the best energy resolution is obtained by reconstructing momenta of individual particles avoiding double counting among Trackers and Calorimeters. - Charged particles (~60%) measured by Tracker. - Photons (~30%) by electromagnetic CAL (ECAL). - Neutral hadrons (~10%) by ECAL + hadron CAL (HCAL). E TOT = p e + p  + p charged hadron + E  + E neutral hadron [ tracks only] [calorimeter only] Particle Flow Algorithm (PFA) Z → qq @ 91.2GeV The tracks are used instead of making a calorimetric measurement of the energies of the charged hadrons (with large errors).

7 5/30/2007LCWS07 @ DESY7 Detector Concepts SiD Particle Flow Algorithm (PFA) Compensation (Dual-Readout Calorimeter) LDCGLD 4th Three out of four are proposing a detector which is optimized for PFA, though the technical realization is quite different.

8 5/30/2007LCWS07 @ DESY8 e + e - → tt @ 500 GeV SiD LDC GLD 4th

9 5/30/2007LCWS07 @ DESY9 Particle Flow Algorithm - In order to get good energy resolution by PFA, separation of particles is important. → Reduce the density of charged and neutral particles at calorimeter surface. Often quoted “Figure of Merit” B : Magnetic field R : CAL inner radius σ: CAL granularity R M : Effective Moliere length - For transverse separation of particles at the ECAL surface, stronger B-field and/or large ECAL radius are preferable. * Fine segmentation of CAL is also important for pattern recognition. CAL surface

10 5/30/2007LCWS07 @ DESY10 Radius vs. B-field R = 140cm B = 5T R = 180cm B = 4T R = 210cm B = 3T B-field Radius To achieve the PFA performance goal with a reasonable detector cost.

11 5/30/2007LCWS07 @ DESY11 PFA Efforts in the World - Several PFAs have been intensively developed in the world so far; SiD - PFA for SiD (by N. Graf, S. Magill, L. Xia …) LDC - Pandora PFA (by M. Thomson) - Wolf PFA (by A. Raspereza) - Track-based PFA (by O. Wendt) GLD - GLD-PFA (by T. Yoshioka) and others … → While the algorithms are distinct, there are a number of features which are common. Details of each algorithm will be presented at on Saturday 02 June. - Cheated/Perfect PFA studies are also in progress.

12 5/30/2007LCWS07 @ DESY12 Cheated/Perfect PFA - e + e - → Z → qq @ 91.18GeV Use simulation information to connect track and calorimeter signals.  Cheated/Perfect PFA Understand factors which affect jet energy resolution - Signal sampling fluctuation in calorimeter. - Tracker resolution - Treatment of V0 decays and interaction before calorimeter. Ultimate performance by PFA.

13 5/30/2007LCWS07 @ DESY13 PFA for SiD Calorimeter Hits Calorimeter Clusters Clustering Algorithm Reconstructed Tracks Tracker Hits Track finding Algorithm

14 5/30/2007LCWS07 @ DESY14 PFA for SiD Calorimeter Hits Calorimeter Clusters Clustering Algorithm Photon Identification EM ClustersHadron Clusters Reconstructed Tracks Tracker Hits Track finding Algorithm

15 5/30/2007LCWS07 @ DESY15 PFA for SiD Calorimeter Hits Calorimeter Clusters Clustering Algorithm Photon Identification EM ClustersHadron Clusters ‘ Neutral ’ ClustersMatched Clusters Track-cluster matching E photon EM sampling fraction Reconstructed Tracks Tracker Hits Track finding Algorithm

16 5/30/2007LCWS07 @ DESY16 PFA for SiD Calorimeter Hits Calorimeter Clusters Clustering Algorithm Photon Identification EM ClustersHadron Clusters ‘ Neutral ’ ClustersMatched Clusters Track-cluster matching E photon EM sampling fraction Reconstructed Tracks Tracker Hits Track finding Algorithm 0P track E/p check

17 5/30/2007LCWS07 @ DESY17 PFA for SiD Calorimeter Hits Reconstructed TracksCalorimeter Clusters Clustering Algorithm Photon Identification EM ClustersHadron Clusters ‘ Neutral ’ ClustersMatched Clusters Track-cluster matching Charge fragment identification Neutral ClustersFragments E photon E neu-had 00P track Hadron sampling fraction EM sampling fraction Total event energy Tracker Hits Track finding Algorithm E/p check

18 5/30/2007LCWS07 @ DESY18 Next: 電子、陽電子衝突 e+e+ e-e- GLD-PFA Yellow : Photon Red, Green : Charged Hadron Black, Blue : Neutral Hadron Z → qqbar @ 91.2GeV

19 5/30/2007LCWS07 @ DESY19 Yellow : Photon Red, Green : Charged Hadron Black, Blue : Neutral Hadron GLD-PFA Photon Identification

20 5/30/2007LCWS07 @ DESY20 Yellow : Photon Red, Green : Charged Hadron Black, Blue : Neutral Hadron GLD-PFA Track-Cluster Matching

21 5/30/2007LCWS07 @ DESY21 Yellow : Photon Red, Green : Charged Hadron Black, Blue : Neutral Hadron GLD-PFA Fragment Identification

22 5/30/2007LCWS07 @ DESY22 Yellow : Photon Red, Green : Charged Hadron Black, Blue : Neutral Hadron GLD-PFA Remaining : Neutral Hadron

23 5/30/2007LCWS07 @ DESY23 - Almost no angular dependence : ~30%/ √ E for |cos  |<0.9. - cf. 60 %/ √ E w/o the PFA (sum up the calorimeter energy) All angle - Z → uds @ 91.2GeV, tile calorimeter, 1cm x 1cm tile size Jet Energy Resolution (GLD-PFA)

24 5/30/2007LCWS07 @ DESY24 Higher Energy Jets For high energy jets, the opening angles between particles decreases due to the large Lorenz Boost. This makes the separation of the clusters in the calorimeter more difficult. → How to resolve this? ILC goal of 30%/ √ E has been achieved w/ the current PFA at the Z-pole (E jet ~ 45GeV), but PFA becomes more challenging when considering higher energy jets. 45GeV250GeV

25 5/30/2007LCWS07 @ DESY25 Pandora PFA 10 GeV Track 30 GeV 12 GeV 18 GeV Change clustering parameters until cluster splits and get sensible track-cluster match - If track momentum and cluster energy inconsistent : RECLUSTER e.g. This is very important for higher energy jets. - In Pandora PFA, some special tools to take care high energy jets.

26 5/30/2007LCWS07 @ DESY26 Performance of Pandora PFA For jet energies < 100 GeV ILC goal reached !!! E JET  E /E = √(E/GeV) |cos|<0.7 45 GeV0.295 100 GeV0.305 180 GeV0.418 250 GeV0.534

27 5/30/2007LCWS07 @ DESY27 Performance of Pandora PFA For jet energies < 100 GeV ILC goal reached !!! E JET  E /E = √(E/GeV) |cos|<0.7 45 GeV0.295 100 GeV0.305 180 GeV0.418 250 GeV0.534 There are known flaws in the algorithm and the performance will become even better.

28 5/30/2007LCWS07 @ DESY28 Detector Optimization 100 GeV jets As expected, the resolution improves with increasing radius and increasing magnetic field. As expected, higher granularity gives better resolution. Previous studies of two particle separations gave similar conclusions. - Detector optimization study with the PFA has already started.

29 5/30/2007LCWS07 @ DESY29 Physics Study Of course, these are full Simulation results, not fast MC. Lots of physics studies are in progress with the current PFA performance. Results will come soon. ZH  bb GLD-PFA

30 5/30/2007LCWS07 @ DESY30 Summary The Particle Flow Algorithm (PFA) is widely believed that the most promising way to achieve a jet energy resolution of σ E /E ~ 30%/√E. We are now confident that PFA can give ILC performance goals for typical ILC jet energies, although there are still plenty of room for improvement. Detector optimization study/Physics study with the PFA are now intensively in progress. Simulation/Reconstruction parallel session on 31st May and 2nd June.

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