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27 September, 2006Gakujyutsu Sousei Monthly Meeting1 The Detector Chapter of The Detector Concept Report 学術創成定例月会議 9月27日 宮本彰也 8 月 7 日の報告も見てください

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Presentation on theme: "27 September, 2006Gakujyutsu Sousei Monthly Meeting1 The Detector Chapter of The Detector Concept Report 学術創成定例月会議 9月27日 宮本彰也 8 月 7 日の報告も見てください"— Presentation transcript:

1 27 September, 2006Gakujyutsu Sousei Monthly Meeting1 The Detector Chapter of The Detector Concept Report 学術創成定例月会議 9月27日 宮本彰也 8 月 7 日の報告も見てください http://agenda.kek.jp/fullAgenda.php?ida=a06157 Very primitive & selected summary of on-going preparation Your comments/inputs are highly welcomed

2 27 September, 2006 Gakujyutsu Sousei Monthly Meeting 2 The RDR and DCR DCR is associated with the RDR: Due end of 2006 Detector Concept Report consists of  Physics section : ~50 Pages – Editors: Klaus Moening, Yasuhiro Okada, Joe Lykken, Mark Oreglia, Satoru Yamashita, Adbelhak Djouadi – Wiki page: http://www.linearcollider.org/wiki/http://www.linearcollider.org/wiki/  Detector section: ~150 pages – Editors: Ties Behnke, C.J.S.Damerell, John Jaros, A.M. – Based on detector DOD's and input from experts DCR is for Non-ILC HEP researchers/beginners Executive summary  Executive summaries of RDR+DCR physics + DCR detector  Executive Summary with a help of communication experts

3 27 September, 2006 Gakujyutsu Sousei Monthly Meeting 3 The Outline of the Detector Chapter 1.General Introduction 2.Challenges for Detector Design and Technology 3.Introduction to the Detector Concepts 4.MDI Issues 5.Subsystem Designs and Technologies 6.Sub-Detector Performance 7.Integrated Physics Performance 8.Why We need 2IRs and 2 Detectors 9.Detector Costs 10.Future Options 11.Next Step 12.Conclusion  Experts : T.Takahashi + ?? + ??  John Jaros + Experts  Concept teams  Ties Behnke + MDI experts  C.Damerell + R&D panels  A.Miyamoto + Concept Rep.  open  2IR panels  Costing panels  WWS OC

4 27 September, 2006 Gakujyutsu Sousei Monthly Meeting 4 Challenge for Detector Design and Technology Editors (John Jaros) + Tim Barklow + Henri Videau + Keisuke Fujii Outlines  Jet energy resolution: Required lum. vs resolution. –  ( WW/ZZ), Br(H  WW*),  (HHZ), SUSY(WW/ZZ)  Momentum resolution: – Recoil mass of ZH  llX, Slepton Mass, Lum weighted ECM det. from  pair and   Vertexing at ILC – Br(H  bb), Br(H  cc,gg), AFB(bb) with vertex charge – Challenges imposed by the ILC beam structure  Beamcal – High rad. Env., reacdout each bunch, need to veto H.E. e at the smallest possible angle – S(SUSY) vs veto efficiency, electron angle,..  Others – Ebeam, Pol., High B Solenoid., Muons, required R&D

5 27 September, 2006 Gakujyutsu Sousei Monthly Meeting 5 Subsystem designs and technologies Prepared by R&D panel members and experts Authors assigned  Beam CAL : Ray Frey  Vertex detector : C. Damerell  Tracker – TPC : Dean Carlen - Silicon:  Calorimeter: Wolfgang  Solenoid : Akira Yamamoto  DAQ: Ecklund Correcting outlines on each topics

6 27 September, 2006 Gakujyutsu Sousei Monthly Meeting 6 Sub-Detector Performance Philosophy  Pickup typical results from concept studies in order to show that detector performance used in the physics chapter is confirmed with some extent by full simulations. Basics  Material budget of detectors Tracker performacne  Momentum resolution: TPC (GLD, LDC, 4 th ), SiD  Track reconstruction – TPC: Old Tesla TDR result – SiD: VTX based, ECAL Based + SiD standalone

7 27 September, 2006 Gakujyutsu Sousei Monthly Meeting 7 Comparison of Momentum Resolution LDC GLD GLD vs LDC Difference in Low Pt region ? Is it by IT matterial ? High Pt: TPC only resol. Different. Spatial resolution difference ? With VTX/IT Constraint, similar performance. No CosTheta dep. From GLD. SiD

8 27 September, 2006 Gakujyutsu Sousei Monthly Meeting 8 Track Reconstruction LDC ( Tesla TDR ) SiD SiD promissed better pictures By the end of Oct.

9 27 September, 2006 Gakujyutsu Sousei Monthly Meeting 9 Calorimeter and PFA Performance Calorimeter performance for single particle   /electron energy resolution & angular resolution  Pi+/Kaon_L energy resolution & angular resolution PFA issues  Describe what is PFA  Typical PFA algorithm(s)  Typical PFA performance at Z pole and higher energy – Resolution : 90% RMS – SiD result ? – LDC – 30%/sqrt(E) at Z pole, but not good for ttbar, 500GeV – GLD – 30%/sqrt(E) at Z pole, barrel region + Not good in endcap region  Hope to improve soon + Still tile geometry.  Strip geometry ? + High Energy performance not good.  Hope : good for baseline physics

10 27 September, 2006 Gakujyutsu Sousei Monthly Meeting 10 Typical PFA result GLD PFA

11 27 September, 2006 Gakujyutsu Sousei Monthly Meeting 11 PFA – cont. Particle ID's in jets (PFA)  Good PFA includes efficient and pure ID of , e,   Typical particle ID efficiency/purity shall (should ) be described.  What studies should be described and How ?

12 27 September, 2006 Gakujyutsu Sousei Monthly Meeting 12 Vertexing Performance Impact parameter resolution: 2D or 3D  SiD, GLD, LDC (wil) have simular performance Efficiency and purity of b/c tagging and vertex charge ID.  Mostly based on fast simulation.  How to describe ?

13 27 September, 2006 Gakujyutsu Sousei Monthly Meeting 13 Impact Parameter resolution + LDC ~1.5  m at 100 GeV ~13  m at 1 GeV I SiD promissed similar plot by the end of Oct. Need a plot of cos  dependance.

14 27 September, 2006 Gakujyutsu Sousei Monthly Meeting 14 Muon ID Pt threshould to be identified by muon detector How highly-segmented calorimeter is effective to identify low momentum muon particles ? GLD case Calorimeter based muon ID will be useful

15 27 September, 2006 Gakujyutsu Sousei Monthly Meeting 15 Beam Calorimeter Describe typical electron tagging efficiency Dependance on  Beam parameters  Crossing anlge

16 27 September, 2006 Gakujyutsu Sousei Monthly Meeting 16 Time line to prepare the detector chapter Time line:  At Vancouver: – Propose the outline – Authors are nominated/selected  By End of September – First draft including major part of figures collected. – Some figures will be preliminary  By End of October=ECFA meeting at Valencia – Combine drafts, make a balance, editing, draft open to society  By End of November – Get feedback from community  By end of 2006: – Shape up and complete DCR  Slower than the initial plan


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