Simulation for CMS HI Dipanwita Dutta Nuclear Physics

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Simulation for CMS HI Dipanwita Dutta Nuclear Physics Division Bhabha Atomic Research centre Mumbai,

Simulation for CMS HI Dipanwita Dutta Nuclear Physics Division Bhabha Atomic Research centre Mumbai, India Dipanwita Dutta 5 -6 April, 2007, India-CMS Meet, Chandigarh

Outline Part I • Cross-section of Z 0 (PYTHIA) • Simulation and Reconstruction of

Outline Part I • Cross-section of Z 0 (PYTHIA) • Simulation and Reconstruction of Z 0 with CMKIN+OSCAR+ORCA • Muon Reconstruction with CMSSW Part II • Future Plan: Simulation for Small mass dimuon / Real Photon with CMS Dipanwita Dutta 5 -6 April, 2007, India-CMS Meet, Chandigarh

Part I Simulation for Z 0 Dipanwita Dutta 5 -6 April, 2007, India-CMS Meet,

Part I Simulation for Z 0 Dipanwita Dutta 5 -6 April, 2007, India-CMS Meet, Chandigarh

Cross-Section of Z 0 (PYTHIA) pp(Z 0) (nb/Ge. V) Total For Pb-Pb minbias collision

Cross-Section of Z 0 (PYTHIA) pp(Z 0) (nb/Ge. V) Total For Pb-Pb minbias collision at 5. 5 Te. V (Z 0 + -) B A 2 pp(Z 0) Z 0 p. T (Ge. V) Dipanwita Dutta 68 b 5 -6 April, 2007, India-CMS Meet, Chandigarh

Cross-section and No. of Z 0 for Pb+Pb collision s=5. 5 Te. V for

Cross-section and No. of Z 0 for Pb+Pb collision s=5. 5 Te. V for Lint=0. 5 nb-1 Cross-section from PYTHIA pp (Z 0) PDF CTEQ 5 ML No. of Z 0 for central collision (CTEQ 5 M) AA=TAA(0) NN pp (Z 0) No. of Z 0 for minbias collision AA=A 2 pp (Z 0) Z 0, Z 0+jet 48 nb 54 nb 4. 3 104 1. 03 106 Z 0 16 nb 17. 5 nb 1. 4 104 3. 4 105 Z 0, Z 0+jet 8. 9 10 -1 nb 9. 5 10 -1 nb 800 1. 9 104 m. Z-5<M < m. Z+5 6. 9 10 -1 nb 7. 7 10 -1 nb 621 1. 4 104 Z 0 2. 8 10 -1 nb 257 6020 Processes For CMS p. T>3. 5 Ge. V <2. 4 Dipanwita Dutta 5 -6 April, 2007, India-CMS Meet, Chandigarh

Differential and Integrated Rate of Z 0 in Pb+Pb collision , s=5. 5 Te.

Differential and Integrated Rate of Z 0 in Pb+Pb collision , s=5. 5 Te. V for Lint=0. 5 nb-1 │ Barrel+Endcap Barrel only Dipanwita Dutta 5 -6 April, 2007, India-CMS Meet, Chandigarh

Muon Reconstruction ● • Tag from Muon chambers • Momentum resolution from Silicon Tracker

Muon Reconstruction ● • Tag from Muon chambers • Momentum resolution from Silicon Tracker • Local Muon Reconstruction (L 1) • Stand-Alone Muon Reconstruction (L 2) • Global Muon Reconstruction (L 3) (Combined with Tracker) Dipanwita Dutta 5 -6 April, 2007, India-CMS Meet, Chandigarh

Simulation of Z 0 + - channel Gen. vs. Rec. Muon from ORCA Dipanwita

Simulation of Z 0 + - channel Gen. vs. Rec. Muon from ORCA Dipanwita Dutta Gen Rec p. T (Ge. V) 5 -6 April, 2007, India-CMS Meet, Chandigarh

Gen. – Rec. Muon p. T, Dipanwita Dutta 5 -6 April, 2007, India-CMS Meet,

Gen. – Rec. Muon p. T, Dipanwita Dutta 5 -6 April, 2007, India-CMS Meet, Chandigarh

Reconstruction without background Stand Alone Muon Reconstruction Dipanwita Dutta 5 -6 April, 2007, India-CMS

Reconstruction without background Stand Alone Muon Reconstruction Dipanwita Dutta 5 -6 April, 2007, India-CMS Meet, Chandigarh

Reconstruction with HI Background Stand Alone Muon Reconstruction Dipanwita Dutta 5 -6 April, 2007,

Reconstruction with HI Background Stand Alone Muon Reconstruction Dipanwita Dutta 5 -6 April, 2007, India-CMS Meet, Chandigarh

Summary : CMKIN-OSCAR-ORCA • Generation, Simulation and Reconstruction of Z 0 performed with HI

Summary : CMKIN-OSCAR-ORCA • Generation, Simulation and Reconstruction of Z 0 performed with HI background using full CMS simulation package CMKIN, OSCAR, ORCA • Stand Alone Muon Reconstruction show poor mass resolution, Mass width~ 18 Ge. V at Z 0 mass ( m/m~0. 2) • Mass Resolution remains unaltered with HI background using Stand Alone Muon Reconstruction • Global Muon Reconstruction with Tracker: Mass Resolution with HI background to be studied --- No further Support for ORCA Dipanwita Dutta 5 -6 April, 2007, India-CMS Meet, Chandigarh

Reconstruction with CMSSW • CMSSW_1_2_2 downloaded and installed locally at BARC • Muon Reconstruction

Reconstruction with CMSSW • CMSSW_1_2_2 downloaded and installed locally at BARC • Muon Reconstruction using CMSSW: Software available for pp, Reconstruction algorithms for HI under development • Involvement of BARC for HI Software transportation to CMSSW is required --Olga • Reconstruction using pp algorithm: Z 0 Generation with PYTHIA using CMSSW Generator Interface -- Simulation+ Digitization--Local + Stand Alone Muon Reconstruction Dipanwita Dutta 5 -6 April, 2007, India-CMS Meet, Chandigarh

Muon Reconstruction with CMSSW PT distribution of Generated and Reconstructed muons Dipanwita Dutta 5

Muon Reconstruction with CMSSW PT distribution of Generated and Reconstructed muons Dipanwita Dutta 5 -6 April, 2007, India-CMS Meet, Chandigarh

Reconstructed-Generated PT Difference Dipanwita Dutta 5 -6 April, 2007, India-CMS Meet, Chandigarh

Reconstructed-Generated PT Difference Dipanwita Dutta 5 -6 April, 2007, India-CMS Meet, Chandigarh

Generated and Reconstructed Invariant Mass m ~ 14 Ge. V Dipanwita Dutta 5 -6

Generated and Reconstructed Invariant Mass m ~ 14 Ge. V Dipanwita Dutta 5 -6 April, 2007, India-CMS Meet, Chandigarh

Part II Real Photon/ Small mass Dilepton Dipanwita Dutta 5 -6 April, 2007, India-CMS

Part II Real Photon/ Small mass Dilepton Dipanwita Dutta 5 -6 April, 2007, India-CMS Meet, Chandigarh

Dipanwita Dutta 5 -6 April, 2007, India-CMS Meet, Chandigarh

Dipanwita Dutta 5 -6 April, 2007, India-CMS Meet, Chandigarh

Dipanwita Dutta 5 -6 April, 2007, India-CMS Meet, Chandigarh

Dipanwita Dutta 5 -6 April, 2007, India-CMS Meet, Chandigarh

Direct Photons at Low p. T – RHIC Result QM 2005: Data consistent with

Direct Photons at Low p. T – RHIC Result QM 2005: Data consistent with thermal+ NLO p. QCD uncertain at low p. T Gordon and Vogelsang Phys. Rev. D 48, 3136 (1993) Thermal d’Enterria, Perresounko Eur. Phys. J. C 46: 451 -464, 2006 (a) New experimental method for the measurement of Dipanwita Dutta 5 -6 April, 2007, India-CMS Meet, Chandigarh

Future Plan • Involvement in transportation as well as improvement of reconstruction HI softwares

Future Plan • Involvement in transportation as well as improvement of reconstruction HI softwares from OSCAR, ORCA to CMSSW • Global Muon Reconstruction with Tracker information included in CMSSW for Z 0 + • Simulation for low mass Dimuon/Photon channel-Background muons – (DY and open charm and bottom) • Study the Thermal Dilepton signal (theoretical prediction) and possibility to see the effect of Chemical unsaturation Dipanwita Dutta 5 -6 April, 2007, India-CMS Meet, Chandigarh

Dipanwita Dutta 5 -6 April, 2007, India-CMS Meet, Chandigarh

Dipanwita Dutta 5 -6 April, 2007, India-CMS Meet, Chandigarh