CBM Experiment: Status and Plans of BHU Group CBM-INDIA SU, Srinagar JU, Jammu ØMore than 7 Universities PU, Chandigarh AMU, Aligarh RU, Jaipur BHU, Varanasi ØMore than 5 Institutes VECC, SINP, CU; Kolkata IIT, Kharagpur BARC, Mumbai IOP, Bhubaneswer ØWhy should we participate? ØHow should we participate? V. Singh Banaras Hindu University, Varanasi - 221 005 India 10 th CBM Collaboration meeting at Dresden, Germany – V. Singh
Why should we participate? BHU Group Prof. C. P. Singh (F) Dr. B. K. Singh (F) Dr. V. Singh (F) Mr. Mr. M. Mishra (R) S. Tarafdar (R) Arun K Soma (R) Saty Prakash (R) 3 Faculty Members (Few will join soon!) 4 Research students More than 6 masters students 10 th CBM Collaboration meeting at Dresden, Germany – V. Singh
Why should we participate? BHU Group Expertise: Prof. C. P. Singh (F) ►Vast experience in strong interaction phenomenology involving production mechanism for exotic exchange reactions, OZI rule violating processes, Current algebra, PCAC, Sum rules, Heavy flavour phenomenology, QCD, Nucleus-Nucleus Collisions and Quark-Gluon Plasma. Experience: ►He has been instrumental in keeping BHU on the international scene in HEP activities from last 35 years. 10 th CBM Collaboration meeting at Dresden, Germany – V. Singh
Phys. Lett. B (2007) Why should we participate? Highlight of few papers Ø Propose a new model which incorporates the excluded volume effect in a thermodynamically consistent manner. th 10 CBM Collaboration meeting at Dresden, Germany – V. Singh
Why should we participate? BHU Group Expertise: Dr. B. K. Singh (F) In Gaseous Detectors consisting of Cs. I photocathode and micro-pattern detectors (GEM, Micro-strip etc. ), Enough knowledge of scintillating crystal detectors. Unique experience in the design, development and engineering of Gaseous Photon detectors. Experience: Worked at Weizmann Institute Israel, INFN Italy, Columbia University USA and CERN Switzerland. 10 th CBM Collaboration meeting at Dresden, Germany – V. Singh
Why should we participate? • Triple GEM • Reflective Cs. I Photocathode Gaseous Photodetectors A. Breskin, A. Buzulutskov, R. Chechik, E. Shefer, B. K. Singh IEEE Trans. Nucl. Sc. 48 (2001) 417 Application: Hadron Blind Detector (PHENIX at Photodetectors Sealed Gaseous. RHIC) (Developed @ Weizmann Institute) D. Morrman, A. Breskin, R. Chechik and B. K. Singh Nucl. Instr. & Meth. A 478 (2002) 230 10 times cheaper than a GEM! 10 th CBM Collaboration meeting at Dresden, Germany – V. Singh
Why should we participate? Ageing of Cs. I thin film photocathodes induced by UV photons B. K. Singha, M. A. Nittib, , A. Valentinib, E. Nappib, C. Coluzzac, G. Di Santoc and R. Zanonid a. Department of Physics, Banaras Hindu University, Varanasi 221005, India b. INFN-Sezione di Bari, c/o Dipartimento Interateneo di Fisica “Michelangelo Merlin”, Via G. Amendola 173, 70126 Bari, Italy c. Dipartimento di Fisica “G. Marconi”, Università di Roma “La Sapienza”, P. le A. Moro 2, 00185 Rome, Italy d. Dipartimento di Chimica Generale e Inorganica, Università di Roma “La Sapienza”, P. le A. Moro 2, 00185 Rome, Italy , Received 30 May 2006; revised 17 July 2007; accepted 6 August 2007. Available online 15 August 2007 Abstract The degradation of Cs. I thin film photocathodes (PCs) under Ultraviolet (UV) irradiation has been investigated by measuring the photocurrent as well as the absolute Quantum Efficiency (QE) as a function of the accumulated charge density. Atomic Force Microscopy (AFM) and UV Photoemission Electron Microscopy (PEEM) have been employed to study the surface morphology and the local QE of polycrystalline Cs. I thin films and their transformation due to UV irradiation. The photo-emissive properties of Cs. I PCs, together with their surface morphology, have been found to be strongly affected by the UV photon ageing. 10 th CBM Collaboration meeting at Dresden, Germany – V. Singh
Why should we participate? Highlight of few papers Ødetailed study of GEM is still continuous ………………… 10 th CBM Collaboration meeting at Dresden, Germany – V. Singh
Why should we participate? BHU Group Dr. V. Singh (F) Expertise: Detector design & Development, Simulation, Logistic, Installation, Analysis, Testing and Calibration etc. Experience: Working in Collaboration, Run Coordinator, Setup of TEXONO (Taiwan EXperiment On Neutrin. O) Small scale but very effective ! 10 th CBM Collaboration meeting at Dresden, Germany – V. Singh
Why should we participate? Highlight of few papers Ø We derived world best limit on neutrino magnetic moments < 7. 4 X 10 -11 μB @ 90% CL. 10 th CBM Collaboration meeting at Dresden, Germany – V. Singh
Why should we participate? Our Achievements So far… (1)PAD Chamber, data analysis and simulation for PHENIX (2)All related hardware work, data analysis, simulation for TEXONO (3)Expertise in Development of advanced gaseous detector and organic/inorganic scintillating detectors etc. (4)Expertise in data analysis and simulation (5)Successful International and National Collaboration (Banaras, Chandigarh, Jaipur, Jammu, Lund); (Banaras, Kosice, Dubna, Lund, Tashkent); (PHENIX), (TEXONO) and (INO) (6)More than 20 students have got Ph. D. Future based on this strong base of experience and expertise 10 th CBM Collaboration meeting at Dresden, Germany – V. Singh
How should we participate? Our Proposal Based on our experience and expertise ! Aim is to take part SIGNIFICANTLY and at equal footing! ØWork with latest technology ØApplication of the expertise in detector development in other fields. ØDo R&D work related to detector (Mu. Ch) 10 th CBM Collaboration meeting at Dresden, Germany – V. Singh
How should we participate? Plans (Hardware): To establish a well equipped laboratory for GEM detector @ BHU. To do R&D for Muon Chamber detector. l l l To study the THGEM / GEM/Micromegas Long term stability vs Rate Understanding the effect of THGEM rim Gain and uniformity Ageing effects etc. Project approved. Waiting for money. Time frame: Few months! 10 th CBM Collaboration meeting at Dresden, Germany – V. Singh
How should we participate? Plans (Simulation): CBMRoot is already installed @ BHU. Getting feeling of program. To do detector (Much) and physics simulation for CBM. Time frame: within few months! 10 th CBM Collaboration meeting at Dresden, Germany – V. Singh
How should we participate? Plans (Data analysis): Physics Topics 1. In-medium modifications of hadrons onset of chiral symmetry restoration at high B Observables: , , e+eopen charm production 2. Strangeness in matter (strange matter) enhanced strangeness production; Observables: K, , 3. Indications for deconfinement at high B anomalous charmonium suppression? Observables: J/ , D excitation function of flow (softening of EOS) 4. Critical point: Observables: event-by-event fluctuations 10 th CBM Collaboration meeting at Dresden, Germany – V. Singh
How should we participate? Motivation-e+e- pair 10 th CBM Collaboration meeting at Dresden, Germany – V. Singh
Thank you ! Conclusion & Summary: ☻Why should we participate? Motivation, Experienced, Expertise, Hardworking and Strength. ☻How should we participate? Latest technology, all possible areas, significantly and at equal footing! We are about to start work for CBM ! 10 th CBM Collaboration meeting at Dresden, Germany – V. Singh
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