PPT-1 The Forward Silicon Vertex Detector Upgrade

Author : aaron | Published Date : 2019-03-16

for the PHENIX Experiment at RHIC Douglas Fields University of New Mexico Feb 12 2011 Douglas Fields WWND11 Feb 12th 2011 Douglas Fields WWND11 Feb 12th 2011 2

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1 The Forward Silicon Vertex Detector Upgrade: Transcript

for the PHENIX Experiment at RHIC Douglas Fields University of New Mexico Feb 12 2011 Douglas Fields WWND11 Feb 12th 2011 Douglas Fields WWND11 Feb 12th 2011 2 Quick PHENIX overview. Au+Au. collisions at √. s. NN. = 200 . GeV. in STAR experiment at RHIC. Jaiby Joseph Ajish. 11/9/2011. Outline. Introduction. Why collide nuclei at high energies?. RHIC and STAR. Physics at RHIC. Preshower. for the CMS: BARC Participation . Anita . Topkar. BARC. CMS Preshower Detector. End caps of . CMS detector has ~4300 . silicon . strip detectors covering . area . of~17 . m. 2 . . BARC . Detector. Markus Friedl (HEPHY Vienna) . for. . the. Belle II SVD Group. VCI, 13 . February. 2013. 13 February 2013. M.Friedl (Belle II SVD Group): The Belle II SVD. 2. Introduction. Front-End. Electronics. NN. = 200 GeV in STAR experiment at RHIC. Jaiby Joseph . Ajish. 11/2/2011. Outline. Quick summary of my contributions. Introduction. Why . collide nuclei at high energies?. RHIC, STAR. Physics at RHIC. Au+Au. collisions at √. s. NN. = 200 . GeV. in STAR experiment at RHIC. Jaiby Joseph Ajish. 11/9/2011. Outline. Introduction. Why collide nuclei at high energies?. RHIC and STAR. Physics at RHIC. IBL – . Insertable. B-Layer. Tobias Flick. University Wuppertal. 17.09.2009, VERTEX 2009 . Putten. , Netherlands. Preliminary. Overview. Current ATLAS pixel detector. What is the IBL and why do we need it?. NN. = 200 GeV in STAR experiment at RHIC. Jaiby Joseph . Ajish. 11/2/2011. Outline. Quick summary of my contributions. Introduction. Why . collide nuclei at high energies?. RHIC, STAR. Physics at RHIC. Hrvoje Štefančić. . Theoretical Physics Division . Ruđer Bošković Institute . (based on joint work with . Hrvoje Abraham . and . Predrag Lazić. ). Electric field strength in a segment of a Si microstrip detector. SuperKEKB. and Belle II Upgrades. Tom Browder. University of Hawaii . B Mesons: . “. Laboratory Rats of the Weak Interaction. ”. Exotic bound state of matter and antimatter. (hydrogen-like). b quark mass . Au Au. collisions at √. s. NN. = 200 . GeV. in STAR experiment at RHIC. Jaiby Joseph Ajish. 11/9/2011. Outline. Introduction. Why collide nuclei at high energies?. RHIC and STAR. Physics at RHIC. Yoshiyuki . Onuki. On behalf of . BelleII. /SVD collaboration. University of Tokyo/. Kavli. IPMU. 1. 2013/9/3. 9th International "Hiroshima" Symposium on the Development and Application of Semiconductor Tracking Detectors, Hiroshima, Japan. PARAMETERS. The . experimental apparatus includes two main detectors: a silicon vertex tracker (SVT) for . precise momentum vertex determination and . and an electromagnetic calorimeter (. ECal. ) to trigger on . , LNL, LNS, TIFPA. Neptune meeting – 19 June 2020. NEPTUNE. Nuclear process-driven Enhancement of Proton. Therapy . UNrav. . Eled. Outline. Goal. Measurements of microdosimetric spectra across the proton Bragg peak with detectors with tissue-equivalent (TE) walls/converters . . A. . Rachevski. 1. , . M. Ahangarianabhari. 2,5. , G. Aquilanti. 3. , P. Bellutti. 4,11. , G. Bertuccio. 2,5. , G. Borghi. 4,11. , J. Bufon. 3,1. , G. Cautero. 3,1. , S. Ciano. 1. , A. Cicuttin. 6,1.

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