PPT-Structural option for the Jinping neutrino central detector

Contributor Yuanqing Wang Zongyi Wang Speaker Z ongyi Wang Department of civil engineering Tsinghua University 20150605 1 Outline Introduction of the whole structure . Naba. K . Mondal. Tata Institute of Fundamental Research. Mumbai 400005, India. Brief History. Atmospheric neutrino experiments study neutrinos produced by cosmic ray interactions in the atmosphere.. Shun Zhou. IHEP, CAS, Beijing. on . behalf of the JUNO Collaboration. The 8. th. Workshop of France-China Particle Physics Laboratory. USTC, Hefei, April 8 - 10, 2015. T. he JUNO Experiment. 20 . kton. (INO) . Naba. K . Mondal. , . TIFR, Mumbai. . ICAL . ( conceptual). INO Peak at. Bodi. West Hills. Prototype ICAL at VECC. 2mX2m RPC Test Stand at TIFR. ASIC for RPC designed at BARC. RPC Test stand at TIFR. 1. John Beacom, The Ohio State University. 2. Plan of the Talk. Introduction to Supernova . N. eutrinos. Focus on . B. urst . D. etection. . What will we know after the next burst?. What . new capabilities do we need?. . . Neutrinos Are Very Elusive!. We now understand that neutrinos are produced in nuclear reactions, but they were actually . predicted several decades before they were finally discovered. . O. n what basis was that prediction made?. its calibration . strategy. Mengjiao Xiao. University of Maryland, College Park. (On behalf of the JUNO collaboration). 2016-11-03. NNN’16, November . 3-5, 2016, IHEP, . Beijing · China. Outline. Introduction to JUNO experiment. PPAP Meeting. Birmingham. 15 July 2009. Elisabeth Falk. University of Sussex. Def. current: running or under construction. Outline. Neutrino-oscillation experiments:. what to measure, and how. Accelerator-based experiments. Fabrice . Piquemal. Laboratoire Souterrain de Modane (CNRS/IN2P3-CEA/DSM) . and CENBG. , . University. Bordeaux 1 . CNRS/IN2P3. Thanks. to: G. Gratta, S. ., . A. . Giuliani. , S. . Schoenert. , . T. . Neutrino Oscillations in Susan Cartwright Neutrino Oscillations Principles Experimental techniques Neutrino oscillations: Principles The Standard Model contains three neutrinos These can be labelled by flavour as Jun Cao. . Institute of High Energy Physics. ICHEP, Melbourne, July 11, . 2012. Neutrino Mixing. . 23. ~ 45. Atmospheric Accelerator. . 1. 2. ~ 34. Solar. Reactor. 0. . 1. 3. PPAP Meeting. Birmingham. 15 July 2009. Elisabeth Falk. University of Sussex. Def. current: running or under construction. Outline. Neutrino-oscillation experiments:. what to measure, and how. Accelerator-based experiments. Contributor. ：. . Yuanqing. Wang. , . Zongyi. Wang. Speaker. ： . Z. ongyi. Wang. Department of civil engineering, Tsinghua University . 2015-06-05. 1. Outline. Introduction of the whole structure . 1Politicsand Foreign Policy after the 19th Party CongressPaper presented toJapanese Views on China and Taiwan Implications for US-Japan AllianceMarch 1 2018Center for Strategic International StudiesW IceCube. Justin Vandenbroucke, June 9, 2021. IceCube. Bootcamp, WIPAC, UW–Madison. Outline. Neutrino interactions and cross sections. Muon lifetime. Charged particles losing energy in matter. Ionization.