P99+2011+Talk

P99 2011 Talk - Neutrino Physics Super-Kamiokande Experimental Particle Physics Group Sobel Hank Sobel Michael Smy Mark Vagins Bill Kropp Shunichi

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Neutrino Physics: Super-Kamiokande
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Experimental Particle Physics Group - Sobel Hank Sobel Michael Smy Mark Vagins Bill Kropp Shunichi Mine Chris Regis Kirk Bays Andrew Renshaw Ben Ziemer Clifford Simon Jeff Griskevich - Engineer Jed Rogge – Computer Systems Graduate Students Supported at UCI by DOE grant Miner ν a Experiment at Fermilab
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Super-Kamiokande Collaboration ~130 authors from 35 institutions Japan, U.S., China, Korea, Poland, France, Canada
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Current Science Objectives • Neutrino Physics – Solve neutrino mass hierarchy problem. – Determine δ CP Matter – Antimatter in universe – Detect vacuum transition in Solar Neutrinos – Detect the relic neutrino flux from the sum of all supernovae out to cosmologically significant distances. – Be ready for a galactic supernova. • Nucleon Decay Grand Unification – Expand the sensitivity for nucleon decay modes by as much as a factor of ten.
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50,000 ton n 1000 m underground
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This note was uploaded on 12/12/2011 for the course PHYS 99 taught by Professor Dennin,m during the Fall '08 term at UC Irvine.

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P99 2011 Talk - Neutrino Physics Super-Kamiokande Experimental Particle Physics Group Sobel Hank Sobel Michael Smy Mark Vagins Bill Kropp Shunichi

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