Huang s 117_final
Supernovae High Energy Astrophysics [email protected]
Search for 13 at Daya Bay On behalf of the Daya Bay Collaboration Deb Mohapatra Virginia Tech.
Gravitational Wave Astronomy
IRFU 2 December 2008CARE'08, CERN1 CARE D ISSEMINATION A CTIVITIES O. Napoly (CEA/Saclay) Chair of CARE Dissemination Board.
Cherenkov Detectors. Index of Refraction When light passes through matter its velocity decreases. –Index of refraction n. The index depends on the medium.
Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.
Astronomy 1020-H Stellar Astronomy Spring_2015 Day-29.
Advantage: Neutrinos 2. Neutrino scattering Super Kamiokande located 1000m underground in Kamioka mine in Japan is a water Cherenkov detector made up of.
27 November 20151 Light Radio-isotopes Nuclear Astrophysics, Neutrino Physics and Fundamental Interactions O. Aviv 1, D. Berkovits 2, M. Hass 1, O. Heber.
Announcements Turn in Homework 5, pick up Homework 6. Another test this week! Same days (W,Th), same format as before. First project due October 13.
Alain Blondel CHIPP Neutrino meeting NEUCHATEL 21-22 June 2004.
