Supernova Neutrinos and Their Implications for Neutrino Parameters

Details Supernova Neutrinos and Their Implications for Neutrino Parameters Supernova Neutrinos and Their Implications for Neutrino Parameters

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003cpa..conf..228s&link_type=abstract

PROCEEDINGS OF THE 2002 INTERNATIONAL SYMPOSIUM ON COSMOLOGY AND PARTICLE ASTROPHYSICS (CosPA 02). Held 31 May ?2 June 2002 in T

Astronomy and Astrophysics

Astrophysics

Scientific paper

Core-collapse driven supernovae are the most luminous neutrino source in the universe. If neutrinos have finite masses and convert each other, the time profile and energy spectrum of the neutrino burst from supernovae are greatly modified. We review the neutrino conversion in a supernova mantle, and how the burst will be detected by SK (Super-Kamiokande) and SNO (Sudbury Neutrino Observatory) if a supernova appear at Galactic Center. We show that various neutrino oscillation models can be discriminated by the combination of the SK and SNO detections of a future galactic Supernova. We also discuss effects of neutrino oscillation on the supernova relic neutrino observations.

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