Neutrinos from Supernovas and Supernova Remnants

Details Neutrinos from Supernovas and Supernova Remnants Neutrinos from Supernovas and Supernova Remnants

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..794..219c&link_type=abstract

IFAE 2005: XVII Incontri de Fisica delle Alte Energie; 17th Italian Meeting on High Energy Physics. AIP Conference Proceedings,

Physics

High Energy Physics

1

Neutrino Interactions, Supernovae, Supernova Remnants, Neutrino Mass And Mixing

Scientific paper

Supernovae (SN) and supernova remnants (SNR) have key roles in galaxies, but their physical descriptions is still incomplete. Thus, it is of interest to study neutrino radiation to understand SN and SNR better. We will discuss: (1) The ~10 MeV thermal neutrinos that arise from core collapse SN, that were observed for SN1987A, and can be seen with several existing or planned experiments. (2) The 10-100 TeV neutrinos expected from galactic SNRs (in particular from RX J1713.7-3946) targets of future underwater neutrino telescopes.

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