2005/08/05 by Francesco Vissani, Vissani, Francesco, Maria Laura Costantini +1
Engineering · Physics and Astronomy · #Astrophysics (astro-ph) #Astrophysics and Cosmic Phenomena #FOS: Physical sciences #Neutrino Physics Research #Particle accelerators and beam dynamics #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0508152
5 pages, 3 figures, to appear in the proceedings of IFAE, Catania 2005
arxiv created 2005/08/05 · openalex publication_date 2005/08/05 · arxiv updated 2011/02/19 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
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 SNR (in particular from RX J1713.7-3946) targets of future underwater neutrino telescopes.