Fast-time Variations of Supernova Neutrino Fluxes and Detection Perspectives

Open Access
Authors
  • G.G. Raffelt
Publication date 2015
Journal Physics Procedia
Event TAUP 2013 - Asilomar
Volume | Issue number 61
Pages (from-to) 359-365
Organisations
  • Faculty of Science (FNWI) - Institute of Physics (IoP) - Institute for Theoretical Physics Amsterdam (ITFA)
Abstract In the delayed explosion scenario of a core-collapse supernova, the accretion phase shows pronounced convective over-turns and a low-multipole hydrodynamic instability, the so-called standing accretion shock instability (SASI). Neutrino signal variations from the first full-scale three-dimensional core-collapse supernova simulations with sophisticated neutrino transport are presented as well as their detection perspectives in IceCube and Hyper-Kamiokande.
Document type Article
Note Proceedings title: Proceedings of 13th Internationa Conference on Topics in Astroparticle and Underground Physics: Asilomar, California USA Publisher: Elsevier Place of publication: Amsterdam Editors: W. Haxton, F. Avignone
Language English
Published at https://doi.org/10.1016/j.phpro.2014.12.076
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