Fast-time Variations of Supernova Neutrino Fluxes and Detection Perspectives
| Authors |
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|---|---|
| Publication date | 2015 |
| Journal | Physics Procedia |
| Event | TAUP 2013 - Asilomar |
| Volume | Issue number | 61 |
| Pages (from-to) | 359-365 |
| Organisations |
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| 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
(Final published version)
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Fast-time Variations of Supernova Neutrino Fluxes
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