Published August 2011
| Version v1
Journal article
Core-collapse supernova explosion simulations
Creators
- 1. Physics Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831-6354 (United States)
Description
Neutrinos play important roles in the pre-collapse evolution, explosion, and aftermath of core-collapse supernovae. Detected neutrino signals from core-collapse supernovae would provide insight into the explosion mechanism and unknown neutrino mixing parameters. Achieving these goals requires large-scale, multiphysics simulations. For many years, several groups have performed such simulations with increasing realism. Current simulations and plans for future work of the Oak Ridge group are described.
Availability note (English)
Available from http://dx.doi.org/10.1016/j.nuclphysbps.2011.04.118Additional details
Identifiers
- DOI
- 10.1016/j.nuclphysbps.2011.04.118;
- PII
- S0920-5632(11)00357-4;
Publishing Information
- Journal Title
- Nuclear Physics. B, Proceedings Supplements
- Journal Volume
- 217
- Journal Issue
- 1
- Journal Page Range
- p. 275-277
- ISSN
- 0920-5632
- CODEN
- NPBSE7
Conference
- Title
- Neutrino Oscillation Workshop
- Acronym
- NOW 2010
- Dates
- 5-11 Sep 2010
- Place
- Otranto (Italy)
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 43070014
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- COMPUTERIZED SIMULATION; COSMIC NEUTRINOS; EXPLOSIONS; STAR EVOLUTION; SUPERNOVAE
- Descriptors DEC
- BINARY STARS; COSMIC RADIATION; ELEMENTARY PARTICLES; ERUPTIVE VARIABLE STARS; EVOLUTION; FERMIONS; IONIZING RADIATIONS; LEPTONS; MASSLESS PARTICLES; NEUTRINOS; RADIATIONS; SIMULATION; STARS; VARIABLE STARS
Optional Information
- Copyright
- Copyright (c) 2011 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.