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.2011.04.118

Additional 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.