Supernova Modeling: Progress and Challenges

Christian Y. Cardall

doi:10.1016/j.nuclphysbps.2012.09.049

Supernova Modeling: Progress and Challenges

Christian Y. Cardall

Theoretical and Computational Physics

Research output: Contribution to journal › Article › peer-review

3 Scopus citations

Abstract

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.

Original language	English
Pages (from-to)	315-319
Number of pages	5
Journal	Nuclear Physics B - Proceedings Supplements
Volume	229-232
DOIs	https://doi.org/10.1016/j.nuclphysbps.2012.09.049
State	Published - Aug 2012

Funding

Support from the Office of Nuclear Physics, DOE, and the Office of Advanced Scientic Computing Research, DOE, is gratefully acknowledged. Oak Ridge National Laboratory is managed by UT-Battelle for the DOE.

Keywords

Core-collapse supernovae
Supernova neutrinos

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10.1016/j.nuclphysbps.2012.09.049

Cite this

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abstract = "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.",

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AB - 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.

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Supernova Modeling: Progress and Challenges

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Keywords

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