Multidimensional, multiphysics simulations of core-collapse supernovae

被引：9

作者：

Messer, O. E. B. ^{[1
]}

Bruenn, S. W. ^{[2
]}

Blondin, J. M. ^{[3
]}

Hix, W. R. ^{[4
]}

Mezzacappa, A. ^{[4
]}

机构：

[1] Oak Ridge Natl Lab, Natl Ctr Computat Sci, Oak Ridge, TN 37831 USA

[2] Florida Atlantic Univ, Dept Phys, Boca Raton, FL 33431 USA

[3] N Carolina State Univ, Dept Phys, Raleigh, NC 27695 USA

[4] Oak Ridge Natl Lab, Div Phys, Oak Ridge, TN 37831 USA

来源：

SCIDAC 2008: SCIENTIFIC DISCOVERY THROUGH ADVANCED COMPUTING | 2008年 / 125卷

基金：

美国国家科学基金会;

关键词：

D O I：

10.1088/1742-6596/125/1/012010

中图分类号：

TP301 [理论、方法];

学科分类号：

081202 ;

摘要：

CHIMERA is a multi-dimensional radiation hydrodynamics code designed to study core-collapse supernovae. The code is made up of three essentially independent parts: a hydrodynamics module, a nuclear burning module, and a neutrino transport solver combined within an operator-split approach. We review the code's architecture and some recently improved implementations used in the code. We also briefly discuss preliminary results obtained with the code in three spatial dimensions.

引用

页数：10

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