Fast Lattice Boltzmann Solver for Relativistic Hydrodynamics

被引：95

作者：

Mendoza, M. ^{[1
]}

Boghosian, B. M. ^{[2
]}

Herrmann, H. J. ^{[1
]}

Succi, S. ^{[3
,4
]}

机构：

[1] ETH, Inst Bldg Mat, HIF, CH-8093 Zurich, Switzerland

[2] Tufts Univ, Dept Math, Medford, MA 02155 USA

[3] CNR, Ist Applicazioni Calcolo, I-00185 Rome, Italy

[4] Freiburg Inst Adv Studies, D-79104 Freiburg, Germany

来源：

PHYSICAL REVIEW LETTERS | 2010年 / 105卷 / 01期

基金：

美国国家科学基金会;

关键词：

D O I：

10.1103/PhysRevLett.105.014502

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

A lattice Boltzmann formulation for relativistic fluids is presented and numerically validated through quantitative comparison with recent hydrodynamic simulations of relativistic fluids. In order to illustrate its capability to handle complex geometries, the scheme is also applied to the case of a three-dimensional relativistic shock wave, generated by a supernova explosion, impacting on a massive interstellar cloud. This formulation opens up the possibility of exporting the proven advantages of lattice Boltzmann methods, namely, computational efficiency and easy handling of complex geometries, to the context of (mildly) relativistic fluid dynamics at large, from quark-gluon plasmas up to supernovae with relativistic outflows.

引用

页数：4

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