SCALING OF MAGNETO-QUANTUM-RADIATIVE HYDRODYNAMIC EQUATIONS: FROM LASER-PRODUCED PLASMAS TO ASTROPHYSICS

被引：34
作者：
Cross, J. E. [1 ]
Reville, B. [2 ]
Gregori, G. [1 ]
机构：
[1] Univ Oxford, Clarendon Lab, Oxford OX1 3PU, England
[2] Queens Univ Belfast, Ctr Plasma Phys, Belfast BT7 1NN, Antrim, North Ireland
来源：
ASTROPHYSICAL JOURNAL | 2014年 / 795卷 / 01期
基金：
欧洲研究理事会;
关键词：
hydrodynamics; ISM: jets and outflows; magnetohydrodynamics (MHD); plasmas; radiative transfer; supernovae: general; SHOCK-WAVES; LABORATORY SIMULATIONS; SUPERNOVA-REMNANTS; FIELDS; GENERATION; SCATTERING; CRITERIA; MATTER; FLOWS; LAWS;
D O I：
10.1088/0004-637X/795/1/59
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We introduce the equations of magneto-quantum-radiative hydrodynamics. By rewriting them in a dimensionless form, we obtain a set of parameters that describe scale-dependent ratios of characteristic hydrodynamic quantities. We discuss how these dimensionless parameters relate to the scaling between astrophysical observations and laboratory experiments.
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页数：10
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