SCALING OF MAGNETO-QUANTUM-RADIATIVE HYDRODYNAMIC EQUATIONS: FROM LASER-PRODUCED PLASMAS TO ASTROPHYSICS
SCALING OF MAGNETO-QUANTUM-RADIATIVE HYDRODYNAMIC EQUATIONS: FROM LASER-PRODUCED PLASMAS TO ASTROPHYSICS
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DOI：
10.1088/0004-637x/795/1/59
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发表时间：
2014-11-01
影响因子：
4.9
通讯作者：
Gregori, G.
中科院分区：
文献类型：
--
作者：
Cross, J. E.;Reville, B.;Gregori, G.
介绍了磁量子辐射流体力学方程。通过将它们重写为无量纲形式，我们获得了一组描述特征流体动力量的尺度相关比率的参数。我们讨论了这些无量纲参数与天体物理观测和实验室实验之间的比例关系。
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.