Scaling of magneto-quantum-radiative hydrodynamic equations: From laser-produced plasmas to astrophysics

J. E. Cross; B. Reville; G. Gregori

doi:10.1088/0004-637X/795/1/59

Scaling of magneto-quantum-radiative hydrodynamic equations: From laser-produced plasmas to astrophysics

J. E. Cross^*, B. Reville, G. Gregori

^*Corresponding author for this work

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

24 Citations (Scopus)

181 Downloads (Pure)

Abstract

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.

Original language	English
Article number	59
Number of pages	10
Journal	Astrophysical Journal
Volume	795
Early online date	14 Oct 2014
DOIs	https://doi.org/10.1088/0004-637X/795/1/59
Publication status	Published - 2014

Keywords

hydrodynamics
ISM: jets and outflows
magnetohydrodynamics (MHD)
plasmas
radiative transfer
supernovae: general

ASJC Scopus subject areas

Nuclear and High Energy Physics

Access to Document

10.1088/0004-637X/795/1/59

Scaling of magneto-quantum-radiative hydrodynamic equations: From laser-produced plasmas to astrophysics
Copyright 2014. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
Final published version, 251 KB

Cite this

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