Radiative properties for astrophysical plasma mixtures in nonlocal thermodynamic equilibrium

Rafael Rodríguez, Guadalupe Espinosa, and Juan Miguel Gil
Phys. Rev. E 98, 033213 – Published 28 September 2018

Abstract

Radiative properties play a pivotal role in astrophysical plasma flows and are needed in radiation-hydrodynamic simulations in order to understand their behavior and also to interpret the plasma emission spectra, which are valuable diagnostic tools. Radiative properties of astrophysical plasma mixtures have been commonly calculated for low-density optically thin plasmas assuming coronal equilibrium and for high density assuming local thermodynamic equilibrium. However, there are wide ranges of conditions in which these thermodynamic regimes are not achieved and the plasma is in the nonlocal thermodynamic equilibrium regime. In the present work, a study of the plasma radiative properties of oxygen and iron and an astrophysical plasma mixture in nonlocal thermodynamic steady-state equilibrium is carried out. The ranges of electron temperatures and densities considered are 1–1000 eV and 10111020cm3, respectively. In the study, departures from coronal and local thermodynamic equilibria in terms of the density and temperature are also analyzed. Large differences in the radiative properties that can reach two orders of magnitude when the plasma is far from these thermodynamic regimes are obtained. These analyses are done assuming the plasma to be optically thin. A brief study of the influence of the plasma self-absorption in the radiative properties of oxygen and iron is made. For that purpose, the plasma is assumed with planar geometry and the study is performed in terms of the width of the plasma slab and electron temperature and density.

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  • Received 20 June 2018

DOI:https://doi.org/10.1103/PhysRevE.98.033213

©2018 American Physical Society

Physics Subject Headings (PhySH)

Plasma Physics

Authors & Affiliations

Rafael Rodríguez1,2,*, Guadalupe Espinosa1, and Juan Miguel Gil1,2

  • 1Departamento de Física, IUNAT, Universidad de Las Palmas de Gran Canaria, 35017 Las Palmas de Gran Canaria, Spain
  • 2Instituto de Fusión Nuclear, Universidad Politécnica de Madrid, 28006 Madrid, Spain

  • *rafael.rodriguezperez@ulpgc.es

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Issue

Vol. 98, Iss. 3 — September 2018

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