Self-consistent radiation-hydrodynamic equations for stellar oscillations. I - Nonlinear form

Details Self-consistent radiation-hydrodynamic equations for stellar oscillations. I - Nonlinear form Self-consistent radiation-hydrodynamic equations for stellar oscillations. I - Nonlinear form

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...284..299m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 284, Sept. 1, 1984, p. 299-302.

Astronomy and Astrophysics

Astrophysics

14

Hydrodynamic Equations, Radiative Transfer, Stellar Oscillations, Eddington Approximation, Plancks Constant, Poisson Equation, Thermodynamic Equilibrium

Scientific paper

Using the correct comoving frame, or Lagrangian, equations of radiation hydrodynamics derived by Castor and Buchler, earlier discussions of radiation hydrodynamics in the nonequilibrium diffusion regime are critically examined. Comparison of corresponding equations reveals a fundamental conceptual error in previous treatments of the interaction between stellar oscillations and the radiation field.

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