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Russian Physics Journal

, Volume 37, Issue 10, pp 925–928 | Cite as

Radiative sublimation of a homogeneous, relativistic model star

  • A. M. Baranov
  • N. N. Paklin
Physics Of Elementary Particles And Field Theory
  • 14 Downloads

Abstract

A relativistic model of a radiating star is constructed as a generalization of an exact, internal Schwarzschild solution. The version of radiative sublimation in which radiation appears at the stellar surface while the inner layers remain in hydrostatic equilibrium is considered. The generalization procedure presumes that Pascal's law is violated for the stress tensor. The model's behavior is studied for different values of the parameter that allows for the predominance of tangential or radial stresses. Upon a change in the sign of the parameter, the model dynamics reveals a bifurcation, reflected in the time dependence of the star's radius, pressure, and luminosity.

Keywords

Radiation Time Dependence Stress Tensor Relativistic Model Radial Stress 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Plenum Publishing Corporation 1995

Authors and Affiliations

  • A. M. Baranov
  • N. N. Paklin

There are no affiliations available

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