Thermal conduction and the stability of self-gravitating spheres

Details Thermal conduction and the stability of self-gravitating spheres Thermal conduction and the stability of self-gravitating spheres

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.165..211h&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 165, no. 2, March 1990, p. 211-218.

Astronomy and Astrophysics

Astrophysics

2

Gravitational Collapse, Spheres, Thermal Conductivity, Astronomical Models, Astrophysics, Relativistic Effects, Self Consistent Fields, Stability

Scientific paper

Recent calculations indicating that thermal effects in the relativistic regime may enhance the stability of spherically symmetric models are confirmed in a new example. This new model presents the particularity that the corresponding equation of state permits a bouncing of the boundary effect under some conditions. It is shown that the boundary condition is relaxed by thermal effects, enhancing thereby the possibility of 'exploding' models.

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