Surface phenomena in general relativistic stellar models: critical mass and stability

Details Surface phenomena in general relativistic stellar models: critical mass and stability Surface phenomena in general relativistic stellar models: critical mass and stability

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988phla..130..211h&link_type=abstract

Physics Letters A, Volume 130, Issue 4-5, p. 211-216.

Physics

4

Scientific paper

The influence of surface phenomena on general relativistic stellar models is investigated, with particular emphasis on the critical mass value and the adiabatic stability. It will be shown, in a particular model, that for a given radius, the maximum value of the total mass (compatible with a static, singularity-free configuration) is a decreasing function of the surface tension coefficient. It will also be shown that the inclusion of surface phenomena enhances the adiabatic instability of the model in the high density regime.

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