The dynamical structure of the Einstein equations for a non-rotating starss

Details The dynamical structure of the Einstein equations for a non-rotating starss The dynamical structure of the Einstein equations for a non-rotating starss

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993gregr..25..441m&link_type=abstract

General Relativity and Gravitation, Volume 25, Issue 5, pp.441-460

Computer Science

11

Scientific paper

The relativistic interior dynamics of a spherically symmetric, non rotating star composed of an elastic material is analyzed. A suitable formulation of relativistic elasticity is used, and the corresponding second order Einstein equations are found. The equations arise naturally in a non-comoving frame and reduce, in the static case, to the “generalized” Tohnan-Oppenheimer-Volkhoff equations considered by J. Kijowski and the author in a previous paper. The charged case is also discussed.

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