Three-Dimensional General Relativistic Dynamics of Relativistic Stars

Details Three-Dimensional General Relativistic Dynamics of Relativistic Stars Three-Dimensional General Relativistic Dynamics of Relativistic Stars

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001cnoc.conf...41r&link_type=abstract

The Second National Conference on Astrophysics of Compact Objects, held in Bologna (Italy), September 19 - 21, 2001, p. 41

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present results obtained with a three-dimensional general- relativistic hydrodynamics code in the study of the long-term dynamics of relativistic stars. Our investigations focus on the pulsations of stable rotating and nonrotating relativistic stars and on the nonlinear evolution of unstable nonrotating relativistic stars. We also discuss the numerical evolution of both spherical and rapidly rotating, stationary configurations, and the formation of an apparent horizon during the collapse of a relativistic star to a black hole. Overall, the results obtained represent the most accurate long-term three-dimensional evolutions of relativistic stars available to date.

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