On the existence of stable relativistic star clusters with arbitrarily large central redshifts

Details On the existence of stable relativistic star clusters with arbitrarily large central redshifts On the existence of stable relativistic star clusters with arbitrarily large central redshifts

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...336l..63r&link_type=abstract

Astrophysical Journal (ISSN 0004-637X), vol. 336, Jan. 15, 1989, p. L63-L66.

Statistics

Computation

15

Computational Astrophysics, Red Shift, Relativistic Effects, Star Clusters, Density Distribution, Fokker-Planck Equation, Gravitational Collapse, Gravitational Fields

Scientific paper

A new numerical method for determining the dynamical evolution of a collisionless system in full general relativity has been developed. Using this new method, the existence of stable relativistic star clusters with arbitrarily large central redshifts has been demonstrated. Such clusters may result from the secular evolution of an initially Newtonian, isotropic cluster toward a relativistic state.

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