We numerically construct models of spherically symmetric relativistic stellar clusters with anisotropic distribution functions. Newtonian solutions obtained in Paper I are generalized as isotropicMaxwellian ones with energy cutoff in their distribution function.We consider distributions with different levels of anisotropy and discuss some general characteristics of the models.

SPHERICALLY SYMMETRIC STELLAR CLUSTERS WITH ANISOTROPY AND CUTOFF ENERGY IN MOMENTUM DISTRIBUTION. II. THE RELATIVISTIC REGIME / Gennady S., Bisnovatyi Kogan; Merafina, Marco; Maria Rosaria, Vaccarelli. - In: THE ASTROPHYSICAL JOURNAL. - ISSN 0004-637X. - ELETTRONICO. - 709:2(2010), pp. 1174-1182. [10.1088/0004-637x/709/2/1174]

SPHERICALLY SYMMETRIC STELLAR CLUSTERS WITH ANISOTROPY AND CUTOFF ENERGY IN MOMENTUM DISTRIBUTION. II. THE RELATIVISTIC REGIME

MERAFINA, Marco;
2010

Abstract

We numerically construct models of spherically symmetric relativistic stellar clusters with anisotropic distribution functions. Newtonian solutions obtained in Paper I are generalized as isotropicMaxwellian ones with energy cutoff in their distribution function.We consider distributions with different levels of anisotropy and discuss some general characteristics of the models.
2010
general relativity; star clusters; dense matter; hydrodynamics
01 Pubblicazione su rivista::01a Articolo in rivista
SPHERICALLY SYMMETRIC STELLAR CLUSTERS WITH ANISOTROPY AND CUTOFF ENERGY IN MOMENTUM DISTRIBUTION. II. THE RELATIVISTIC REGIME / Gennady S., Bisnovatyi Kogan; Merafina, Marco; Maria Rosaria, Vaccarelli. - In: THE ASTROPHYSICAL JOURNAL. - ISSN 0004-637X. - ELETTRONICO. - 709:2(2010), pp. 1174-1182. [10.1088/0004-637x/709/2/1174]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/67350
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