Annotation
We find numerical solutions for a system of gravitational equations (these equations were proposed by Yu.M. Loskutov after modification of the Hilbert-Einstein equations) for the internal and external physical characteristics of compact stars with a moderate concentration of matter when their gravitational fields are not too strong. The evolution of solutions with an increase of the mass of an object is simulated. The corresponding graphs are constructed.
Received: 2012 February 1
Approved: 2012 November 2
PACS:
95.30.Sf Relativity and gravitation
04.70.-s Physics of black holes
04.70.-s Physics of black holes
© 2016 Publisher M.V.Lomonosov Moscow State University
Authors
A.S. Rokhmanenkov
Department of Quantum Theory and High Energy Physics, Faculty of Physics, Moscow State University, Moscow, 119991, Russia
Department of Quantum Theory and High Energy Physics, Faculty of Physics, Moscow State University, Moscow, 119991, Russia
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