Physics
Scientific paper
Nov 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.197...87s&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 197, no. 1, p. 87-108.
Physics
3
Gravitation Theory, Gravitational Collapse, Gravitational Fields, Field Theory (Physics), Nonlinearity, Tensors
Scientific paper
An expression is derived for the density of energy-momentum-tension of gravitational field in vacuum around a collapsed object in the framework of a theoretical scheme that treats gravitational interaction as dynamic field in flat space-time. An interacting static spherically-symmetric field of a collapsar in vacuum is considered taking into account the input of all possible components into the energy for the symmetric tensor of second rank. It is found that the radius of the sphere filled by matter for the collapsar of mass M may reach values up to GM/c exp 2.
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