Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984rpphm...6..113g&link_type=abstract
In its USSR Rept.: Phys. and Math. (JPRS-UPM-84-006) p 113 (SEE N85-11676 02-70) Transl. into ENGLISH from Dokl. Akad. Nauk SSS
Astronomy and Astrophysics
Astronomy
Black Holes (Astronomy), Gravitation, Space-Time Functions, Stellar Mass, Vacuum, Mass Distribution, Momentum, Polarization Characteristics, Stellar Structure
Scientific paper
The existence of a special gravitational vacuum is considered in this paper. A phenomenological method differing from the traditional Einsteinian formalization is utilized. Vacuum, metric and matter form a complex determined by field equations and at great distances from gravitational masses vacuum effects are small but could be large in powerful fields. Singularities and black holes justify the approach as well as the Ambartsmyan theory concerning the existence of supermassive and superdense prestallar bodies that then disintegrate. A theory for these superdense bodies is developed involving gravitational field equations that describe the vacuum by an energy momentum tensor and define the field and mass distribution. Computations based on the theory for gravitational radii with incompressible liquid models adequately reflecting real conditions indicate that a gravitational vacuum could have considerable effects on superdense stars and could have radical effects for very large masses.
Grigoryan Sh. L.
Saakyan G. S.
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