Physics
Scientific paper
Nov 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.197..179s&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 197, no. 2, p. 179-212.
Physics
4
Gravitational Collapse, Gravitational Fields, High Energy Interactions, Stellar Mass, Field Theory (Physics), Gravitons, Particle Mass, Statics
Scientific paper
The strong field of a compact object (a collapsar) - an analog to the black hole in general relativity - is investigated within the framework of the totally nonmetric model of gravitational interaction theory (gravidynamics). In the case of the strongest possible (for gravidynamics) collapsar field a region filled by matter (a bag) must have a radius equal to GM/C-squared is less than about 10 km at the total collapsar mass of less than about 7 solar masses. Only half of the collapsar mass is contained in the bag, while the other half of its total energy (Mc-squared) is distributed in the space surrounding the bag in the form of a 'coat', i.e., in the form of a continuous medium of virtual gravitons. The object must have a surface (bag surface) with absolutely definite physical properties. The potential of such a surface is finite, and the particle mass in a bound state on the bag surface is half that of the mass of the same particle in a totally free state. The bag surface can perform periodic oscillations with a period of 0.00003 sec.
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