Abstract
In the bounds of a theoretical scheme treating consistently gravitational interaction as dynamical (gauge) field in flat space-time, an expression was obtained for the density of energy-momentum-tension of gravitational field in vacuum around a collapsed object. A case was studied of an interacting static spherically-symmetric field of a collapsar in vacuum with taking into account of input of all the possible components (spin states of virtual gravitons) into the energy for the symmetric tensor of second rankψ ik . The radius of the sphere filled by matter for the collapsar of massM may achieve values up toGM/c 2.
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References
Baryshev, Y. V. and Sokolov, V. V.: 1984,AStrofizika 21, 361.
Bogolyubov, N. N. and Shirkov, D. V.: 1973,Introduction in Gauge Field Theory, Nauka, Moscow, p. 480.
Konopleva, N. P. and Popov, V. N.: 1973,Gauge Fields, Atomizdat, Moscow (in Russian).
Landau, L. D. and Lifshitz, E. M.: 1973,Theory of Field, Nauka, Moscow, p. 504.
Mosinsky, M.: 1950,Phys. Rev. 80, 514.
Sexl, R. U.: 1967,Fortschritte Phys. 15, 269.
Sokolov, V. V.: 1992,Astrophys. Space Sci. 191, 231.
Sokolov, V. V. and Baryshev, Y. V.: 1980, inGravitation and General Relativity, KGU Kazan', Vol. 17, p. 34 (in Russian).
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Sokolov, V.V. Nonlinear gravidynamics: Energy-momentum tensor of collapsar field. Astrophys Space Sci 197, 87–108 (1992). https://doi.org/10.1007/BF00645075
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DOI: https://doi.org/10.1007/BF00645075