What happens near the Schwarzschild sphere for a nonzero graviton rest mass
Teoretičeskaâ i matematičeskaâ fizika, Tome 121 (1999) no. 1, pp. 4-24
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In the relativistic theory of gravity, we analyze the solution for a static spherically symmetrical body in detail. Comparing this solution with the Schwarzschild solution in general relativity, we find that they are essentially different in the domain near the Schwarzschild sphere. This difference eliminates the possibility of a collapse leading to the formation of “black holes”.
@article{TMF_1999_121_1_a1,
author = {A. A. Logunov and M. A. Mestvirishvili},
title = {What happens near the {Schwarzschild} sphere for a nonzero graviton rest mass},
journal = {Teoreti\v{c}eska\^a i matemati\v{c}eska\^a fizika},
pages = {4--24},
publisher = {mathdoc},
volume = {121},
number = {1},
year = {1999},
language = {ru},
url = {http://geodesic.mathdoc.fr/item/TMF_1999_121_1_a1/}
}
TY - JOUR AU - A. A. Logunov AU - M. A. Mestvirishvili TI - What happens near the Schwarzschild sphere for a nonzero graviton rest mass JO - Teoretičeskaâ i matematičeskaâ fizika PY - 1999 SP - 4 EP - 24 VL - 121 IS - 1 PB - mathdoc UR - http://geodesic.mathdoc.fr/item/TMF_1999_121_1_a1/ LA - ru ID - TMF_1999_121_1_a1 ER -
A. A. Logunov; M. A. Mestvirishvili. What happens near the Schwarzschild sphere for a nonzero graviton rest mass. Teoretičeskaâ i matematičeskaâ fizika, Tome 121 (1999) no. 1, pp. 4-24. http://geodesic.mathdoc.fr/item/TMF_1999_121_1_a1/