Abstract:
The condition under which a spherically symmetric gravitational field is physical in the relativistic theory of gravitation is analyzed. It is shown that this condition restricts the value of the constant that appears in the exterior spherically symmetric stationary solution to the equations of the relativistic theory of gravitation.
Citation:
P. V. Karabut, Yu. V. Chugreev, “Conditions under which the exterior spherically symmetric solution to the equations of the relativistic theory of gravitation is physical”, TMF, 84:3 (1990), 474–480; Theoret. and Math. Phys., 84:3 (1990), 1006–1011
\Bibitem{KarChu90}
\by P.~V.~Karabut, Yu.~V.~Chugreev
\paper Conditions under which the exterior spherically symmetric solution to~the equations of~the relativistic theory of~gravitation is~physical
\jour TMF
\yr 1990
\vol 84
\issue 3
\pages 474--480
\mathnet{http://mi.mathnet.ru/tmf5924}
\zmath{https://zbmath.org/?q=an:0717.53053|0709.53056}
\transl
\jour Theoret. and Math. Phys.
\yr 1990
\vol 84
\issue 3
\pages 1006--1011
\crossref{https://doi.org/10.1007/BF01017360}
\isi{https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=Publons&SrcAuth=Publons_CEL&DestLinkType=FullRecord&DestApp=WOS_CPL&KeyUT=A1990FF85600013}
Linking options:
https://www.mathnet.ru/eng/tmf5924
https://www.mathnet.ru/eng/tmf/v84/i3/p474
This publication is cited in the following 3 articles:
Chugreev Yu.V., “Cosmological Constraints on the Graviton Mass in Rtg”, Phys. Part. Nuclei Lett., 14:4 (2017), 539–549
Yu. V. Chugreev, “Causality Principle for a Reissner–Nordstrom Field in the RTG: The Small-Charge Case $q^2 \le m^2$”, Theoret. and Math. Phys., 132:3 (2002), 1301–1308
A. V. Genk, “Spherical gravitational waves in the relativistic theory of gravitation”, Theoret. and Math. Phys., 91:2 (1992), 570–574