Abstract
The conservation laws are used to find the dependence of the energy transported by a spherical gravitation disturbance (emitted by a centrally symmetric body on the transition between two static states) on the distance from the source. The observability of such a wave is discussed.
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N. A. Voznesenskii Leningrad Finance and Economics Institute. Translated from Teoreticheskaya i Matematicheskaya Fizika, Vol. 91, No. 2, pp. 346–352, May, 1992.
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Genk, A.V. Spherical gravitational waves in the relativistic theory of gravitation. Theor Math Phys 91, 570–574 (1992). https://doi.org/10.1007/BF01018855
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DOI: https://doi.org/10.1007/BF01018855