Geodesic
Spherical gravitational waves in the relativistic theory of gravitation
Teoretičeskaâ i matematičeskaâ fizika, Tome 91 (1992) no. 2, pp. 346-352

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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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     author = {A. V. Genk},
     title = {Spherical gravitational waves in the relativistic theory of gravitation},
     journal = {Teoreti\v{c}eska\^a i matemati\v{c}eska\^a fizika},
     pages = {346--352},
     publisher = {mathdoc},
     volume = {91},
     number = {2},
     year = {1992},
     language = {ru},
     url = {http://geodesic.mathdoc.fr/item/TMF_1992_91_2_a11/}
}
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A. V. Genk. Spherical gravitational waves in the relativistic theory of gravitation. Teoretičeskaâ i matematičeskaâ fizika, Tome 91 (1992) no. 2, pp. 346-352. http://geodesic.mathdoc.fr/item/TMF_1992_91_2_a11/