Spherical quasi-Newtonian stellar pulsations in RTG
Teoretičeskaâ i matematičeskaâ fizika, Tome 106 (1996) no. 2, pp. 320-324
A. A. Vlasov. Spherical quasi-Newtonian stellar pulsations in RTG. Teoretičeskaâ i matematičeskaâ fizika, Tome 106 (1996) no. 2, pp. 320-324. http://geodesic.mathdoc.fr/item/TMF_1996_106_2_a12/
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It is shown that in Relativistic Theory of Gravity, in contrast to GTR the spherically symmetric stellar pulsations lead to the nonstatic behaviour of an external gravitational field.

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