Spherical quasi-Newtonian stellar pulsations in RTG

A. A. Vlasov

M. V. Lomonosov Moscow State University

Abstract: 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.

Received: 10.03.1995

DOI: 10.4213/tmf1118

 English version: Theoretical and Mathematical Physics, 1996, 106:2, 265–268

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