|
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
Citation:
A. A. Vlasov, “Spherical quasi-Newtonian stellar pulsations in RTG”, TMF, 106:2 (1996), 320–324; Theoret. and Math. Phys., 106:2 (1996), 265–268
Linking options:
https://www.mathnet.ru/eng/tmf1118https://doi.org/10.4213/tmf1118 https://www.mathnet.ru/eng/tmf/v106/i2/p320
|
Statistics & downloads: |
Abstract page: | 396 | Full-text PDF : | 209 | References: | 68 | First page: | 1 |
|