Perturbative solutions of the -theory of gravity in a central gravitational field and some applications
arXiv:1807.04628 · doi:10.1140/epjc/s10052-018-6023-6
Abstract
Exact solutions of an -theory (of gravity) in a static central (gravitational) field have been studied in the literature quite well, but, to find and study exact solutions in the case of a non-static central field are not easy at all. There are, however, approximation methods of finding a solution in a central field which is not necessarily static. It is shown in this article that an approximate solution of an -theory in a general central field, which is not necessary to be static, can be found perturbatively around a solution of the Einstein equation in the general theory of relativity. In particular, vacuum solutions are found for of general and some special forms. Further, applications to the investigation of a planetary motion and light's propagation in a central field are presented. An effect of an -gravity is also estimated for the SgrA*--S2 system. The latter gravitational system is much stronger than the Sun--Mercury system, thus the effect could be much stronger and, thus, much more measurable.
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- Metric Variation of the Energy-Momentum Tensor of a Perfect Fluid and Its Applications to Cosmology and Neutron Stars