Issue of the spherically symmetric static vacuum metric in the relativistic theory of gravity
The spherically symmetric vacuum metric in the relativistic theory of gravity is analyzed numerically. It is found that there is no deviation of the numerical solution from that of general relativity except in the near-horizon range. The solution obtained has the well-established analytical asymptotics for both the near-and far-horizon limits. It satisfies the causality principle and does not impose a lower limit on the graviton mass.
Keywordsrelativistic theory of gravity Schwarzschild problem
PACS (2008)04.20.-q 04.25.dg 04.20.Ex 04.70.s
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