Relativity and Cosmology


A Fully Relativistic Description of Stellar or Planetary Objects Orbiting a Very Heavy Central Mass

Authors: Ll. Bel

A fully relativistic numerical program is used to calculate the advance of the peri-helium of Mercury or the deflection of light by the Sun is here used also to discuss the case of S2, a star orbiting a very heavy central mass of the order of $4.3\,10^6$ solar masses.

Comments: 8 Pages. A section has been extended, some material suppressed

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Submission history

[v1] 2018-09-07 06:09:33
[v2] 2018-10-23 04:13:03

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