Relativity and Cosmology

   

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

Authors: Lluís 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: 6 Pages.

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Submission history

[v1] 2018-09-07 06:09:33

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