Abstract
The form of “gravitation”'s law in “projective relativity” is examined, based on a suitable generalization of Poisson's equation in de Sitter space-time; it is found that, in the interior case, a small difference with the customary Newtonian law arises. This difference, of a repulsive character, can be very important in cosmological problems.
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References
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Arcidiacono, G. (1968).Collectanea Mathematica,19, 177.
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Pessa, E. Poisson's equation in de Sitter space-time. Gen Relat Gravit 12, 913–916 (1980). https://doi.org/10.1007/BF00757360
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DOI: https://doi.org/10.1007/BF00757360