A special-relativistic approach to gravitation and its astrophysical consequences

Details A special-relativistic approach to gravitation and its astrophysical consequences A special-relativistic approach to gravitation and its astrophysical consequences

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.113..199m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 113, no. 1, July 1985, p. 199-203.

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Computation

4

Computational Astrophysics, Gravitation Theory, Relativistic Theory, Elementary Particles, Gravitational Fields, Mass

Scientific paper

A variant of modified classical gravitation theory that is based on Einstein's energy-mass equivalence principle is presently constructed within the framework of Rastall's (1979) conservative program for the construction of gravitation theory. Special-relativistic arguments are pursued, and a theory is obtained for the static, spherically symmetric gravitation field that is based only on well established physical principles and accounts for all experimental tests thus far conducted in gravitation theory. Attention is also given to such atronomical consequences of the modified classical gravitation theory as the nonexistence of black holes and the creation of real particles in a strong gravitation field.

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