Investigation on the Consequences of a Strengthened Newtonian Gravity at Short Distances

Aghalovyan, Lenser (2020) Investigation on the Consequences of a Strengthened Newtonian Gravity at Short Distances. In: New Insights into Physical Science Vol. 9. B P International, pp. 24-33. ISBN 978-93-90516-35-3

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Abstract

The construction of the theory of movement of the solar planet system was a triumph of science in the
middle ages, especially in Astronomy and Mechanics. The confrontation between the supporters of
Ptolemaic geocentric system and heliocentric system of Aristarchus-Copernicus lasting for centuries
ended with the victory of the latters. A central interaction of bodies which at short distances is stronger
than Newtonian is considered. It is shown that the escape velocity from a body is essentially more
than the escape velocity given by Newton’s theory. According to Newton’s law the force of Universal
Gravitation is central, each mass m is attracted by another mass M in the Universe with force,
inversely proportional to the quadrate of distance between the masses, and is directed along the line,
connecting the centers of the masses. The connection of the new central interaction with the
gravitational radius of a black hole is found. It is shown that the gravitational radius of a black hole
may be arbitrarily large. The gravitation of the Black Hole (Dark Body) does not obey the classical
(Newtonian) law of Gravitation, it obeys the law of the essentially powerful central gravitation.

Item Type: Book Section
Subjects: Archive Paper Guardians > Physics and Astronomy
Depositing User: Unnamed user with email support@archive.paperguardians.com
Date Deposited: 15 Nov 2023 07:29
Last Modified: 15 Nov 2023 07:29
URI: http://archives.articleproms.com/id/eprint/2267

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