Collective scattering of massive stars in higher order gravity

Details Collective scattering of massive stars in higher order gravity Collective scattering of massive stars in higher order gravity

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997phrvd..55..733h&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 55, Issue 2, 15 January 1997, pp.733-738

Mathematics

Probability

6

Gravity In More Than Four Dimensions, Kaluza-Klein Theory, Unified Field Theories, Alternative Theories Of Gravity, Dark Matter

Scientific paper

In the weak field approximation of higher order gravity theory a gravitational potential is described by a Newtonian plus a Yukawa-like term. This new term is used to explain some aspects of galactic dynamics, without considering dark matter. Its presence modifies the scattering probability of a massive intruder star and relaxation time of the stellar system.

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