Classical repulsive gravity and broken Lorentz symmetry

Details Classical repulsive gravity and broken Lorentz symmetry Classical repulsive gravity and broken Lorentz symmetry

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986phrvd..34.2260g&link_type=abstract

Physical Review D (Particles and Fields), Volume 34, Issue 8, 15 October 1986, pp.2260-2262

Physics

9

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

Scientific paper

A four-dimensional quasi-Riemannian theory of gravity, with local SO(3) invariance, is used as a simple model to describe gravity under the hypothesis of broken Lorentz gauge symmetry, and to show that in this case the sign of the force between two masses may depend on their relative distance. Considering in particular the field of a static, central macroscopic source, we find however that the gravitational interaction experienced by a macroscopic test body may become repulsive only immediately close to the Schwarzschild surface.

Affiliated with

Also associated with

No associations

Rating

Classical repulsive gravity and broken Lorentz symmetry does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Classical repulsive gravity and broken Lorentz symmetry, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Classical repulsive gravity and broken Lorentz symmetry will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1740918