Cosmological implications of phase coupling gravity

Details Cosmological implications of phase coupling gravity Cosmological implications of phase coupling gravity

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.241..135s&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 241, Nov. 1, 1989, p. 135-151.

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Computation

15

Computational Astrophysics, Cosmology, Evolution (Development), Gravitational Effects, Astronomical Models, Dark Matter, Galactic Rotation, Hubble Diagram, Relativity, Tensors

Scientific paper

The cosmological implications of Bekenstein's (1988) theory of phase coupling gravitation (PCG) are examined. Constraints are placed on the form of the self-interaction potential of the scalar field in PCG theory, which added to the tensor field of general relativity. Cosmological models are calculated for the case of a linear potential that satisfies the general constraints and can predict the observed form of galaxy rotation curves for an evolving universe.

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