Cosmological models in the Schmidt-Greiner-Heinz-Müller theory of gravitation

Details Cosmological models in the Schmidt-Greiner-Heinz-Müller theory of gravitation Cosmological models in the Schmidt-Greiner-Heinz-Müller theory of gravitation

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993phrvd..47.2363s&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 47, Issue 6, 15 March 1993, pp.2363-2370

Mathematics

Logic

6

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

Scientific paper

An exhaustive study of homogeneous and isotropic cosmological models in the Schmidt-Greiner-Heinz-Müller (SGHM) theory of gravitation is performed, where present values of dynamical functions are consistent with astronomical observations and solar-system experiments. We find two types of SGHM models: a first class which is exactly equal to the standard general relativistic (GR) cosmological models, and a second class which never reduces to GR. Some analytical and numerical solutions for the second type of SGHM models are then obtained. The age of the Universe predicted by these models is compatible with the age of old globular clusters except for weak bounds on the Δ0 parameter defined in this paper.

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