Homogeneous radiation-filled universe in general scalar tensor theory

Details Homogeneous radiation-filled universe in general scalar tensor theory Homogeneous radiation-filled universe in general scalar tensor theory

Oct 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981jpha...14.2829b&link_type=abstract

Journal of Physics A - Mathematical and General, vol. 14, Oct. 1981, p. 2829-2835. Research supported by the Financiadora de Es

Mathematics

8

Astronomical Models, Cosmic Rays, Cosmology, Tensor Analysis, Universe, Big Bang Cosmology, Radiation Distribution, Singularity (Mathematics)

Scientific paper

The cosmological equations for the general scalar tensor theory proposed by Nordvedt (1970) in a Bianchi type-I, radiation-filled universe are solved, and the behavior of the model is discussed. There are two distinct situations: either the universe will explode from a big bang-type singularity and continuously increase, or the universe may continuously contract to approach the singularity at the end.

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