A singularity-free cosmological model in ECSK theory.

Details A singularity-free cosmological model in ECSK theory. A singularity-free cosmological model in ECSK theory.

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988gregr..20..565j&link_type=abstract

General Relativity and Gravitation, Volume 20, Issue 6, pp.565-571

Mathematics

Logic

8

Cosmological Models:Singularities, Cosmology:General Relativity, General Relativity:Cosmology

Scientific paper

In the framework of the ECSK [Einstein-Cartan-Sciama-Kibble] theory of cosmology, a scalar field nonminimally coupled to the gravitational field is considered. For a Robertson-Walker open universe (k=0) in the radiation era, the field equations admit a singularity-free solution for the scale factor. In theory, the torsion is generated through nonminimal coupling of a scalar field to the gravitation field. The nonsingular nature of the cosmological model automatically solves the flatness problem. Further absence of event horizon and particle horizon explains the high degree of isotropy, especially of 2.7-K background radiation.

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