Journal of the Korean Physical Society vol. 28, no. SUPPL. 4, pp. S519 - S524
Indexed
SCI; SCIE; SCOPUS; KCI
Document Type
Article
Abstract
In this paper the Brans-Dicke cosmological model with torsion is considered. The effects of the spin and the scalar field on the expansion rate and the types of inflation are discussed. It is shown that the expansion rate is faster than the extended inflation.