Oscillatory phase of inflaton and power-law expansion in Bianchi type-I universe

dc.contributor.author	Suresh, P. K.
dc.date.accessioned	2022-03-27T11:32:18Z
dc.date.available	2022-03-27T11:32:18Z
dc.date.issued	2002-12-01
dc.description.abstract	A homogeneous massive scalar field, minimally coupled to the spatially homogeneous and anisotropic background metric, in the semiclassical theory of gravity is examined. In the oscillatory phase of inflaton, the approximate leading solution to the semiclassical Einstein equation for the Bianchi type-I universe shows, each scale factor in each direction obeys t2/3 power-law expansion. Further noted that the evolution of scale factors are mutually correlated.
dc.identifier.citation	International Journal of Theoretical Physics. v.41(7)
dc.identifier.issn	00207748
dc.identifier.uri	10.1023/A:1019611318047
dc.identifier.uri	http://link.springer.com/10.1023/A:1019611318047
dc.identifier.uri	https://dspace.uohyd.ac.in/handle/1/13889
dc.subject	Anisotropic
dc.subject	Cosmology
dc.subject	Inflaton
dc.subject	Power-law expansion
dc.title	Oscillatory phase of inflaton and power-law expansion in Bianchi type-I universe
dc.type	Journal. Article
dspace.entity.type

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