Oscillatory phase of nonclassical thermal inflaton in frw universe

dc.contributor.author Venkataratnam, K. K.
dc.contributor.author Suresh, P. K.
dc.date.accessioned 2022-03-27T11:32:09Z
dc.date.available 2022-03-27T11:32:09Z
dc.date.issued 2010-07-01
dc.description.abstract A minimally coupled nonclassical homogeneous scalar field is examined in the flat FRW universe in the semiclassical theory of gravity. Particle production in thermal coherent and squeezed states is studied for the flat FRW universe, in the oscillatory phase of the inflaton. Solutions for the semiclassical Friedmann equations are obtained in the thermal nonclassical states. Validity of the semiclassical theory is examined in the thermal coherent and squeezed states in the oscillatory phase of inflaton. Particle creation can be enhanced due to thermal and quantum effects. Quantum fluctuations of the inflaton in thermal coherent and squeezed state formalisms are also studied. Classical gravity differ from semiclassical gravity in the thermal coherent state only by an amplitude factor. © 2010 World Scientific Publishing Company.
dc.identifier.citation International Journal of Modern Physics D. v.19(7)
dc.identifier.issn 02182718
dc.identifier.uri 10.1142/S0218271810017184
dc.identifier.uri https://www.worldscientific.com/doi/abs/10.1142/S0218271810017184
dc.identifier.uri https://dspace.uohyd.ac.in/handle/1/13872
dc.subject inflaton
dc.subject particle creation
dc.subject semiclassical gravity
dc.subject Thermal coherent state
dc.subject thermal squeezed state
dc.title Oscillatory phase of nonclassical thermal inflaton in frw universe
dc.type Journal. Article
dspace.entity.type
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