Density fluctuations in the oscillatory phase of a nonclassical inflaton in the FRW universe

dc.contributor.author Venkataratnam, K. K.
dc.contributor.author Suresh, P. K.
dc.date.accessioned 2022-03-27T11:32:13Z
dc.date.available 2022-03-27T11:32:13Z
dc.date.issued 2008-10-01
dc.description.abstract The use of the coherent and squeezed state formalisms of quantum optics for a minimally coupled nonclassical inflaton in the FRW metric is studied, in the semiclassical theory of gravity. The leading order solutions to the semiclassical Einstein equations in the coherent, squeezed and squeezed vacuum states are obtained perturbatively and exhibit power law expansion behavior. The validity of the semiclassical theory is examined in the squeezed vacuum state in the oscillatory phase of the inflaton. The semiclassical theory in the oscillatory phase of the nonclassical inflaton holds only if the associated squeezing parameter is much smaller than unity. Quantum fluctuations of the inflaton are also examined in the coherent and squeezed state formalisms. © 2008 World Scientific Publishing Company.
dc.identifier.citation International Journal of Modern Physics D. v.17(11)
dc.identifier.issn 02182718
dc.identifier.uri 10.1142/S0218271808013662
dc.identifier.uri https://www.worldscientific.com/doi/abs/10.1142/S0218271808013662
dc.identifier.uri https://dspace.uohyd.ac.in/handle/1/13878
dc.subject Density fluctuations
dc.subject Semiclassical theory
dc.subject Squeezed vacuum
dc.title Density fluctuations in the oscillatory phase of a nonclassical inflaton in the FRW universe
dc.type Journal. Article
dspace.entity.type
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