Density fluctuations and single-mode thermal states in the FRW universe

Using single-mode squeezed and coherent thermal states formalism, we analyzed the validity of the semiclassical Einstein equation (SCEE) in the flat Friedmann–Robertson–Walker universe by analyzing the density fluctuations in terms of a massive inflaton. In a single-mode squeezed thermal states the...

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Veröffentlicht in:European physical journal plus 2020-04, Vol.135 (4), p.360, Article 360
Hauptverfasser: Dhayal, Renu, Rathore, Meghna, Kambila, Vijay Kumar, Venkataratnam, K. K.
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Rathore, Meghna
Kambila, Vijay Kumar
Venkataratnam, K. K.
description Using single-mode squeezed and coherent thermal states formalism, we analyzed the validity of the semiclassical Einstein equation (SCEE) in the flat Friedmann–Robertson–Walker universe by analyzing the density fluctuations in terms of a massive inflaton. In a single-mode squeezed thermal states the density fluctuations are too large; consequently, the semiclassical theory of gravity (SCTG) does not hold good, for squeezing parameter greater than unity, i.e., r s > 1 ; however, the theory is valid when this related squeezing parameter is smaller than the unity, i.e., r s < < 1 and r s < 1 . Also, it is noted that the SCEE is dependable on coherent thermal state formalism. The current study provides a description of the density fluctuations as a result of the quantum and thermal effects in the SCTG.
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subjects Applied and Technical Physics
Atomic
Complex Systems
Compressing
Condensed Matter Physics
Cosmology
Density
Einstein equations
Fluctuations
Formalism
Gravitation theory
Gravity
Mathematical and Computational Physics
Molecular
Optical and Plasma Physics
Parameters
Physics
Physics and Astronomy
Quantum field theory
Regular Article
Temperature effects
Theoretical
Unity
Universe
Validity
title Density fluctuations and single-mode thermal states in the FRW universe
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