Emergence of squeezed coherent states in Kaluza–Klein cosmology
In this work, we consider a propagating scalar field on Kaluza–Klein-type cosmological background. It is shown that this geometrical description of the Universe resembles – from a Hamiltonian standpoint – a damped harmonic oscillator with mass and frequency, both time-dependents. In this scenario, w...
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Published in | Annals of physics Vol. 470; p. 169805 |
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Main Authors | , , , |
Format | Journal Article |
Language | English |
Published |
Elsevier Inc
01.11.2024
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Subjects | |
Online Access | Get full text |
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Summary: | In this work, we consider a propagating scalar field on Kaluza–Klein-type cosmological background. It is shown that this geometrical description of the Universe resembles – from a Hamiltonian standpoint – a damped harmonic oscillator with mass and frequency, both time-dependents. In this scenario, we construct the squeezed coherent states (SCSs) for the quantized scalar field by employing the invariant operator method of Lewis–Riesenfeld (non-Hermitian) in a non-unitary approach. The non-classicality of SCSs has been discussed by examining the quadrature squeezing properties from the uncertainty principle. Moreover, we compute the probability density, which allows us to investigate whether SCSs can be used to seek traces of extra dimensions. We then analyze the effects of the existence of supplementary space on cosmological particle production in SCSs by considering different cosmological eras.
•The scalar field on a Kaluza-Klein-type scenario behaves as a damped oscillator.•Squeezed coherent states (SCSs) are constructed for a quantized scalar field.•The non-classical nature of SCSs is analyzed.•The influence of extra dimension on the constructed SCSs has been investigated. |
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ISSN: | 0003-4916 |
DOI: | 10.1016/j.aop.2024.169805 |