Theoretical and observational prescription of warm-inflation in FLRW universe with torsion

Abstract The paper deals with Warm Inflationary scenario in FLRW with torsion both from theoretical and observational point of view. In the background of flat FLRW model the Hubble parameter is found to be proportional to the torsion function and warm inflation is examined both in weak and strong di...

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Main Authors: Madhukrishna Chakraborty, Gopal Sardar, Akash Bose, Subenoy Chakraborty
Format: Article
Language:English
Published: SpringerOpen 2023-09-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-023-12030-8
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author Madhukrishna Chakraborty
Gopal Sardar
Akash Bose
Subenoy Chakraborty
author_facet Madhukrishna Chakraborty
Gopal Sardar
Akash Bose
Subenoy Chakraborty
author_sort Madhukrishna Chakraborty
collection DOAJ
description Abstract The paper deals with Warm Inflationary scenario in FLRW with torsion both from theoretical and observational point of view. In the background of flat FLRW model the Hubble parameter is found to be proportional to the torsion function and warm inflation is examined both in weak and strong dissipation regimes for the power law choice of potential using slow-roll approximation with quasi-stable criteria for radiation. The slow-roll parameters, no.of e-folds, scalar spectral index, and tensor-to-scalar ratio are determined in the present model for mainly three choices of the dissipation coefficient $$\Gamma $$ Γ using the Planck data set. Finally, we focus on single-field chaotic quartic potential with the above choices of the dissipation coefficient to confront the warm inflation observational predictions directly with the latest observational data set.
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spelling doaj.art-bc3c8f1cacbb4b3fb7381a39d255632c2023-10-29T12:33:36ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60522023-09-0183911410.1140/epjc/s10052-023-12030-8Theoretical and observational prescription of warm-inflation in FLRW universe with torsionMadhukrishna Chakraborty0Gopal Sardar1Akash Bose2Subenoy Chakraborty3Department of Mathematics, Jadavpur UniversityDepartment of Mathematics, Jadavpur UniversityDepartment of Mathematics, Jadavpur UniversityDepartment of Mathematics, Jadavpur UniversityAbstract The paper deals with Warm Inflationary scenario in FLRW with torsion both from theoretical and observational point of view. In the background of flat FLRW model the Hubble parameter is found to be proportional to the torsion function and warm inflation is examined both in weak and strong dissipation regimes for the power law choice of potential using slow-roll approximation with quasi-stable criteria for radiation. The slow-roll parameters, no.of e-folds, scalar spectral index, and tensor-to-scalar ratio are determined in the present model for mainly three choices of the dissipation coefficient $$\Gamma $$ Γ using the Planck data set. Finally, we focus on single-field chaotic quartic potential with the above choices of the dissipation coefficient to confront the warm inflation observational predictions directly with the latest observational data set.https://doi.org/10.1140/epjc/s10052-023-12030-8
spellingShingle Madhukrishna Chakraborty
Gopal Sardar
Akash Bose
Subenoy Chakraborty
Theoretical and observational prescription of warm-inflation in FLRW universe with torsion
European Physical Journal C: Particles and Fields
title Theoretical and observational prescription of warm-inflation in FLRW universe with torsion
title_full Theoretical and observational prescription of warm-inflation in FLRW universe with torsion
title_fullStr Theoretical and observational prescription of warm-inflation in FLRW universe with torsion
title_full_unstemmed Theoretical and observational prescription of warm-inflation in FLRW universe with torsion
title_short Theoretical and observational prescription of warm-inflation in FLRW universe with torsion
title_sort theoretical and observational prescription of warm inflation in flrw universe with torsion
url https://doi.org/10.1140/epjc/s10052-023-12030-8
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