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Main Authors: Yeasmin, Sabina, Deshamukhya, Atri
Format: Preprint
Published: 2024
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Online Access:https://arxiv.org/abs/2408.00595
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author Yeasmin, Sabina
Deshamukhya, Atri
author_facet Yeasmin, Sabina
Deshamukhya, Atri
contents We study warm inflation in the framework of $f(ϕ)T$ gravity, where $ϕ$ is the inflaton and $T$ is the trace of the energy-momentum tensor. The inflaton field is assumed to roll on the natural potential and the result is analyzed in light of Planck 2018 and BICEP/Keck 2021 data. We start our work by obtaining the field equations under slow-roll approximations. We then evaluate the scalar and tensor power spectra and their corresponding spectral index and tensor-to-scalar ratio with a temperature-dependent form of the dissipation coefficient during the inflationary era. We find that the warm inflation model in $f(ϕ)T$ gravity is compatible with observational bands.
format Preprint
id arxiv_https___arxiv_org_abs_2408_00595
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Embedding Warm Natural Inflation in $f(ϕ)T$ gravity
Yeasmin, Sabina
Deshamukhya, Atri
General Relativity and Quantum Cosmology
We study warm inflation in the framework of $f(ϕ)T$ gravity, where $ϕ$ is the inflaton and $T$ is the trace of the energy-momentum tensor. The inflaton field is assumed to roll on the natural potential and the result is analyzed in light of Planck 2018 and BICEP/Keck 2021 data. We start our work by obtaining the field equations under slow-roll approximations. We then evaluate the scalar and tensor power spectra and their corresponding spectral index and tensor-to-scalar ratio with a temperature-dependent form of the dissipation coefficient during the inflationary era. We find that the warm inflation model in $f(ϕ)T$ gravity is compatible with observational bands.
title Embedding Warm Natural Inflation in $f(ϕ)T$ gravity
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2408.00595