A model of inflation consistent with Planck 2018 and BICEP/Keck data

Abstract We establish a phenomenological inflation model in this paper and find that the predicted values of the spectral index and the tensor-to-scalar ratio are well consistent with the results from the Planck 2018 survey and the BICEP/Keck array measurement, significantly improving the theoretica...

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Main Authors: Li-Yang Chen, Hongwei Yu, Puxun Wu
Format: Article
Language:English
Published: SpringerOpen 2025-01-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-024-13728-z
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author Li-Yang Chen
Hongwei Yu
Puxun Wu
author_facet Li-Yang Chen
Hongwei Yu
Puxun Wu
author_sort Li-Yang Chen
collection DOAJ
description Abstract We establish a phenomenological inflation model in this paper and find that the predicted values of the spectral index and the tensor-to-scalar ratio are well consistent with the results from the Planck 2018 survey and the BICEP/Keck array measurement, significantly improving the theoretical precision in describing the early universe’s inflationary process. After inflation, we find that preheating can occur from the tachyonic instability or the parametric resonance, which depends on the value of one of model parameters.
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institution Kabale University
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publishDate 2025-01-01
publisher SpringerOpen
record_format Article
series European Physical Journal C: Particles and Fields
spelling doaj-art-f579c77dc4744a0388119641e0fef5342025-02-02T12:38:39ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60522025-01-018521510.1140/epjc/s10052-024-13728-zA model of inflation consistent with Planck 2018 and BICEP/Keck dataLi-Yang Chen0Hongwei Yu1Puxun Wu2College of Physics and Engineering Technology, Chengdu Normal UniversityDepartment of Physics and Synergetic Innovation, Center for Quantum Effects and Applications, Hunan Normal UniversityDepartment of Physics and Synergetic Innovation, Center for Quantum Effects and Applications, Hunan Normal UniversityAbstract We establish a phenomenological inflation model in this paper and find that the predicted values of the spectral index and the tensor-to-scalar ratio are well consistent with the results from the Planck 2018 survey and the BICEP/Keck array measurement, significantly improving the theoretical precision in describing the early universe’s inflationary process. After inflation, we find that preheating can occur from the tachyonic instability or the parametric resonance, which depends on the value of one of model parameters.https://doi.org/10.1140/epjc/s10052-024-13728-z
spellingShingle Li-Yang Chen
Hongwei Yu
Puxun Wu
A model of inflation consistent with Planck 2018 and BICEP/Keck data
European Physical Journal C: Particles and Fields
title A model of inflation consistent with Planck 2018 and BICEP/Keck data
title_full A model of inflation consistent with Planck 2018 and BICEP/Keck data
title_fullStr A model of inflation consistent with Planck 2018 and BICEP/Keck data
title_full_unstemmed A model of inflation consistent with Planck 2018 and BICEP/Keck data
title_short A model of inflation consistent with Planck 2018 and BICEP/Keck data
title_sort model of inflation consistent with planck 2018 and bicep keck data
url https://doi.org/10.1140/epjc/s10052-024-13728-z
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