Big Bang Nucleosynthesis constraints on f(T,T) gravity

Big Bang Nucleosynthesis provides us with an observational insight into the very early Universe. Since this mechanism of light element synthesis comes out of the standard model of particle cosmology which follows directly from General Relativity, it is expected that any modifications to GR will resu...

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Main Authors: Sai Swagat Mishra, Ameya Kolhatkar, P.K. Sahoo
Format: Article
Language:English
Published: Elsevier 2024-01-01
Series:Physics Letters B
Subjects:
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269323007244
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author Sai Swagat Mishra
Ameya Kolhatkar
P.K. Sahoo
author_facet Sai Swagat Mishra
Ameya Kolhatkar
P.K. Sahoo
author_sort Sai Swagat Mishra
collection DOAJ
description Big Bang Nucleosynthesis provides us with an observational insight into the very early Universe. Since this mechanism of light element synthesis comes out of the standard model of particle cosmology which follows directly from General Relativity, it is expected that any modifications to GR will result in deviations in the predicted observable parameters which are mainly, the neutron-to-proton ratio and the baryon-to-photon ratio. We use the measured neutron-to-proton ratio and compare the theoretically obtained expressions to constrain two models in the framework of f(T,T) gravity. The theoretically constrained models are then tested against observational data from the Hubble dataset and the ΛCDM model to explain the accelerated expansion of the Universe.
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spelling doaj.art-8e2fda35083b43d49722c8c603a1117d2024-01-07T04:29:39ZengElsevierPhysics Letters B0370-26932024-01-01848138391Big Bang Nucleosynthesis constraints on f(T,T) gravitySai Swagat Mishra0Ameya Kolhatkar1P.K. Sahoo2Department of Mathematics, Birla Institute of Technology and Science-Pilani, Hyderabad Campus, Hyderabad-500078, IndiaDepartment of Mathematics, Birla Institute of Technology and Science-Pilani, Hyderabad Campus, Hyderabad-500078, IndiaCorresponding author.; Department of Mathematics, Birla Institute of Technology and Science-Pilani, Hyderabad Campus, Hyderabad-500078, IndiaBig Bang Nucleosynthesis provides us with an observational insight into the very early Universe. Since this mechanism of light element synthesis comes out of the standard model of particle cosmology which follows directly from General Relativity, it is expected that any modifications to GR will result in deviations in the predicted observable parameters which are mainly, the neutron-to-proton ratio and the baryon-to-photon ratio. We use the measured neutron-to-proton ratio and compare the theoretically obtained expressions to constrain two models in the framework of f(T,T) gravity. The theoretically constrained models are then tested against observational data from the Hubble dataset and the ΛCDM model to explain the accelerated expansion of the Universe.http://www.sciencedirect.com/science/article/pii/S0370269323007244Big Bang NucleosynthesisNeutron abundanceEarly cosmologyf(T,T) gravity
spellingShingle Sai Swagat Mishra
Ameya Kolhatkar
P.K. Sahoo
Big Bang Nucleosynthesis constraints on f(T,T) gravity
Physics Letters B
Big Bang Nucleosynthesis
Neutron abundance
Early cosmology
f(T,T) gravity
title Big Bang Nucleosynthesis constraints on f(T,T) gravity
title_full Big Bang Nucleosynthesis constraints on f(T,T) gravity
title_fullStr Big Bang Nucleosynthesis constraints on f(T,T) gravity
title_full_unstemmed Big Bang Nucleosynthesis constraints on f(T,T) gravity
title_short Big Bang Nucleosynthesis constraints on f(T,T) gravity
title_sort big bang nucleosynthesis constraints on f t t gravity
topic Big Bang Nucleosynthesis
Neutron abundance
Early cosmology
f(T,T) gravity
url http://www.sciencedirect.com/science/article/pii/S0370269323007244
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