H0 tension in torsion-based modified gravity

被引：24

作者：

Mandal, Sanjay ^{[1
]}

Sokoliuk, Oleksii ^{[2
,3
]}

Mishra, Sai Swagat ^{[4
]}

Sahoo, P. K. ^{[1
,4
]}

机构：

[1] Transilvania Univ Brasov, Fac Math & Comp Sci, Eroilor 29, Brasov, Romania

[2] Natl Acad Sci Ukraine, Main Astron Observ, 27 Akad Zabolotny St, UA-03143 Kiev, Ukraine

[3] Taras Shevchenko Natl Univ Kyiv, Astron Observ, 3 Observatorna St, UA-04053 Kiev, Ukraine

[4] Birla Inst Technol & Sci Pilani, Dept Math, Hyderabad Campus, Hyderabad 500078, India

来源：

NUCLEAR PHYSICS B | 2023年 / 993卷

关键词：

PROBE WMAP OBSERVATIONS; LUMINOUS RED GALAXIES; CONSTRAINTS; SCALE; PARAMETER; LAMBDA; F(R; CMB;

D O I：

10.1016/j.nuclphysb.2023.116285

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

The rising concern in the Hubble constant tension (H-0 tension) of the cosmological models motivates the scientific community to search for alternative cosmological scenarios that could resolve the H-0 tension. In this regard, we aim to work on a torsion-based modified theory of gravity which is an alternative description to the coherence model. We solve numerically for the Hubble parameter using two exponential Lagrangian functions of torsion T and a trace of energy-momentum tensor T for the dust case. Further, we constrain the cosmological and model parameters; to do that, we use Hubble, SNe Ia, Baryon Acoustic Oscillations, Cosmic Microwave Background samples, and Markov Chain Monte Carlo (MCMC) simulation through Bayesian statistics. We obtain the values of Hubble constant H-0 for our model, and the outputs align with the recent observational measurements of H-0. In addition, we check the deviation of our results from model-independent measurements of H-0 from Planck2018, SH0ES, and H0LiCOW experiments. In contrast, our finding partially solved the H-0 tension but gave a new possible direction to alleviate the H-0 tension.(c) 2023 The Author(s). Published by Elsevier B. V. This is an open access article under the CCBY license (http://creativecommons.org/licenses/by/4.0/).

引用

页数：15

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