Cosmological Constraints on f(T,B) Gravity from Observations of Early and Late Universe

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Main Authors: Al-Omar, Yahia, Nahili, Majida, Chamoun, Nidal
Format: Preprint
Published: 2026
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author Al-Omar, Yahia
Nahili, Majida
Chamoun, Nidal
author_facet Al-Omar, Yahia
Nahili, Majida
Chamoun, Nidal
contents We present a unified framework that combines early- and late-Universe observations to constrain three functional realizations of f(T,B) gravity: the linear, quadratic, and general power-law models. First, constraints on deviations from the standard weak interaction freeze-out temperature are derived using the most recent measurements of the primordial helium-4 mass fraction. Second, we perform a joint analysis incorporating five priors: Type Ia supernovae, baryon acoustic oscillations, cosmic chronometers, Big Bang Nucleosynthesis, and Cosmic Microwave Background in order to place bounds on the model parameters. The joint likelihood analysis significantly tightens the constraints compared to individual datasets. Third, we test the null, strong, and dominant energy conditions to evaluate the physical viability of the best-fit solutions across the cosmic redshift range. Our results show that all three f(T,B) models are consistent with current observations and exhibit stable behavior under the energy-condition criteria, supporting torsion-boundary modified gravity as a robust and viable alternative to General Relativity.
format Preprint
id arxiv_https___arxiv_org_abs_2601_14729
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Cosmological Constraints on f(T,B) Gravity from Observations of Early and Late Universe
Al-Omar, Yahia
Nahili, Majida
Chamoun, Nidal
Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
We present a unified framework that combines early- and late-Universe observations to constrain three functional realizations of f(T,B) gravity: the linear, quadratic, and general power-law models. First, constraints on deviations from the standard weak interaction freeze-out temperature are derived using the most recent measurements of the primordial helium-4 mass fraction. Second, we perform a joint analysis incorporating five priors: Type Ia supernovae, baryon acoustic oscillations, cosmic chronometers, Big Bang Nucleosynthesis, and Cosmic Microwave Background in order to place bounds on the model parameters. The joint likelihood analysis significantly tightens the constraints compared to individual datasets. Third, we test the null, strong, and dominant energy conditions to evaluate the physical viability of the best-fit solutions across the cosmic redshift range. Our results show that all three f(T,B) models are consistent with current observations and exhibit stable behavior under the energy-condition criteria, supporting torsion-boundary modified gravity as a robust and viable alternative to General Relativity.
title Cosmological Constraints on f(T,B) Gravity from Observations of Early and Late Universe
topic Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2601.14729