Cosmological Evolution of the Universe in Torsion-based Modified Gravity
Sai Swagat Mishra

TL;DR
This paper explores torsion-based modified gravity theories, particularly f(T) and f(T,T), demonstrating their potential to resolve key cosmological tensions like H0 and S8, and linking early Universe baryogenesis with late-time acceleration.
Contribution
It introduces extended teleparallel gravity models that can alleviate cosmological tensions and connect early Universe baryogenesis with late-time cosmic acceleration.
Findings
Extended teleparallel models can better fit recent cosmological data than Lambda-CDM.
Some models outperform Lambda-CDM in explaining DESI and Union3 datasets.
Torsional gravity can reproduce observed baryon asymmetry while matching late-time expansion.
Abstract
General Relativity, despite its century-long success, faces conceptual and observational challenges, including singularities, incompatibility with quantum mechanics, and the need to introduce dark matter and dark energy. Precision cosmology has also revealed persistent tensions, notably the H0 and S8 discrepancies, which question the completeness of the standard Lambda-CDM model. This thesis investigates cosmological applications of teleparallel gravity and its extensions, focusing on f(T) and f(T,T) theories. We show that torsion-based modifications can shift late-time expansion and matter clustering, alleviating the H0 and S8 tensions. Using datasets including cosmic chronometers, baryon acoustic oscillations, Type Ia supernovae, Pantheon+SH0ES, Union3, DESI, and gravitational wave standard sirens, we perform Markov Chain Monte Carlo analyses to constrain model parameters.…
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Taxonomy
TopicsCosmology and Gravitation Theories · Computational Physics and Python Applications · Pulsars and Gravitational Waves Research
