Thermodynamical Aspects of Some Cosmological Models
Tanima Duary

TL;DR
This thesis investigates the thermodynamic properties of various cosmological models, including dark energy and scalar-tensor theories, to assess their stability and compatibility with thermodynamic laws in explaining cosmic acceleration.
Contribution
It provides a comprehensive thermodynamic analysis of multiple cosmological models, including quintessence, Brans-Dicke, and reconstructed dark energy models, highlighting their stability and physical viability.
Findings
Certain dark energy models satisfy the Generalized Second Law
Brans-Dicke models show thermodynamic consistency under specific conditions
The $ ext{Λ}$CDM-like model demonstrates thermodynamic stability
Abstract
The research work in the thesis is focused on the thermodynamic analysis of cosmological models, especially the models that explain late-time cosmic acceleration. According to the cosmological principle, the universe is spatially homogeneous and isotropic. FRW metric is considered to describe it. In the initial chapter, an overview of cosmology is presented. Chapter 2 delves into thermodynamics applied to cosmology, emphasizing the Generalized Second Law. It thoroughly covers Hayward-Kodama temperature and discusses the apparent horizon and the conditions for thermodynamic stability. Chapter 3 presents a thermodynamic comparison of quintessence models, focusing on thawing and freezing scenarios. Chapter 4 examines Brans-Dicke cosmological models in a spatially isotropic and homogeneous universe, assessing their compatibility with the Generalized Second Law of Thermodynamics. Chapter 5…
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Taxonomy
TopicsCosmology and Gravitation Theories · Solar and Space Plasma Dynamics · Relativity and Gravitational Theory
