Research Article
Modeling the Thermodynamics of Neutron Stars: Insights from Statistical Mechanics
Diriba Gonfa Tolasa*
,
Adugna Terecha Furi
Issue:
Volume 13, Issue 1, March 2025
Pages:
1-10
Received:
25 December 2024
Accepted:
16 January 2025
Published:
11 February 2025
DOI:
10.11648/j.ijass.20251301.11
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Views:
Abstract: This paper explores the thermodynamic properties of neutron stars through the lens of statistical mechanics. Neutron stars, the remnants of massive stellar explosions, exhibit extreme physical conditions that challenge our understanding of matter under such densities. This paper investigates the thermodynamic properties of neutron stars using statistical mechanics as a framework. A comprehensive literature review, is conducted highlighting key findings from previous studies on the equation of state and thermal behavior of neutron stars. The methodology employed integrates both numerical simulations and analytical approaches to model the thermodynamic states of neutron stars, taking into account various parameters such as density, temperature, and pressure. Advanced numerical techniques, including finite difference methods and Monte Carlo simulations, alongside analytical derivations to provide a robust understanding of the underlying physics. Results from analysis reveal significant correlations between density and pressure, as well as the impact of temperature on specific heat capacity. These findings are illustrated through several plots and tables, showcasing the relationships between key thermodynamic variables. The discussion section elaborates on the implications of our results for the stability and cooling mechanisms of neutron stars, emphasizing how our insights contribute to the broader field of astrophysics. This work not only enhances our understanding of neutron star thermodynamics but also sets the stage for future research into the behavior of matter under extreme conditions. We introduce a novel methodology for modeling the equations of state (EoS) that govern neutron stars, enhancing our understanding of their stability and structure under extreme conditions. Utilizing numerical simulations, are analyze the relationships between pressure, density, temperature, and energy density. The results are significant for developing astrophysical models that elucidate neutron star formation and evolution.
Abstract: This paper explores the thermodynamic properties of neutron stars through the lens of statistical mechanics. Neutron stars, the remnants of massive stellar explosions, exhibit extreme physical conditions that challenge our understanding of matter under such densities. This paper investigates the thermodynamic properties of neutron stars using stati...
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