Mentor
Joseph Moscoso, University of North Carolina at Chapel Hill
Gema P. Villegas, Florida International University
Publication Date
2024
Document Type
Paper
DOI
10.25776/x1y8-7e58
Pages
1-6 pp.
Abstract
Understanding neutron star structures is crucial for advancing astrophysical research. This study explores the structure of neutron stars using advanced equations, including the Tolman-Oppenheimer-Volkoff (TOV) equations, and various equations of state (EoS). We investigate the mass-radius relationship, stability criteria, and cooling mechanisms. Key findings highlight the impact of relativistic corrections and rotational effects on neutron star properties. The results demonstrate how integrating these advanced equations enhances the understanding of neutron star behavior and stability. This research provides a comprehensive framework for analyzing neutron star structures, with implications for future astrophysical studies.
Repository Citation
Sameh, Sohila, "Analysis of Neutron Star Structure and Equation of State Using Computational Simulations" (2024). 2024 REYES Proceedings. 13.
https://digitalcommons.odu.edu/reyes-2024/13