Abstract:
Thermal evolution of neutron stars(NSs) is one of the active research areas in astrophysics. In this thesis we focused on the temperature evolution of the NSs where energy
conservation and transformation, mainly derived from the General relativistic TolmanOppenheimer-Volko (TOV) based evolutionary models were considered. In the energy
transformation process, cooling of the star via electromagnetic emission in terms of luminosity is used in tracking the evolutionary scenario of the star. Mathematica 13 was
used for the computation and also for observational data process in the analysis. The
plots of the theoretical results by pattern are similar with that of the observational data.
However, a detailed analysis with ne data sets and boundary conditions are needed in
the future for better analysis and progress
