Temperature Evolution of Neutron Stars

Tagesse, Teka; Tolu, Biressa; Abdisa, Tessema

dc.contributor.author	Tagesse, Teka
dc.contributor.author	Tolu, Biressa
dc.contributor.author	Abdisa, Tessema
dc.date.accessioned	2023-10-04T08:31:57Z
dc.date.available	2023-10-04T08:31:57Z
dc.date.issued	2022-05
dc.identifier.uri	https://repository.ju.edu.et//handle/123456789/8489
dc.description.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	en_US
dc.language.iso	en	en_US
dc.subject	Neutron Star	en_US
dc.subject	Temperatur	en_US
dc.subject	Compact objects	en_US
dc.title	Temperature Evolution of Neutron Stars	en_US
dc.type	Thesis	en_US