Um estudo sobre a evolução térmica das estrelas de nêutrons.
This work consists of a study about the Thermal Evolution of neutron stars, through bibliographic survey, modeling and computing of the cooling of these stars. Cooling calculations are sensitive to the adopted state equation (EOS) nuclear model, and other characteristics of the structure and comp...
| Autor principal: | Oliveira, Klemilton Murilo Veloso |
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| Grau: | Monografia |
| Idioma: | pt_BR |
| Publicado em: |
Universidade Federal do Tocantins
2023
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| Assuntos: | |
| Acesso em linha: |
http://hdl.handle.net/11612/4591 |
| Resumo: |
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This work consists of a study about the Thermal Evolution of neutron stars, through bibliographic
survey, modeling and computing of the cooling of these stars. Cooling calculations are sensitive
to the adopted state equation (EOS) nuclear model, and other characteristics of the structure and
composition of neutron stars. The study of thermal evolution is a great tool to test neutron star
models, since it depends on the structure and composition considered. In addition, the study of
cooling can help us in better understanding especially in high densities and low temperature
regimens (a regime that is currently out of reach of terrestrial experiments). |