Corpus ID: 220666156

Thermodynamical description of hot rapidly rotating neutron stars and neutron stars merger remnant

@inproceedings{Koliogiannis2020ThermodynamicalDO,
  title={Thermodynamical description of hot rapidly rotating neutron stars and neutron stars merger remnant},
  author={P. S. Koliogiannis and Ch.C. Moustakidis},
  year={2020}
}
The prediction of the equation of state of hot dense nuclear matter is one of the most complicated and interesting problems in Nuclear Astrophysics. At the same time, its knowledge is the basic ingredient for some of the most interesting studies. In the present work we concentrate our study on the construction of the equation of state of hot dense nuclear matter, related mainly to the interior of the neutron star core. We employ a theoretical nuclear model, which includes momentum dependent… CONTINUE READING

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