Quiescent luminosities of accreting neutron stars with different equation of states

@article{Liu2021QuiescentLO,
  title={Quiescent luminosities of accreting neutron stars with different equation of states},
  author={Helei Liu and Akira Dohi and Masa‐aki Hashimoto and Yasuhide Matsuo and Guoliang L{\"u} and Tsuneo Noda},
  journal={Physical Review D},
  year={2021},
  volume={103},
  pages={063009}
}
We model the quiescent luminosity of accreting neutron stars with several equation of states (EOSs), including the effect of pion condensation and superfluidity. As a consequence of comparison with the observations, we show that the results with Togashi EOS (the strong direct Urca process is forbidden) and TM1e EOS (mass at direct Urca process is $2.06\text{ }\text{ }{M}_{\ensuremath{\bigodot}}$) can explain the observations well by considering pion condensation and the effect of superfluidity… Expand

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