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Thermal structures of accreting neutron stars with neutrino losses due to strong pion condensations

Quiescent X-ray luminosities are presented in low mass X-ray binaries with use of evolutionary calculations. The calculated luminosities are compared with observed ones in terms of timeaveraged mass accretion rate. It is shown that neutrino emission by strong pion condensation can explain quiescent X-ray luminosity of SAX J1808.4-3658 and we do not need direct Urca processes concerning nucleons and/or hyperons.

preprint2016arXivOpen access
Yasuhide MatsuoMasa-aki HashimotoKoutarou HayashidaHelei LiuTsuneo NodaMasayuki Y. Fujimoto
astro-ph.HE
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Open access6 authors1 topic
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Yasuhide MatsuoMasa-aki HashimotoKoutarou HayashidaHelei LiuTsuneo NodaMasayuki Y. Fujimoto

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