期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 452, 期 1, 页码 540-548出版社
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stv1293
关键词
dense matter; equation of state; neutrinos; stars: neutron
资金
- Dynasty Foundation
- Foundation for Support of Education and Science (Alferov's Foundation)
- Russian Foundation for Basic Research [14-02-00868-a, 13-02-12017-ofi-M]
- 'NewCompStar', COST Action [MP1304]
We apply our recently suggested statistical approach to thermal evolution of isolated neutron stars and accreting quasi-stationary neutron stars in X-ray transients for constraining the position and relative broadening a of the direct Urca threshold of powerful neutrino emission in neutron star cores. We show that most likely explanation of observations corresponds to alpha approximate to 0.08-0.10 and to the neutron star mass, at which the direct Urca process is open, M-D approximate to 1.6-1.8 M-circle dot.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据