Deconfinement Phase Transition Heating and Thermal Evolution of Neutron Stars

摘要：

The deconfinement phase transition will lead to the release of latent heat during spins down of neutron stars if the transition is the first-order one. We have investigated the thermal evolution of neutron stars undergoing such deconfinement phase transition. The results show that neutron stars may be heated to higher temperature. This feature could be particularly interesting for high temperature of low- magnetic field millisecond pulsar at late stage.

关键词： dense matter-equation of state-stars evolution-stars neutron-stars rotation

作者: Miao Kang Nana Pan Xiaodong Wang

作者单位: The college of physics and electron, Henan university, Kaifeng, 475004, Henan, P. R. China The insti The institute of astrophysics, Huazhong normal university, Wuhan, 430079, Hubei, P. R. China

会议类型: 国际会议

会议名称: 紧凑型物体的天体物理学国际会议(International Conference on Astrophysics of Compact Objects)

会议地点: 安徽黄山

会议语种:英文

页码: 203-205

在线出版日期: 2007-07-01（万方平台首次上网日期，不代表论文的发表时间）