Thermal neutron stars including the hyperon-hyperon interactions
Yu, Z3; Liu, GZ; Zhu, MF; Yan-Xu; Zhao, EG
2010
会议日期AUG 16-21, 2009
会议地点Beijing, PEOPLES R CHINA
关键词DOUBLE HYPERFRAGMENT
卷号834
期号1-4
DOI10.1016/j.nuclphysa.2010.01.029
页码97C-99C
英文摘要At finite temperature systems with the hyperon-hyperon(W) interactions are investigated within the framework of the RN4FT. With the weak YY interaction, the maximum strangeness content for bound strange hadronic matter decreases with the increase of temperature, if the temperature exceeds 21MeV, strange hadronic matter does not have bound state, while with the strong YY interaction the highest temperature is 30MeV. There is a, highest temperature limit(40MeV) for stable neutron stars, which is independent on the choose of the YY interactions. The maximum mass with the weak YY interaction (1.75M circle dot) is consistent with the mass constraint.
会议录NUCLEAR PHYSICS A
会议录出版者ELSEVIER SCIENCE BV
会议录出版地AMSTERDAM
语种英语
URL标识查看原文
ISSN号0375-9474
WOS研究方向Physics
内容类型会议论文
源URL[http://ir.itp.ac.cn/handle/311006/23635]  
专题SCI会议论文
作者单位1.Nanjing Forest Univ, Coll Sci, Nanjing 210037, Peoples R China
2.Chinese Acad Sci, Inst Theoret Phys, Beijing 100080, Peoples R China
3.Jilin Univ, Coll Phys, Changchun 130023, Peoples R China
推荐引用方式
GB/T 7714
Yu, Z,Liu, GZ,Zhu, MF,et al. Thermal neutron stars including the hyperon-hyperon interactions[C]. 见:. Beijing, PEOPLES R CHINA. AUG 16-21, 2009.
个性服务
查看访问统计
相关权益政策
暂无数据
收藏/分享
所有评论 (0)
暂无评论
 

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。


©版权所有 ©2017 CSpace - Powered by CSpace