中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
On the Neutrino Radiation of Neutron Stars

文献类型:期刊论文

作者Li, Rong-Hong1; Xu, Die2; Wang, Hui1
刊名ASTRONOMISCHE NACHRICHTEN
出版日期2025-07-22
页码8
关键词direct Urca process magnetic field effects modified Urca process neutrino radiation neutron stars superfluidity and superconductivity thermal evolution
ISSN号0004-6337
DOI10.1002/asna.70038
产权排序2
通讯作者Wang, Hui(gjwang@my.swjtu.edu.cn)
英文摘要The paper first meticulously analyzes the primary mechanisms of neutrino generation within neutron stars, namely the direct Urca process and the modified Urca process, elucidates the computational methods for neutrino radiation rates, including the physical mechanisms of weak interactions, applications of quantum field theory, and complex mathematical integration techniques. Additionally, it comprehensively investigates various critical factors affecting neutron star cooling processes, such as the inhibitory effect of superfluidity and superconductivity on neutrino emission rates, the anisotropic impact of strong magnetic fields on neutrino radiation, the modulating effect of baryon density on neutrino emission rates, and how these factors alter the cooling curves and observational characteristics of neutron stars. Finally, based on the existing research findings, the paper outlines future research directions in the field of neutron star thermal evolution, emphasizing the importance of enhancing the measurement accuracy of neutron star cooling curves, delving into neutrino radiation mechanisms under extreme physical conditions, and exploring potential new physical phenomena within neutron stars, such as quark matter. These studies will not only refine the physical models of neutron stars but also propel the broader field of astrophysics, offering new perspectives and insights into extreme physical conditions and fundamental interactions in the universe.
资助项目National Natural Science Foundation of China ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region[2022A03013-1] ; Natural Science Foundation of Xinjiang Uygur Autonomous Region[2022D01A155] ; Natural Science Foundation of Xinjiang Uygur Autonomous Region[2022D01B218] ; NSFC[12373114] ; Scientific and Technological Innovation Programs of Higher Education Institutions in Shanxi[2021L483] ; [12288102]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001532856700001
出版者WILEY-V C H VERLAG GMBH
资助机构National Natural Science Foundation of China ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; Natural Science Foundation of Xinjiang Uygur Autonomous Region ; NSFC ; Scientific and Technological Innovation Programs of Higher Education Institutions in Shanxi
源URL[http://ir.xao.ac.cn/handle/45760611-7/7959]  
专题脉冲星研究团组
通讯作者Wang, Hui
作者单位1.Yuncheng Univ, Shanxi Prov Intelligent Optoelect Sensing Applicat, Yuncheng, Shanxi, Peoples R China
2.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi, Xinjiang, Peoples R China
推荐引用方式
GB/T 7714
Li, Rong-Hong,Xu, Die,Wang, Hui. On the Neutrino Radiation of Neutron Stars[J]. ASTRONOMISCHE NACHRICHTEN,2025:8.
APA Li, Rong-Hong,Xu, Die,&Wang, Hui.(2025).On the Neutrino Radiation of Neutron Stars.ASTRONOMISCHE NACHRICHTEN,8.
MLA Li, Rong-Hong,et al."On the Neutrino Radiation of Neutron Stars".ASTRONOMISCHE NACHRICHTEN (2025):8.

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来源:新疆天文台

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