中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
The Energy-loss Rate of Neutrinos in the Urca Process of Strange Quark Matter in Weak and Ultra-strong Magnetic Fields

文献类型:期刊论文

作者Zheng Xiaoping1; Liu Xuewen2; Kang Miao1; Yu Yunwei1; Zhou Xia1
刊名Chinese Astronomy and Astrophysics
出版日期2007
卷号31期号:1页码:1
ISSN号0275-1062
英文摘要The influence of magnetic field on the energy-loss rate of neutrinos in the direct Urca process of quarks in the model of strange stars is investigated in this article. First, an improvement is made on the method of approximate calculation in the case of weak field, which can be extended to other processes of weak interactions. Then, a rigorous calculation is made for ultra-strong magnetic fields, of the energy-loss rate of neutrinos in the Urca process. The result shows that the emissivity strongly depends on the magnetic field, being directly proportional to the square of the magnetic field strength. More importantly, the dependence on temperature is different in the cases of strong and weak or null magnetic fields.
语种英语
源URL[http://libir.pmo.ac.cn/handle/332002/30149]  
专题中国科学院紫金山天文台
作者单位1.Institute of Astrophysics, Huazhong Normal University
2.中国科学院紫金山天文台
推荐引用方式
GB/T 7714
Zheng Xiaoping,Liu Xuewen,Kang Miao,et al. The Energy-loss Rate of Neutrinos in the Urca Process of Strange Quark Matter in Weak and Ultra-strong Magnetic Fields[J]. Chinese Astronomy and Astrophysics,2007,31(1):1.
APA Zheng Xiaoping,Liu Xuewen,Kang Miao,Yu Yunwei,&Zhou Xia.(2007).The Energy-loss Rate of Neutrinos in the Urca Process of Strange Quark Matter in Weak and Ultra-strong Magnetic Fields.Chinese Astronomy and Astrophysics,31(1),1.
MLA Zheng Xiaoping,et al."The Energy-loss Rate of Neutrinos in the Urca Process of Strange Quark Matter in Weak and Ultra-strong Magnetic Fields".Chinese Astronomy and Astrophysics 31.1(2007):1.

入库方式: OAI收割

来源:紫金山天文台

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