Neutrino Emission From Inhomogeneous Pion Condensed Quark Matter
Neutrino Emission From Inhomogeneous Pion Condensed Quark Matter
复制标题
非均匀π介子凝聚夸克物质的中微子发射
DOI:
10.1142/s021830130801088x
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发表时间:
2007-10
期刊:
影响因子:
--
通讯作者:
Xu-guang Huang
中科院分区:
文献类型:
--
作者:
Peng-fei Zhuang;Qun Wang;Xu-guang Huang
It is believed that quark matter can exist in neutron star interior if the baryon density is high enough. When there is a large isospin density, quark matter could be in a pion condensed phase. We compute neutrino emission from direct Urca processes in such a phase, particularly in the inhomogeneous Larkin-Ovchinnikov-Fulde-Ferrell (LOFF) states. The neutrino emissivity and specific heat are obtained, from which the cooling rate is estimated.
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影响因子:
6.7
作者:
J. Ketterson;K. Bennemann
通讯作者:
J. Ketterson;K. Bennemann
DOI:
10.1016/0375-9474(76)90513-3
发表时间:
1976-05
期刊:
Nuclear Physics
影响因子:
--
作者:
G. Baym;S. Chin
通讯作者:
G. Baym;S. Chin
DOI:
10.1063/1.2398858
发表时间:
2006-07
期刊:
--
影响因子:
--
作者:
Qun Wang
通讯作者:
Qun Wang
影响因子:
8.6
作者:
M. Alford;C. Kouvaris;K. Rajagopal
通讯作者:
M. Alford;C. Kouvaris;K. Rajagopal
影响因子:
5
作者:
Huang, Xuguang;Zhuang, Pengfei;Wang, Qun
通讯作者:
Wang, Qun