Neutrino Emission From Inhomogeneous Pion Condensed Quark Matter

Neutrino Emission From Inhomogeneous Pion Condensed Quark Matter
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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:
Int. J. Mod. Phys. E
影响因子:
--
通讯作者:
Xu-guang Huang
Xu-guang Huang
中科院分区:
其他
文献类型:
--
作者:
Peng-fei Zhuang;Qun Wang;Xu-guang Huang

文献摘要

参考文献

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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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