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arXiv 0710.3634hep-phastro-phnucl-th
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非均匀π介子凝聚夸克物质的中微子发射

Neutrino Emission From Inhomogeneous Pion Condensed Quark Matter

Xuguang Huang, Qun Wang, Pengfei Zhuang

摘要:

人们认为,如果重子密度足够高,中子星内部可以存在夸克物质。当有一个大的同位旋密度时,夸克物质可能处于π凝聚相。我们计算了直接Urca过程在这样一个阶段,特别是在非均匀Larkin-Ovchinnikov-Fulde-Ferrell(LOFF)状态下的中微子发射。得到了中微子的发射率和比热,并由此估算了冷却速率。

英文摘要:

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.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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