Diquark condensates and compact star cooling

被引：123

作者：

Blaschke, D

Klähn, T

Voskresensky, DN

机构：

[1] Univ Rostock, D-18051 Rostock, Germany

[2] Moscow Engn Phys Inst, Moscow 115409, Russia

来源：

ASTROPHYSICAL JOURNAL | 2000年 / 533卷 / 01期

关键词：

stars : evolution; stars : neutron; pulsars : general;

D O I：

10.1086/308664

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The effect of color superconductivity on the cooling of quark stars and neutron stars with large quark cores is investigated. Various known and new quark-neutrino processes are studied. As a result, stars in the color-flavor-locked color superconducting phase cool down extremely fast. Quark stars with no crust cool down too rapidly, in disagreement with X-ray data. The cooling of stars in the N-f = 2 color superconducting phase with a crust is compatible with existing X-ray data. In addition, the cooling histories of stars with hypothetical pion condensate nuclei and a crust do not contradict the data.

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收藏

页码：406 / 412

页数：7

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