Neutron stars with outbursts from superfluid crust

被引：2

作者：

Kaminker, A. D. ^{[1
,2
]}

Chaikin, E. A. ^{[2
]}

Kaurov, A. A. ^{[3
]}

Yakovlev, D. G. ^{[1
]}

机构：

[1] Ioffe Inst, Politech Skaya 26, St Petersburg 194021, Russia

[2] Peter Great St Petersburg Polytech Univ, Politech Skaya 29, St Petersburg 195251, Russia

[3] Inst Adv Study, 1 Einstein Dr, Princeton, NJ 08540 USA

来源：

INTERNATIONAL CONFERENCE PHYSICS OF NEUTRON STARS: 50 YEARS AFTER, 2017 | 2017年 / 932卷

基金：

俄罗斯科学基金会;

关键词：

X-RAY TRANSIENTS; EMISSION;

D O I：

10.1088/1742-6596/932/1/012047

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We model heat propagation and the thermal surface luminosity L-s(infinity) (t) of a neutron star after an internal outburst in its crust. Simulations take into account superfluidity of free neutrons and the thickness of the outbursting layer (heater) in the crust. Crustal superfluidity can shorten and intensify variations of L-s(infinity) (t).

引用

页数：5

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