Dark matter seeding and the kinematics and rotation of neutron stars

被引：32

作者：

Perez-Garcia, M. Angeles ^{[1
,2
]}

Silk, Joseph ^{[3
,4
,5
]}

机构：

[1] Univ Salamanca, Dept Fis Fundamental, E-37008 Salamanca, Spain

[2] Univ Salamanca, IUFFyM, E-37008 Salamanca, Spain

[3] UPMC, Inst Astrophys, F-75014 Paris, France

[4] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA

[5] Univ Oxford, Beecroft Inst Particle Astrophys & Cosmol, Oxford OX1 3RH, England

来源：

PHYSICS LETTERS B | 2012年 / 711卷 / 01期

关键词：

VELOCITY VECTORS; ALIGNMENT; STRANGE; QUARK; KICKS;

D O I：

10.1016/j.physletb.2012.03.065

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Self-annihilation of dark matter accreted from the galactic halo in the inner regions of neutron stars may significantly affect their kinematical properties, namely velocity kicks and rotation patterns. We find that if a stable long-lived single or multiple strangelet off-center seed forms leading to an asymmetric ejection of matter and radiation, there is a significant modification in linear and angular momentum observables of the star. (C) 2012 Elsevier B.V. All rights reserved.

引用

页码：6 / 9

页数：4

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