Dark spiky primordial black holes

被引:1
|
作者
Ireland, Aurora [1 ]
机构
[1] Univ Chicago, Dept Phys, Chicago, IL 60637 USA
关键词
DYNAMICAL FRICTION; BINARY; ACCRETION; GROWTH; MASS;
D O I
10.1103/PhysRevD.111.023513
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Recent observations of two nearby black hole low-mass x-ray binaries have suggested possible indication of dark matter density spikes. While the evidence is compelling, one issue with this interpretation is that light black holes formed from stellar collapse are not expected to form dark matter spikes, and so it is unclear how the stellar-mass black holes in these binaries could have acquired such features. Since primordial black holes are expected to form ultradense dark matter minispikes, in this article we explore the possibility of a primordial origin for these light black holes.
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页数:12
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