Formation of Superdense Dark Matter Lumps at the Radiation-Dominated Cosmological Stage

被引：5

作者：

Berezinsky, V. S. ^{[1
]}

Dokuchaev, V. I. ^{[2
]}

Eroshenko, Yu N. ^{[2
]}

机构：

[1] Ist Nazl Fis Nucl, Lab Nazl Gran Sasso, I-67010 Assergi, AQ, Italy

[2] RAS, Inst Nucl Res, Moscow 117312, Russia

来源：

GRAVITATION & COSMOLOGY | 2012年 / 18卷 / 01期

关键词：

PRIMORDIAL BLACK-HOLES;

D O I：

10.1134/S0202289312010045

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We study the process of superdense dark matter clump (DMC) formation at the radiation-dominated stage of the Universe. High-magnitude density perturbations that lead to DMC formation can be peaks in the inflationary perturbation spectrum or closed loops of cosmic strings. A model with superdense DMCs provides new opportunities for annihilation of particles having small annihilation cross-sections. Superdense DMCs can be detected by their tidal effect on gravitational wave detectors.

引用

页码：57 / 60

页数：4

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