Formation of superdense dark matter lumps at the radiation-dominated cosmological stage

被引：0
|
作者：
V. S. Berezinsky
V. I. Dokuchaev
Yu. N. Eroshenko
机构：
[1] Laboratori Nazionali del Gran Sasso,INFN
[2] RAS,Institute for Nuclear Research
来源：
Gravitation and Cosmology | 2012年 / 18卷
关键词：
Cosmic String; Gravitational Wave Detector; Primordial Black Hole; String Loop; Perturbation Spectrum;
D O I：
暂无
中图分类号：
学科分类号：
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
收藏
页码：57 / 60
页数：3
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