A Brief Review on Primordial Black Holes as Dark Matter

被引：112

作者：

Villanueva-Domingo, Pablo ^{[1
]}

Mena, Olga ^{[1
]}

Palomares-Ruiz, Sergio ^{[1
]}

机构：

[1] CSIC Univ Valencia, Inst Fis Corpuscular IFIC, Paterna, Spain

来源：

FRONTIERS IN ASTRONOMY AND SPACE SCIENCES | 2021年 / 8卷

基金：

欧盟地平线“2020”;

关键词：

primordial black holes; dark matter; cosmology; accretion; 21 cm cosmology; gravitational waves; cosmic microwave background; microlensing; ADVECTION-DOMINATED ACCRETION; ABSORPTION PROFILE; LIMITS; CONSTRAINTS; ABUNDANCE; EVAPORATION; SCENARIO; SPECTRA; SYSTEMS; MODELS;

D O I：

10.3389/fspas.2021.681084

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Primordial black holes (PBHs) represent a natural candidate for one of the components of the dark matter (DM) in the Universe. In this review, we shall discuss the basics of their formation, abundance and signatures. Some of their characteristic signals are examined, such as the emission of particles due to Hawking evaporation and the accretion of the surrounding matter, effects which could leave an impact in the evolution of the Universe and the formation of structures. The most relevant probes capable of constraining their masses and population are discussed.

引用

页数：10

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