New cosmological constraints on primordial black holes

被引：886

作者：

Carr, B. J. ^{[1
,2
,3
]}

Kohri, Kazunori ^{[4
,5
,6
]}

Sendouda, Yuuiti ^{[7
,8
]}

Yokoyama, Junichi ^{[2
,9
]}

机构：

[1] Queen Mary Univ London, Astron Unit, London E1 4NS, England

[2] Univ Tokyo, Grad Sch Sci, Res Ctr Early Universe, Tokyo 1130033, Japan

[3] Univ Toronto, Canadian Inst Theoret Astrophys, Toronto, ON M5S 1A1, Canada

[4] Tohoku Univ, Dept Phys, Sendai, Miyagi 9808578, Japan

[5] Univ Lancaster, Dept Phys, Lancaster LA1 4YB, England

[6] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA

[7] Kyoto Univ, Yukawa Inst Theoret Phys, Kyoto 6068502, Japan

[8] Univ Tokyo, Grad Sch Sci, Dept Phys, Tokyo 1130033, Japan

[9] Univ Tokyo, Inst Phys & Math Universe, Chiba 2778568, Japan

来源：

PHYSICAL REVIEW D | 2010年 / 81卷 / 10期

关键词：

GAMMA-RAY BURSTS; PARTICLE-EMISSION RATES; 1ST-ORDER PHASE-TRANSITIONS; SELF-SIMILAR GROWTH; GLUON-JET EMISSION; DARK-MATTER; COSMIC-RAYS; DENSITY PERTURBATIONS; GRAVITATIONAL-WAVES; HELIUM ABUNDANCE;

D O I：

10.1103/PhysRevD.81.104019

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We update the constraints on the fraction of the Universe going into primordial black holes in the mass range 10(9)-10(17) g associated with the effects of their evaporations on big bang nucleosynthesis and the extragalactic photon background. We include for the first time all the effects of quark and gluon emission by black holes on these constraints and account for the latest observational developments. We then discuss the other constraints in this mass range and show that these are weaker than the nucleosynthesis and photon background limits, apart from a small range 10(13)-10(14) g, where the damping of cosmic microwave background anisotropies dominates. Finally we review the gravitational and astrophysical effects of nonevaporating primordial black holes, updating constraints over the broader mass range 1-10(50) g.

引用

页数：33

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