Primordial black holes

Primordial black holes (PBHs) are a profound signature of primordial cosmological structures and provide a theoretical tool to study nontrivial physics of the early Universe. The mechanisms of PBH formation are discussed and observational constraints on the PBH spectrum, or effects of PBH evaporatio...

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Published inResearch in astronomy and astrophysics Vol. 10; no. 6; pp. 495 - 528
Main Author Khlopov, Maxim Yu
Format Journal Article
LanguageEnglish
Published IOP Publishing 01.06.2010
Centre for Cosmoparticle Physics "Cosmion" Kashirskoe Sh., 31, Moscow 115409, Russia
National Research Nuclear University "Moscow Engineering Physics Institute," Kashirskoe Sh.,31, Moscow
APC laboratory 10, rue Alice Domon et Léonie Duquet 75205 Paris Cedex 13,France
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Abstract Primordial black holes (PBHs) are a profound signature of primordial cosmological structures and provide a theoretical tool to study nontrivial physics of the early Universe. The mechanisms of PBH formation are discussed and observational constraints on the PBH spectrum, or effects of PBH evaporation, are shown to restrict a wide range of particle physics models, predicting an enhancement of the ultraviolet part of the spectrum of density perturbations, early dust-like stages, first order phase transitions and stages of superheavy metastable particle dominance in the early Universe. The mechanism of closed wall contraction can lead, in the inflationary Universe, to a new approach to galaxy formation, involving primordial clouds of massive BHs created around the intermediate mass or supermassive BH and playing the role of galactic seeds.
AbstractList Primordial black holes (PBHs) are a profound signature of primordial cosmological structures and provide a theoretical tool to study nontrivial physics of the early Universe. The mechanisms of PBH formation are discussed and observational constraints on the PBH spectrum, or effects of PBH evaporation, are shown to restrict a wide range of particle physics models, predicting an enhancement of the ultraviolet part of the spectrum of density perturbations, early dust-like stages, first order phase transitions and stages of superheavy metastable particle dominance in the early Universe. The mechanism of closed wall contraction can lead, in the inflationary Universe, to a new approach to galaxy formation, involving primordial clouds of massive BHs created around the intermediate mass or supermassive BH and playing the role of galactic seeds.
Primordial black holes (PBHs) are a profound signature of primordial cosmological structures and provide a theoretical tool to study nontrivial physics of the early Universe. The mechanisms of PBH formation are discussed and observational constraints on the PBH spectrum, or effects of PBH evaporation, are shown to restrict a wide range of particle physics models, predicting an enhancement of the ultraviolet part of the spectrum of density perturbations, early dust-like stages, first order phase transitions and stages of superheavy metastable particle dominance in the early Universe. The mechanism of closed wall contraction can lead, in the inflationary Universe, to a new approach to galaxy formation, involving primordial clouds of massive BHs created around the intermediate mass or supermassive BH and playing the role of galactic seeds.
P1; Primordial black holes (PBHs) are a profound signature of primordial cos-mological structures and provide a theoretical tool to study nontrivial physics of the early Universe. The mechanisms of PBH formation are discussed and observational constraints on the PBH spectrum, or effects of PBH evaporation, are shown to re-strict a wide range of particle physics models, predicting an enhancement of the ul-traviolet part of the spectrum of density perturbations, early dust-like stages, first or-der phase transitions and stages of superheavy metastable particle dominance in the early Universe. The mechanism of closed wall contraction can lead, in the inflation-ary Universe, to a new approach to galaxy formation, involving primordial clouds of massive BHs created around the intermediate mass or supermassive BH and playing the role of galactic seeds.
Author Maxim Yu. Khlopov
AuthorAffiliation Centre for Cosmoparticle Physics "Cosmion," Kashirskoe Sh., 31, Moscow 115409, Russia National Research Nuclear University "Moscow Engineering Physics Institute," Kashirskoe Sh., 31, Moscow APC laboratory 10, rue Alice Domon et Leonie Duquet 75205 Pads Cedex 13, France
AuthorAffiliation_xml – name: Centre for Cosmoparticle Physics "Cosmion" Kashirskoe Sh., 31, Moscow 115409, Russia;National Research Nuclear University "Moscow Engineering Physics Institute," Kashirskoe Sh.,31, Moscow;APC laboratory 10, rue Alice Domon et Léonie Duquet 75205 Paris Cedex 13,France
Author_xml – sequence: 1
  fullname: Khlopov, Maxim Yu
BackLink https://in2p3.hal.science/in2p3-00294662$$DView record in HAL
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DocumentTitleAlternate Primordial black holes
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Issue 6
Keywords elementary particles
early universe
black hole physics
cosmology:theory
dark matter
Particle physics and field theory
Gravitation and cosmology
Astrophysics and astroparticles
Language English
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Centre for Cosmoparticle Physics "Cosmion" Kashirskoe Sh., 31, Moscow 115409, Russia
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Snippet Primordial black holes (PBHs) are a profound signature of primordial cosmological structures and provide a theoretical tool to study nontrivial physics of the...
P1; Primordial black holes (PBHs) are a profound signature of primordial cos-mological structures and provide a theoretical tool to study nontrivial physics of...
Primordial black holes (PBHs) are a profound signature of primordial cosmological structures and provide a theoretical tool to study nontrivial physics of the...
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SubjectTerms Astrophysics
Cosmology and Extra-Galactic Astrophysics
General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
Physics
Sciences of the Universe
中等质量
宇宙结构
密度扰动
早期宇宙
星系形成
粒子物理学
通货膨胀
Title Primordial black holes
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