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 in | Research in astronomy and astrophysics Vol. 10; no. 6; pp. 495 - 528 |
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Main Author | |
Format | Journal Article |
Language | English |
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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Online Access | Get full text |
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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. |
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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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Publisher | IOP Publishing 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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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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