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相关论文: Primordial Black Holes from QCD Axion Bubbles

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We study the formation of primordial black holes (PBHs) from the collapse of closed domain walls (DWs) which naturally arise in QCD axion models near the QCD scale together with the main string-wall network. The size distribution of the…

高能物理 - 唯象学 · 物理学 2020-01-08 Shuailiang Ge

Primordial black holes (PBHs) may be part of the dark matter. It is shown here that PBHs form more easily during cosmic phase transitions. For approximately scale-invariant primordial curvature fluctuations the PBH mass function may…

宇宙学与河外天体物理 · 物理学 2024-06-18 Karsten Jedamzik

In a recent paper we pointed out that supermassive black holes, with masses ranging from $10^5$ to $10^{10} M_\odot$ form naturally at cosmic dawn if the dark matter is QCD axions or axion-like particles with mass $m > 10^{-16}\,…

高能天体物理现象 · 物理学 2026-05-07 Pierre Sikivie , Yuxin Zhao

We argue that the existence of the cold dark matter is explained by primordial black holes.We show that a significant number of primordial black holes can be formed in an axion-like curvaton model, in which the highly blue-tilted power…

高能物理 - 唯象学 · 物理学 2013-03-22 Masahiro Kawasaki , Naoya Kitajima , Tsutomu T. Yanagida

We study the possibility of production of primordial black holes (PBHs) from bubble collisions during a first-order phase transition. While typical colliding bubbles are small and irrelevant for PBH production, we find that those that can…

高能物理 - 唯象学 · 物理学 2024-11-20 Tae Hyun Jung , Takemichi Okui

Although the dark matter is usually assumed to be some form of elementary particle, primordial black holes (PBHs) could also provide some of it. However, various constraints restrict the possible mass windows to $10^{16}$ - $10^{17}\,$g,…

宇宙学与河外天体物理 · 物理学 2020-09-08 Bernard Carr , Florian Kuhnel

Primordial Black Holes (PBHs) might have formed in the early Universe due to the collapse of density fluctuations. PBHs may act as the sources for some of the gravitational waves recently observed. We explored the formation scenarios of…

宇宙学与河外天体物理 · 物理学 2020-07-06 J. L. G. Sobrinho , P. Augusto

Primordial Black Holes (PBHs) are, typically light, black holes which can form in the early Universe. There are a number of formation mechanisms, including the collapse of large density perturbations, cosmic string loops and bubble…

广义相对论与量子宇宙学 · 物理学 2021-04-07 Anne M. Green

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…

天体物理学 · 物理学 2014-11-18 M. Yu. Khlopov

In this letter, we propose a novel scenario which simultaneously explains $\mathcal{O}(10)M_\odot$ primordial black holes (PBHs) and dark matter in the minimally supersymmetric standard model. Gravitational waves (GWs) events detected by…

宇宙学与河外天体物理 · 物理学 2018-08-22 Fuminori Hasegawa , Masahiro Kawasaki

The Primordial Black Holes (PBHs) are gradually involved into consideration as the phenomenon having reliable basis. We discuss here the possibility of their agglomeration into clusters that may have several prominent observable features.…

We study the primordial black hole (PBH) formation from Q-balls that are non-topological solitons in scalar field theories. We develop a formula for calculating the density perturbations from the Q-ball charge distribution. We also…

高能物理 - 唯象学 · 物理学 2025-11-24 Shinta Kasuya , Masahiro Kawasaki , Alexander Kusenko , Shunsuke Neda

We investigate the phenomenological consequences of axion-like particle (ALP) dark matter with an early matter domination triggered by primordial black holes (PBHs). We focus on light BHs with masses smaller than $\sim 10^9~$g which fully…

高能物理 - 唯象学 · 物理学 2022-01-05 Nicolás Bernal , Yuber F. Perez-Gonzalez , Yong Xu , Óscar Zapata

LIGO-Virgo collaboration has found black holes as heavy as $M \sim 30M_\odot$ through the detections of the gravitational waves emitted during their mergers. Primordial black holes (PBHs) produced by inflation could be an origin of such…

宇宙学与河外天体物理 · 物理学 2018-01-08 Keisuke Inomata , Masahiro Kawasaki , Kyohei Mukaida , Yuichiro Tada , Tsutomu T. Yanagida

A universal mechanism may be responsible for several unresolved cosmic conundra. The sudden drop in the pressure of relativistic matter at $W^{\pm}/Z^{0}$ decoupling, the quark--hadron transition and $e^{+}e^{-}$ annihilation enhances the…

宇宙学与河外天体物理 · 物理学 2020-12-16 Bernard Carr , Sebastien Clesse , Juan Garcia-Bellido , Florian Kuhnel

The computation of PBH (primordial black hole) production from primordial perturbations has recently been improved by considering a more accurate relation between the primordial power spectrum and the PBH mass variance. We present here…

天体物理学 · 物理学 2009-11-07 David Blais , Claus Kiefer , David Polarski

Primordial black holes (PBHs) could provide the dark matter but a variety of constraints restrict the possible mass windows to $10^{16} - 10^{17}$g, $10^{20} - 10^{24}$g and $10 - 10^3M_{\odot}$. The last possibility is of special interest…

宇宙学与河外天体物理 · 物理学 2020-01-08 Bernard Carr

We study the formation of primordial black holes (PBHs) in strongly supercooled first-order phase transitions. The mechanism is based on the presence of remnants dominated by the false vacuum that scale slower with the expansion of the…

宇宙学与河外天体物理 · 物理学 2023-09-20 Marek Lewicki , Piotr Toczek , Ville Vaskonen

Primordial black hole (PBH) formation is a more generic phenomenon than was once thought. The dynamics of a scalar field in inflationary universe can produce PBHs under mild assumptions regarding the scalar potential. In the early universe,…

宇宙学与河外天体物理 · 物理学 2019-11-04 Eric Cotner , Alexander Kusenko , Misao Sasaki , Volodymyr Takhistov

Primordial Black Holes (PBHs) have entered the forefront of theoretical cosmology, due their potential role in phenomena ranging from gravitational waves, to dark matter, to galaxy formation. While producing PBHs from inflationary…

宇宙学与河外天体物理 · 物理学 2022-01-12 Keisuke Inomata , Evan McDonough , Wayne Hu