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Phase transitions in the early universe are prime settings for the production of primordial black holes, since they can break the relatively quiescent homogeneity and isotropy of Friedmann-Robertson-Walker (FRW) cosmologies. These epochs of…

天体物理学 · 物理学 2007-05-23 Mitesh Patel , George M. Fuller

Primordial black holes (PBHs) might be formed in the early Universe and could comprise at least a fraction of the dark matter. Using the recently released GWTC-2 dataset from the third observing run of the LIGO-Virgo Collaboration, we…

广义相对论与量子宇宙学 · 物理学 2021-02-03 Kaze W. K. Wong , Gabriele Franciolini , Valerio De Luca , Vishal Baibhav , Emanuele Berti , Paolo Pani , Antonio Riotto

We consider the formation of horizon-size primordial black holes (PBH's) from pre-existing density fluctuations during cosmic phase transitions. It is pointed out that the formation of PBH's should be particularly efficient during the QCD…

天体物理学 · 物理学 2010-01-06 K. Jedamzik

In this paper, we show that if passive fluctuations are considered, primordial black holes (PBHs) can be easily produced in the framework of single-field, slow-roll inflation models. The formation of PBHs is due to the blue spectrum of…

高能物理 - 唯象学 · 物理学 2015-06-05 Chia-Min Lin , Kin-Wang Ng

Recent astronomical data on Black hole observations are reviewed. The arguments in favor that the observed black holes are predominantly primordial (PBH) are presented. The mass spectrum of PBH is best fit to the log-normal one. A model of…

宇宙学与河外天体物理 · 物理学 2021-02-03 A. D. Dolgov

Primordial black holes (PBH) can arise in a wide range of scenarios, from inflation to first-order phase transitions. Light PBHs, such as those produced during preheating, in bounce cosmologies, or at the GUT scale, could induce an early…

宇宙学与河外天体物理 · 物理学 2025-04-17 Taehun Kim , Philip Lu

Linear scalar cosmological perturbations have increasing spectra in the contracting phase of bouncing models. We study the conditions for which these perturbations may collapse into primordial black holes and the hypothesis that these…

宇宙学与河外天体物理 · 物理学 2025-01-15 E. J. Barroso , L. F. Demétrio , S. D. P. Vitenti , Xuan Ye

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 review the creation mechanism of primordial black holes from first order phase transitions. We discuss various model-dependent and independent mechanisms and relate the properties of these mechanisms to the properties of primordial black…

高能物理 - 唯象学 · 物理学 2025-12-30 Indra Kumar Banerjee , Ujjal Kumar Dey , Shaaban Khalil

Strongly supercooled first-order phase transitions have been proposed as a primordial black hole (PBH) production mechanism. While previous works rely on simplified models with limited thermodynamic precision, we stress that reliable…

高能物理 - 唯象学 · 物理学 2026-05-25 Maciej Kierkla , Nicklas Ramberg , Philipp Schicho , Daniel Schmitt

Primordial Black Holes (PBHs) that form from the collapse of density perturbations are more clustered than the underlying density field. In a previous paper, we showed the constraints that this has on the prospects of PBH dark matter. In…

宇宙学与河外天体物理 · 物理学 2015-05-30 James R. Chisholm

We discuss the possibility of forming primordial black holes during a first-order phase transition in the early Universe. As is well known, such a phase transition proceeds through the formation of true-vacuum bubbles in a Universe that is…

宇宙学与河外天体物理 · 物理学 2025-08-20 Michael J. Baker , Moritz Breitbach , Joachim Kopp , Lukas Mittnacht

We study the production of primordial black holes (PBHs) during the preheating stage that follows a chaotic inflationary phase. The scalar fields present in the process are evolved numerically using a modified version of the HLATTICE code.…

宇宙学与河外天体物理 · 物理学 2014-04-30 E. Torres-Lomas , Juan Carlos Hidalgo , Karim A. Malik , L. Arturo Ureña-López

We perform the numerical simulation of primordial black hole formation from a nonspherical profile of the initial curvature perturbation $\zeta$. We consider the background expanding universe filled with the perfect fluid with the linear…

广义相对论与量子宇宙学 · 物理学 2024-04-29 Chul-Moon Yoo

Primordial Black Holes (PBHs) might have formed in the early Universe as a consequence of the collapse of density fluctuations with an amplitude above a critical value $\delta_{c}$: the formation threshold. Although for a…

宇宙学与河外天体物理 · 物理学 2024-04-12 J. L. G. Sobrinho , P. Augusto , A. L. Gonçalves

Large-amplitude density perturbations may have collapsed during the radiation dominated epoch of the Universe to form primordial black holes (PBHs). There are several constraints to the abundance of PBHs that stem from evaporation or…

宇宙学与河外天体物理 · 物理学 2019-09-25 Gabriela Sato-Polito , Ely D. Kovetz , Marc Kamionkowski

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

We propose a novel primordial black hole (PBH) formation mechanism based on a first-order phase transition (FOPT). If a fermion species gains a huge mass in the true vacuum, the corresponding particles get trapped in the false vacuum as…

宇宙学与河外天体物理 · 物理学 2021-11-24 Kiyoharu Kawana , Ke-Pan Xie

Recently, the formation of primordial black holes (PBHs) from the collapse of primordial fluctuations has received much attention. The abundance of PBHs formed during radiation domination is sensitive to the tail of the probability…

宇宙学与河外天体物理 · 物理学 2019-01-09 Tomohiro Nakama , Yi Wang

Primordial Black Holes (PBH) may have formed from the collapse of cosmic string loops. The spectral shape of the PBH mass spectrum can be determined by the scaling argument for string networks. Limits on the spectral amplitude derived from…

天体物理学 · 物理学 2009-10-30 U. F. Wichoski , Jane H. MacGibbon , Robert H. Brandenberger