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We propose a novel mechanism where Primordial Black Hole (PBH) dark matter is formed much later in the history of the universe between the epoch of Big Bang Nucleosynthesis (BBN) and Cosmic Microwave Background (CMB) photon decoupling. In…

宇宙学与河外天体物理 · 物理学 2022-06-24 Amlan Chakraborty , Prolay K Chanda , Kanhaiya Lal Pandey , Subinoy Das

Recent developments in the study of primordial black holes (PBHs) will be reviewed, with particular emphasis on their formation and evaporation. PBHs could provide a unique probe of the early Universe, gravitational collapse, high energy…

天体物理学 · 物理学 2008-11-26 B. J. Carr

It is believed that primordial black holes (PBHs), if they exist, can serve as a powerful tool to probe the early stage of the cosmic history. Essentially, in the radiation dominated universe, PBHs could form by the gravitational collapse…

广义相对论与量子宇宙学 · 物理学 2021-02-11 Che-Yu Chen

The formation and abundance of primordial black holes (PBHs) arising from the curvature perturbation $\zeta$ is studied. The non-linear relation between $\zeta$ and the density contrast $\delta$ means that, even when $\zeta$ has an exactly…

宇宙学与河外天体物理 · 物理学 2019-11-15 Sam Young , Ilia Musco , Christian T. Byrnes

Primordial black holes (PBHs) are of fundamental interest in cosmology and astrophysics, and have received much attention as a dark matter candidate and as a potential source of gravitational waves. One possible PBH formation mechanism is…

宇宙学与河外天体物理 · 物理学 2020-08-13 Alexander C. Jenkins , Mairi Sakellariadou

Small black holes should have formed in the early Universe if the density contrast was high enough. This article aims at giving a - biased and partial - short overview of the latest breakthroughs in this field. It first deals with tentative…

天体物理学 · 物理学 2007-05-23 G. Boudoul , A. Barrau

Primordial black holes (PBHs) can form in the early Universe via the collapse of large density perturbations. There are tight constraints on the abundance of PBHs formed due to their gravitational effects and the consequences of their…

宇宙学与河外天体物理 · 物理学 2009-07-30 Amandeep S. Josan , Anne M. Green , Karim A. Malik

The recent discovery of critical phenomena arising in gravitational collapse near the threshold of black hole formation is used to estimate the initial mass function of primordial black holes (PBHs). It is argued that the universal scaling…

天体物理学 · 物理学 2008-11-26 J. C. Niemeyer , K. Jedamzik

Primordial black holes, which could have been formed in the very early Universe due to the collapse of large curvature fluctuations, are nowadays one of the most attractive and fascinating research areas in cosmology for their possible…

广义相对论与量子宇宙学 · 物理学 2022-01-27 Albert Escrivà

Primordial black holes (PBHs) constitute a compelling dark matter candidate whose gravitational effects could significantly influence early cosmic structure formation. We investigate the impact of PBHs on Population III star formation…

宇宙学与河外天体物理 · 物理学 2025-07-08 Julia Monika Koulen , Stefano Profumo , Nolan Smyth

Using the concept of apparent horizon for dynamical black holes, we revisit the formation of primordial black holes (PBH) in the early universe for both linear and non-linear regimes. First, we develop the perturbation theory for…

广义相对论与量子宇宙学 · 物理学 2017-06-28 Alireza Allahyari , Javad T. Firouzjaee , Ali Akbar Abolhasani

We present a complete analytic and semi-analytic study of gravitational collapse and primordial black hole (PBH) formation in the quadratic $f(R)$ model $f(R)=R+\alpha R^2$. We first derive the perturbative expansion around General…

广义相对论与量子宇宙学 · 物理学 2026-01-07 G. G. L. Nashed

Primordial black holes (PBHs) are expected to accrete particle dark matter around them to form ultracompact minihalos (UCMHs), if the PBHs themselves are not most of the dark matter. We show that if most dark matter is a thermal relic, then…

宇宙学与河外天体物理 · 物理学 2015-05-18 Brian C. Lacki , John F. Beacom

In the model where Primordial Black Holes (PBHs) form from large primordial curvature (C) perturbations, i.e., CPBHs, constraints on PBH abundance provide in principle constraints on the primordial curvature power spectrum. This connection…

宇宙学与河外天体物理 · 物理学 2019-10-15 Alba Kalaja , Nicola Bellomo , Nicola Bartolo , Daniele Bertacca , Sabino Matarrese , Ilia Musco , Alvise Raccanelli , Licia Verde

First results of a numerical investigation of primordial black hole formation in the radiation dominated phase of the Early Universe are presented. The simulations follow the gravitational collapse of three different families of…

天体物理学 · 物理学 2007-05-23 J. C. Niemeyer

Primordial black holes (PBHs) provide a unique probe of the early Universe and may have an enhanced abundance in bouncing cosmologies, where a long contracting phase can amplify perturbations. We develop a unified framework to study PBH…

广义相对论与量子宇宙学 · 物理学 2026-02-27 Xuan Ye , Luiz Felipe Demetrio , Eduardo Jose Barroso , Shen-Feng Yan , Nelson Pinto-Neto

We describe a realistic mechanism whereby black holes with significant QCD color charge could have formed during the early universe. Primordial black holes (PBHs) could make up a significant fraction of the dark matter if they formed well…

高能物理 - 唯象学 · 物理学 2024-06-11 Elba Alonso-Monsalve , David I. Kaiser

Primordial black holes (PBHs) can form in the early Universe from the collapse of rare, large density fluctuations. They have never been observed, but this fact is enough to constrain the amplitude of fluctuations on very small scales which…

宇宙学与河外天体物理 · 物理学 2013-09-20 Sam Young , Christian T. Byrnes

Primordial black holes (PBHs) can form in the early Universe, for instance during radiation domination, from the collapse of large-amplitude density perturbations shortly after horizon re-entry. This mechanism establishes an approximate…

宇宙学与河外天体物理 · 物理学 2026-03-25 Ashu Kushwaha , Teruaki Suyama

In this chapter we first describe the early history of primordial black hole (PBH) research. We then discuss their possible formation mechanisms, including critical collapse from inflationary fluctuations and various types of phase…

宇宙学与河外天体物理 · 物理学 2025-02-24 Bernard Carr , Florian Kuhnel