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Primordial black holes (PBHs) have been proposed to explain at least a portion of dark matter. Observations have put strong constraints on PBHs in terms of the fraction of dark matter which they can represent, $f_{\rm PBH}$, across a wide…

宇宙学与河外天体物理 · 物理学 2021-10-20 Jie-Shuang Wang , Antonio Herrera-Martín , Yi-Ming Hu

We study the matter power spectrum constraint on primordial black holes (PBH) by the dark matter (DM) emitted through Hawking radiation. We particularly focus on the scenario where PBH, with mass ranges between 1g and $10^9$g, evaporates…

高能物理 - 唯象学 · 物理学 2026-03-06 Yu-Ming Chen

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

As a promising dark matter candidate, primordial black holes (PBHs) lighter than $\sim10^{-18}M_{\odot}$ are supposed to have evaporated by today through Hawking radiation. This scenario is challenged by the memory burden effect, which…

宇宙学与河外天体物理 · 物理学 2024-11-27 Yang Jiang , Chen Yuan , Chong-Zhi Li , Qing-Guo Huang

Primordial black holes (PBHs) can make up all of the dark matter (DM) if their mass, $m$, is in the so-called 'asteroid-mass window', $10^{17} \, {\rm g} \lesssim m \lesssim 10^{22} \, {\rm g}$. Observational constraints on the abundance of…

宇宙学与河外天体物理 · 物理学 2024-08-07 Matthew Gorton , Anne M. Green

A very pressing question in contemporary physics is the identity of Dark Matter (DM). Primordial Black Holes (PBHs) are one of the most well-motivated DM candidates. Light PBHs have been constrained by either the non-detection of their…

宇宙学与河外天体物理 · 物理学 2025-10-15 Akash Kumar Saha , Abhijeet Singh , Priyank Parashari , Ranjan Laha

We revisit the role of primordial black holes (PBHs) as potential dark matter (DM) candidates, particularly focusing on light asteroid-mass PBHs. These PBHs are expected to emit particles through Hawking evaporation that can generate cosmic…

高能天体物理现象 · 物理学 2026-03-26 Pedro De la Torre Luque , Jordan Koechler , Shyam Balaji

Superradiance provides a unique opportunity for investigating dark sectors as well as primordial black holes, which themselves are candidates for dark matter over a wide mass range. Using axion-like particles as an example, we show that…

高能物理 - 唯象学 · 物理学 2025-01-22 James B. Dent , Bhaskar Dutta , Tao Xu

Overdense regions can collapse into primordial black holes (PBHs) in the early universe, which are a compelling candidate for dark matter. Current constraints leave the asteroid-mass window the only possible one for PBH to account for all…

宇宙学与河外天体物理 · 物理学 2026-01-21 Wencong Hong , Shi Pi , Ao Wang , Zhenyu Zhang

Primordial black holes (PBHs) are one of the most appealing dark matter candidates over a wide range of masses and abundances. This broad parameter space has been constrained by a variety of observational probes. In this work, for the first…

高能天体物理现象 · 物理学 2026-04-14 Mainak Mukhopadhyay , Joaquim Iguaz Juan

Primordial black holes (PBHs) have long been a candidate for the elusive dark matter (DM), and remain poorly constrained in the ~20-100 Msun mass range. PBH binaries were recently suggested as the possible source of LIGO's first detections.…

宇宙学与河外天体物理 · 物理学 2018-01-10 Yacine Ali-Haïmoud , Ely D. Kovetz , Marc Kamionkowski

Within the mass range of $10^{16}-5\times 10^{18}$ g, primordial black holes (PBHs) persist as plausible candidates for dark matter. Our study involves a reassessment of the constraints on PBHs through a comparative analysis of the cosmic…

宇宙学与河外天体物理 · 物理学 2024-04-30 Xiu-hui Tan , Jun-qing Xia

Stellar-mass primordial black holes (PBHs) from the early Universe can directly contribute to the gravitational wave (GW) events observed by LIGO, but can only comprise a subdominant component of the dark matter (DM). The primary DM…

宇宙学与河外天体物理 · 物理学 2023-11-21 Masamune Oguri , Volodymyr Takhistov , Kazunori Kohri

Primordial black holes (PBHs) in the mass range $(30$--$100)~M_{\odot}$ are interesting candidates for dark matter, as they sit in a narrow window between microlensing and cosmic microwave background constraints. There are however tight…

宇宙学与河外天体物理 · 物理学 2021-03-25 Celine Boehm , Archil Kobakhidze , Ciaran A. J. O'Hare , Zachary S. C. Picker , Mairi Sakellariadou

Context. Primordial black holes (PBHs) have been proposed as potential candidates for dark matter (DM) and have garnered significant attention in recent years. Aims. Our objective is to delve into the distinct impact of PBHs on gas…

We discuss formation of dark matter (DM) mini-halos around primordial black holes (PBHs) and its implication on DM direct detection experiments, including axion searches. Motivated by LIGO observations, we consider $f_{\textrm{DM}} \simeq…

宇宙学与河外天体物理 · 物理学 2020-06-26 Mark P. Hertzberg , Enrico D. Schiappacasse , Tsutomu T. Yanagida

Historically the most popular dark matter candidates have been new elementary particles, such as Weakly Interacting Massive Particles and axions. However Primordial Black Holes (PBHs), black holes formed from overdensities in the early…

宇宙学与河外天体物理 · 物理学 2024-02-26 Anne M. Green

Dark matter could comprise, at least in part, primordial black holes (PBH). To test this hypothesis, we present an approach to constrain the PBH mass ($M_{\rm{PBH}}$) and mass fraction ($f_{\rm{PBH}}$) from the flux ratios of quadruply…

宇宙学与河外天体物理 · 物理学 2023-05-12 Veronica Dike , Daniel Gilman , Tommaso Treu

The detection of binary black hole coalescences by LIGO/Virgo has aroused the interest in primordial black holes (PBHs), because they could be both the progenitors of these black holes and a compelling candidate of dark matter (DM). PBHs…

宇宙学与河外天体物理 · 物理学 2025-03-28 Zu-Cheng Chen , Chen Yuan , Qing-Guo Huang

Soon after the recent first ever detection of gravitational waves from merging black holes it has been suggested that their origin is primordial. Appealingly, a sufficient number of primordial black holes (PBHs) could also partially or…

星系天体物理 · 物理学 2024-08-09 Jakob Stegmann , Pedro R. Capelo , Elisa Bortolas , Lucio Mayer