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相关论文: Signatures of primordial black holes in gravitatio…

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The most massive black holes in our Universe form binaries at the centre of merging galaxies. The recent evidence for a gravitational-wave (GW) background from pulsar timing may constitute the first observation that these supermassive black…

高能天体物理现象 · 物理学 2024-08-09 Jakob Stegmann , Lorenz Zwick , Sander M. Vermeulen , Fabio Antonini , Lucio Mayer

In the recent second part of the third observation run by the LIGO-Virgo-KAGRA collaboration, a candidate with sub-solar mass components was reported, which we labelled as SSM200308. This study investigates the premise that primordial black…

宇宙学与河外天体物理 · 物理学 2024-09-20 Chen Yuan , Qing-Guo Huang

Are the stellar-mass merging binary black holes, recently detected by their gravitational wave signal, of stellar or primordial origin? Answering this question will have profound implications for our understanding of the Universe, including…

宇宙学与河外天体物理 · 物理学 2020-05-27 Giulio Scelfo , Nicola Bellomo , Alvise Raccanelli , Sabino Matarrese , Licia Verde

Interest to astrophysical evidence for primordial black holes (PBHs) formed in the early Universe from initial cosmological perturbations has increased after the discovery of coalescing binary black holes with masses more than dozen solar…

高能天体物理现象 · 物理学 2023-09-29 Konstantin Postnov , Aleksandre Kuranov , Nikita Mitichkin

The detection of a subsolar object in a compact binary merger is regarded as one of the smoking gun signatures of a population of primordial black holes~(PBHs). We critically assess whether these systems could be distinguished from stellar…

高能天体物理现象 · 物理学 2024-07-09 F. Crescimbeni , G. Franciolini , P. Pani , A. Riotto

Primordial black holes (PBHs) are compact objects proposed to have formed in the early Universe from the collapse of small-scale over-densities. Their existence may be detected from the observation of gravitational waves (GWs) emitted by…

宇宙学与河外天体物理 · 物理学 2022-09-01 Matteo Martinelli , Francesca Scarcella , Natalie B. Hogg , Bradley J. Kavanagh , Daniele Gaggero , Pierre Fleury

Primordial black holes (PBHs) can be not only cold dark matter candidates but also progenitors of binary black holes observed by LIGO-Virgo-KAGRA (LVK) Collaboration. The PBH mass can be shifted to the heavy distribution if multi-merger…

宇宙学与河外天体物理 · 物理学 2025-03-28 Lang Liu , Zhi-Qiang You , You Wu , Zu-Cheng Chen

It has been suggested that primordial black holes (PBHs) of roughly 30 solar masses could make up the dark matter and if so, might account for the recent detections by LIGO involving binary black holes in this mass range. It has also been…

宇宙学与河外天体物理 · 物理学 2019-02-26 Hiroya Nishikawa , Ely D. Kovetz , Marc Kamionkowski , Joseph Silk

Cosmic voids are known as underdense substructures of the cosmic web that cover a large volume of the Universe. It is known that cosmic voids contain a small number of dark matter halos, so the existence of primordial black holes (PBHs) in…

宇宙学与河外天体物理 · 物理学 2023-05-09 Saeed Fakhry , Seyed Sajad Tabasi , Javad T. Firouzjaee

The possibility that primordial black holes (PBHs) represent all of the dark matter (DM) in the Universe and explain the coalescences of binary black holes detected by LIGO/Virgo has attracted a lot of attention. PBHs are generated by the…

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

This is a review article on the primordial black holes (PBHs), with particular focus on the massive ones ($\gtrsim 10^{15}{\rm g}$) which have not evaporated by the present epoch by the Hawking radiation. By the detections of gravitational…

宇宙学与河外天体物理 · 物理学 2018-03-14 Misao Sasaki , Teruaki Suyama , Takahiro Tanaka , Shuichiro Yokoyama

The LIGO/Virgo collaboration has by now observed or constrained the gravitational merger rates of different classes of compact objects. We consider the possibility that the bulk of these mergers are primordial black hole (PBH) mergers of…

宇宙学与河外天体物理 · 物理学 2021-02-10 Karsten Jedamzik

As a candidate of dark matter, primordial black holes (PBHs) have attracted more and more attentions as they could be possible progenitors of the heavy binary black holes (BBHs) observed by LIGO/Virgo. Accurately estimating the merger rate…

宇宙学与河外天体物理 · 物理学 2020-04-15 You Wu

Ground-based gravitational-wave (GW) observatories have transformed our view of compact-object mergers, yet their reach still limits a comprehensive reconstruction of the processes that generate these systems. Only next-generation…

We study the prospects of future gravitational wave (GW) detectors in probing primordial black hole (PBH) binaries. We show that across a broad mass range from $10^{-5}M_\odot$ to $10^7M_\odot$, future GW interferometers provide a potential…

宇宙学与河外天体物理 · 物理学 2021-10-14 Oriol Pujolas , Ville Vaskonen , Hardi Veermäe

As a candidate of dark matter, and related to many fundamental physics issues, the primordial black hole (PBH) is a crucial topic. However, so far the existence of PBHs is still not confirmed, and currently running GW detectors are still…

综合物理 · 物理学 2019-07-10 Hao Wen

Formation of significant number of primordial black holes (PBHs) is realized if and only if primordial density fluctuations have a large amplitude, which means that tensor perturbations generated from these scalar perturbations as a second…

天体物理学 · 物理学 2011-07-06 Ryo Saito , Jun'ichi Yokoyama

We conduct a thorough Bayesian analysis of the possibility that the black hole merger events seen in gravitational waves are primordial black hole (PBH) mergers. Using the latest merger rate models for PBH binaries drawn from a lognormal…

宇宙学与河外天体物理 · 物理学 2021-01-04 Alex Hall , Andrew D. Gow , Christian T. Byrnes

For a variety of on-going and planned gravitational-wave (GW) experiments, we study expected constraints on the fraction ($f_{\rm PBH}$) of primordial black holes (PBHs) in dark matter by evaluating the energy-density spectra of two kinds…

宇宙学与河外天体物理 · 物理学 2020-03-26 Sai Wang , Takahiro Terada , Kazunori Kohri

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.…