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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

Primordial black holes (PBHs) are supposed to form from the collapse of over-densed regions generated by large scalar curvature perturbations in the radiation dominated era. Despite decades of various independent observations, the nature of…

星系天体物理 · 物理学 2021-08-31 Chen Yuan , Qing-Guo Huang

Primordial black hole (PBH) mergers have been proposed as an explanation for the gravitational wave events detected by the LIGO collaboration. Such PBHs may be formed in the early Universe as a result of the collapse of extremely rare…

宇宙学与河外天体物理 · 物理学 2017-02-20 Tomohiro Nakama , Joseph Silk , Marc Kamionkowski

There has recently been renewed interest in the possibility that the dark matter in the universe consists of primordial black holes (PBHs). Current observational constraints leave only a few PBH mass ranges for this possibility. One of them…

宇宙学与河外天体物理 · 物理学 2019-06-05 N. Bartolo , V. De Luca , G. Franciolini , A. Lewis , M. Peloso , A. Riotto

As potential candidates of dark matter, primordial black holes (PBHs) are within the core scopes of various astronomical observations. In light of the explosive development of gravitational wave (GW) and radio astronomy, we thoroughly…

宇宙学与河外天体物理 · 物理学 2019-08-23 Yi-Fu Cai , Chao Chen , Xi Tong , Dong-Gang Wang , Sheng-Feng Yan

In the recent years, primordial black holes (PBHs) have emerged as one of the most interesting and hotly debated topics in cosmology. Among other possibilities, PBHs could explain both some of the signals from binary black hole mergers…

We consider the possibility that the majority of dark matter in our Universe consists of black holes of primordial origin. We determine the conditions under which such black holes may have originated from a single-field model of inflation…

宇宙学与河外天体物理 · 物理学 2020-07-22 Guillermo Ballesteros , Julián Rey , Marco Taoso , Alfredo Urbano

Primordial black holes (PBHs) are one of the candidates to explain the gravitational wave (GW) signals observed by the LIGO detectors. Among several phenomena in the early Universe, cosmic inflation is a major example to generate PBHs from…

宇宙学与河外天体物理 · 物理学 2017-06-14 Keisuke Inomata , Masahiro Kawasaki , Kyohei Mukaida , Yuichiro Tada , Tsutomu T. Yanagida

We propose a novel method to probe primordial gravitational waves by means of primordial black holes (PBHs). When the amplitude of primordial tensor perturbations on comoving scales much smaller than those relevant to Cosmic Microwave…

广义相对论与量子宇宙学 · 物理学 2016-05-17 Tomohiro Nakama , Teruaki Suyama

Primordial Black Holes (PBH) from peaks in the curvature power spectrum could constitute today an important fraction of the Dark Matter in the Universe. At horizon reentry, during the radiation era, order one fluctuations collapse…

宇宙学与河外天体物理 · 物理学 2018-12-31 Sebastien Clesse , Juan García-Bellido , Stefano Orani

Various mechanisms have been suggested for the formation of Primordial Black Holes (PBHs), and this thesis focuses on the standard mechanism based on the critical collapse of cosmological fluctuations. The underlying idea is that during…

宇宙学与河外天体物理 · 物理学 2025-01-07 Antonio Junior Iovino

Primordial black holes (PBHs) can constitute the predominant fraction of dark matter (DM) if PBHs reside in the currently unconstrained "sublunar" mass range. PBHs originating from scalar perturbations generated during inflation can…

宇宙学与河外天体物理 · 物理学 2021-01-28 Sunao Sugiyama , Volodymyr Takhistov , Edoardo Vitagliano , Alexander Kusenko , Misao Sasaki , Masahiro Takada

We study the formation of primordial black holes (PBHs) from the collapse of density perturbations induced by primordial gravitational waves (PGWs). The PGWs' interpretation of the stochastic gravitational wave background (SGWB) detected by…

广义相对论与量子宇宙学 · 物理学 2025-10-14 Utkarsh Kumar

We dedicate this thesis to the study of signatures coming from the primordial epochs of the universe. We will focus in particular on Primordial Black Holes (PBHs), which may be formed from perturbations generated during inflation and might…

宇宙学与河外天体物理 · 物理学 2022-07-19 Valerio De Luca

Primordial black holes (PBHs) from the early Universe have been connected with the nature of dark matter and can significantly affect cosmological history. We show that coincidence dark radiation and density fluctuation gravitational wave…

宇宙学与河外天体物理 · 物理学 2021-11-08 Guillem Domènech , Volodymyr Takhistov , Misao Sasaki

The idea that primordial black holes (PBHs) can comprise most of the dark matter of the universe has recently reacquired a lot of momentum. Observational constraints, however, rule out this possibility for most of the PBH masses, with a…

宇宙学与河外天体物理 · 物理学 2019-07-31 N. Bartolo , V. De Luca , G. Franciolini , M. Peloso , D. Racco , A. Riotto

The NANOGrav Collaboration has recently published a strong evidence for a stochastic common-spectrum process that may be interpreted as a stochastic gravitational wave background. We show that such a signal can be explained by second-order…

宇宙学与河外天体物理 · 物理学 2021-02-03 V. De Luca , G. Franciolini , A. Riotto

We investigate a new mechanism to create large curvature perturbations on small scales due to parameter resonance in a single-field inflationary model with a small periodic structure upon the potential. After reentering the horizon, the…

宇宙学与河外天体物理 · 物理学 2020-06-17 Rong-Gen Cai , Zong-Kuan Guo , Jing Liu , Lang Liu , Xing-Yu Yang

Primordial Black Holes (PBH) could be the cold dark matter of the universe. They could have arisen from large (order one) curvature fluctuations produced during inflation that reentered the horizon in the radiation era. At reentry, these…

宇宙学与河外天体物理 · 物理学 2017-09-20 Juan Garcia-Bellido , Marco Peloso , Caner Unal

Multiple pulsar timing array (PTA) collaborations recently announced the evidence of common-spectral processes caused by gravitational waves (GWs). These can be the stochastic GW background and its origin may be astrophysical and/or…

宇宙学与河外天体物理 · 物理学 2024-03-05 Keisuke Inomata , Kazunori Kohri , Takahiro Terada
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