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相关论文: Primordial black hole versus inflaton

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We investigate the cosmology of mini Primordial Black Holes (PBHs) produced by large density perturbations. The mini PBHs evaporate promptly in the early universe and we assume that a stable remnant is left behind. The PBHs remnants can…

宇宙学与河外天体物理 · 物理学 2019-10-16 Ioannis Dalianis , George Tringas

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

The primordial black hole (PBH) productions from the inflationary potential with an inflection point usually rely heavily on the fine-tuning of the model parameters. We propose in this work a new kind of the $\alpha$-attractor inflation…

宇宙学与河外天体物理 · 物理学 2023-06-09 Chengjie Fu , Shao-Jiang Wang

Primordial black holes are produced in a minimal UV extension to the Higgs inflation with an included $R^2$ term. We show that for parameters consistent with Standard Model measurements and Planck observation results lead to $M_{\rm PBH}…

高能物理 - 唯象学 · 物理学 2021-02-03 Dhong Yeon Cheong , Sung Mook Lee , Seong Chan Park

Primordial Black Holes (PBH) could dominate in the early universe and, evaporating before Big bang Nucleosynthesis, can provide new freeze in mechanism of dark matter (DM) production. The proposed scenario is considered for two possible…

高能物理 - 唯象学 · 物理学 2024-06-11 Pratik Chattopadhyay , Arnab Chaudhuri , Maxim Yu. Khlopov

Primordial black holes (PBHs) may have formed through the gravitational collapse of cosmological perturbations that were generated and stretched during the inflationary era, later entering the cosmological horizon during the decelerating…

广义相对论与量子宇宙学 · 物理学 2024-12-03 Tomohiro Harada

The Reheating process at the end of inflation is often modeled by an oscillating scalar field which shows a background dust-like behaviour, prompting the analysis of gravitational collapse and black hole formation in this era to be…

宇宙学与河外天体物理 · 物理学 2022-08-31 Luis E. Padilla , Juan Carlos Hidalgo , Karim A. Malik

We investigate Primoridal Black Hole (PBH) formation by which we mean black holes produced in the early universe during radiation domination. After discussing the range of PBH mass permitted in the original mechanism of Carr and Hawking,…

广义相对论与量子宇宙学 · 物理学 2016-04-27 Paul H. Frampton

In this work, we explore the production of primordial black holes (PBHs) within the context of $\alpha$-attractor inflationary models, focusing on the preheating phase following inflation. During this phase, self-resonance instabilities…

宇宙学与河外天体物理 · 物理学 2025-05-26 Daniel del-Corral , Paolo Gondolo , K. Sravan Kumar , João Marto

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

We show that fragmentation of the inflaton into long-lived spatially localized oscillon configurations can lead to copious production of black holes. In a single-field inflation model primordial black holes of sublunar mass can form, and…

宇宙学与河外天体物理 · 物理学 2018-10-12 Eric Cotner , Alexander Kusenko , Volodymyr Takhistov

The inflationary diffusion of (pseudo-)scalar fields with discrete symmetries can seed the formation of a gas of closed domain walls after inflation, when the distance between degenerate minima in field space is not too far from the…

宇宙学与河外天体物理 · 物理学 2025-04-11 Miguel Faria , Ricardo Z. Ferreira , Fabrizio Rompineve

We investigate the formation of primordial black holes (PBHs) from the collapse of spherically symmetric domain wall bubbles, which spontaneously nucleate via quantum tunneling during inflation. Since the tension of domain walls changes…

宇宙学与河外天体物理 · 物理学 2020-01-22 Jing Liu , Zong-Kuan Guo , Rong-Gen Cai

Primordial Black Hole (PBH) is one of the leading non-particle candidates for dark matter (DM). Although several observations severely constrain the amount of PBHs, it is recently pointed out that there is an uncertainty on the microlensing…

宇宙学与河外天体物理 · 物理学 2018-02-21 Keisuke Inomata , Masahiro Kawasaki , Kyohei Mukaida , Tsutomu T. Yanagida

We investigate the generation of Primordial Black Holes (PBHs) with the aid of gravitationally increased friction mechanism originated from the NonMinimal field Derivative Coupling (NMDC) to gravity framework, with the quartic potential.…

广义相对论与量子宇宙学 · 物理学 2022-02-02 Soma Heydari , Kayoomars Karami

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

We propose a model of inflation capable of generating a population of light black holes (about $10^{-16}$ - $10^{-14}$ solar masses) that might account for a significant fraction of the dark matter in the Universe. The effective potential…

高能物理 - 唯象学 · 物理学 2018-01-10 Guillermo Ballesteros , Marco Taoso

We investigate the effects of producing dark matter by Hawking evaporation of primordial black holes (PBHs) in scenarios that may have a second well-motivated dark matter production mechanism, such as freeze-out, freeze-in, or gravitational…

高能物理 - 唯象学 · 物理学 2020-11-25 Paolo Gondolo , Pearl Sandick , Barmak Shams Es Haghi

We speculate that the early Universe was inside a primordial black hole. The interior of the the black hole is a dS background and the two spacetimes are separated on the surface of black hole's event horizon. We argue that this picture…

高能物理 - 理论 · 物理学 2016-10-13 Hassan Firouzjahi

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.…