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Primordial black holes (PBHs) are a profound signature of primordial cosmological structures and provide a theoretical tool to study nontrivial physics of the early Universe. The mechanisms of PBH formation are discussed and observational…

天体物理学 · 物理学 2014-11-18 M. Yu. Khlopov

We update the constraints on the fraction of the Universe that may have gone into primordial black holes (PBHs) over the mass range $10^{-5}\text{--}10^{50}$ g. Those smaller than $\sim 10^{15}$ g would have evaporated by now due to Hawking…

宇宙学与河外天体物理 · 物理学 2021-12-22 Bernard Carr , Kazunori Kohri , Yuuiti Sendouda , Jun'ichi Yokoyama

Magnetic monopoles, if they exist, would be produced amply in strong magnetic fields and high temperatures via the thermal Schwinger process. Such circumstances arise in heavy ion collisions and in neutron stars, both of which imply lower…

高能物理 - 唯象学 · 物理学 2017-12-20 Oliver Gould , Arttu Rajantie

The mass function of primordial black holes created through the near-critical gravitational collapse is calculated in a manner fairly independent of the statistical distribution of underlying density fluctuation, assuming that it has a…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Jun'ichi Yokoyama

Primordial black holes may have formed in the radiative era of the early Universe from the collapse of large enough amplitude perturbations of the metric. These correspond to non linear energy density perturbations characterized by an…

广义相对论与量子宇宙学 · 物理学 2020-01-06 Ilia Musco

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

We study the properties of a nonlinear magnetic-charged black hole in the presence of a phantom global monopole. By incorporating nonlinear electrodynamics (NLE) and exotic scalar fields, we derive an exact black hole solution and analyze…

广义相对论与量子宇宙学 · 物理学 2025-10-13 B. Hamil , B. C. Lütfüoğlu

Primordial magnetic fields generated in the early universe are subject of considerable investigation, and observational limits on their strength are required to constrain the theory. Due to their impact on the reionization process, the…

宇宙学与河外天体物理 · 物理学 2015-05-30 Dominik R. G. Schleicher , Francesco Miniati

We discuss some cosmological implications of extensions of the Standard Model with hidden sector scalars coupled to the Higgs boson. We put special emphasis on the conformal case, in which the electroweak symmetry is broken radiatively with…

高能物理 - 唯象学 · 物理学 2010-04-21 J. R. Espinosa , T. Konstandin , J. M. No , M. Quiros

Dark matter coupled solely gravitationally can be produced through the decay of primordial black holes in the early universe. If the dark matter is lighter than the initial black hole temperature, it could be warm enough to be subject to…

宇宙学与河外天体物理 · 物理学 2020-09-23 Iason Baldes , Quentin Decant , Deanna C. Hooper , Laura Lopez-Honorez

A recent understanding on how quantum effects may affect black-hole evolution opens new scenarios for dark matter, in connection with the presence of black holes in the very early universe. Quantum fluctuations of the geometry allow for…

广义相对论与量子宇宙学 · 物理学 2018-12-27 Francesca Vidotto

The presence of a primordial magnetic field in the early universe affects the dynamic of the electroweak phase transition enhancing its strength. This effect may enlarge the window for electroweak baryogenesis in the minimal supersymmetric…

高能物理 - 唯象学 · 物理学 2009-10-31 D. Comelli , D. Grasso , M. Pietroni , A. Riotto

We study the impact on electroweak baryogenesis from a swifter cosmological expansion induced by dark matter. We detail the experimental bounds that one can place on models that realize it, and we investigate the modifications of these…

高能物理 - 唯象学 · 物理学 2016-12-01 Marek Lewicki , Tanja Rindler-Daller , James D. Wells

A consequence of the evaporation of primordial black holes in the early universe may be the generation of mirror matter. This would have implications with regard to dark matter, and the number of light particle species in equilibrium at the…

天体物理学 · 物理学 2009-10-31 Nicole F. Bell , Raymond R. Volkas

Thermal fluctuations of the gauge field lead to monopole formation at the grand unified phase transition in the early Universe, even if the transition is merely a smooth crossover. The dependence of the produced monopole density on various…

高能物理 - 唯象学 · 物理学 2007-05-23 A. Rajantie

In this paper, we explore the implications of the so-called slingshot effect. It represents a rather general phenomenon occurring when a localized source, such as a monopole, quark, or a $D$-brane, crosses a domain wall separating the…

高能物理 - 唯象学 · 物理学 2026-03-20 Maximilian Bachmaier , Gia Dvali , Juan Sebastián Valbuena-Bermúdez , Michael Zantedeschi

We show that monopoles can be pair produced by cosmological magnetic fields in the early universe. The pair production gives rise to relic monopoles, and at the same time induces a self-screening of the magnetic fields. By studying these…

高能物理 - 唯象学 · 物理学 2021-08-17 Takeshi Kobayashi

Primordial black holes formed in an early post-inflation matter-dominated epoch during preheating provide a novel pathway for a source of the dark matter that utilizes known physics in combination with plausible speculations about the role…

宇宙学与河外天体物理 · 物理学 2020-03-30 J. A. de Freitas Pacheco , Joseph Silk

Independently from the formation mechanism of primordial black holes in the early Universe, their generation is accompanied by a ringdown phase during which they relax to a stationary configuration and gravitational waves under the form of…

广义相对论与量子宇宙学 · 物理学 2026-02-23 Valerio De Luca , Antonio J. Iovino , Antonio Riotto

One of the remarkable features of black holes is that they possess a thermodynamic description, even though they do not appear to be statistical systems. We use self-gravitating magnetic monopole solutions as tools for understanding the…

广义相对论与量子宇宙学 · 物理学 2015-06-25 Arthur Lue , Erick J. Weinberg