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Primordial black holes (PBHs) could account for all or part of dark matter, as well as for some LIGO events. We discuss the spins of primordial black holes produced in different cosmological scenarios, with the emphasis on recently…

宇宙学与河外天体物理 · 物理学 2021-09-06 Marcos M. Flores , Alexander Kusenko

Black holes with masses $\approx 1\, M_{\odot}$ cannot be produced via stellar evolution. A popular scenario of their formation involves transmutation of neutron stars - by accumulation of dark matter triggering gravitational collapse in…

高能物理 - 唯象学 · 物理学 2022-03-28 Raghuveer Garani , Dmitry Levkov , Peter Tinyakov

In this note we suggest that high-mass black holes; i.e., black holes of several solar masses, can be formed in binaries with low-mass main-sequence companions, provided that the hydrogen envelope of the massive star is removed in common…

天体物理学 · 物理学 2009-10-30 G. E. Brown , C. -H. Lee , H. A. Bethe

We propose that any black hole has atomic structure in its inside and has no horizon as a model of black holes. Our proposal is founded on a mean field approximation of gravity. The structure of our model consists of a (charged) singularity…

高能物理 - 理论 · 物理学 2008-11-26 Yukinori Nagatani

There are ongoing efforts in detecting Hawking radiation from primordial black holes (PBH) formed during the early universe. Here we put an upper limit on the PBH number density that could have been formed prior to the big bang…

综合物理 · 物理学 2010-06-29 C. Sivaram , Kenath Arun

The nonbaryonic dark matter of the Universe can consist of new stable charged leptons and quarks, if they are hidden in elusive "dark atoms" of composite dark matter. Such possibility can be compatible with the severe constraints on…

宇宙学与河外天体物理 · 物理学 2015-05-20 Maxim Yu. Khlopov

It has been postulated that black holes could be created in particle collisions within the range of the available energies for nowadays colliders (LHC). In this paper we analyze the evaporation of a type of black holes that are candidates…

广义相对论与量子宇宙学 · 物理学 2015-06-17 R. Torres , F. Fayos , O. Lorente-Espin

Aspects of primordial black holes, i.e. black holes formed in the early Universe, are reviewed. Special emphasis is put on their formation, their role as dark matter candidates and their manifold signatures, particularly through…

宇宙学与河外天体物理 · 物理学 2025-03-25 Albert Escrivà , Florian Kuhnel , Yuichiro Tada

We examine the production and evolution of microscopic black holes in the early universe in the large extra dimensions scenario. We demonstrate that, unlike in the standard four-dimensional cosmology, in large extra dimensions absorption of…

高能物理 - 唯象学 · 物理学 2008-11-26 John A. Conley , Tommer Wizansky

The spontaneous creation of primordial black holes in a violently expanding Universe is a well studied phenomenon. Based on quantum gravity arguments, it has been conjectured that the early Universe might have undergone a lower dimensional…

广义相对论与量子宇宙学 · 物理学 2020-10-06 Konstantinos F. Dialektopoulos , Piero Nicolini , Athanasios G. Tzikas

We reexamine production of primordial black holes in a supercooled phase transition. While a mere overdensity associated with a surviving false-vacuum patch does not imply formation of a black hole, it is possible for such a patch to evolve…

高能物理 - 唯象学 · 物理学 2024-03-05 Marcos M. Flores , Alexander Kusenko , Misao Sasaki

The nonbaryonic dark matter of the Universe is assumed to consist of new stable particles. A specific case is possible, when new stable particles bear ordinary electric charge and bind in heavy "atoms" by ordinary Coulomb interaction. Such…

宇宙学与河外天体物理 · 物理学 2015-03-17 Maxim Yu. Khlopov , Andrey G. Mayorov , Evgeny Yu. Soldatov

It has been proposed that the first, intermediate-mass ($\approx 10^{5-6}~M_\odot$) black holes might form through direct collapse of unpolluted gas in atomic-cooling halos exposed to a strong Lyman-Werner (LW) or near-infrared (NIR)…

宇宙学与河外天体物理 · 物理学 2015-06-18 Bin Yue , Andrea Ferrara , Ruben Salvaterra , Yidong Xu , Xuelei Chen

In theories with a broken discrete symmetry, Hubble sized spherical domain walls may spontaneously nucleate during inflation. These objects are subsequently stretched by the inflationary expansion, resulting in a broad distribution of…

广义相对论与量子宇宙学 · 物理学 2017-05-10 Heling Deng , Jaume Garriga , Alexander Vilenkin

Supernova theory suggests that black holes of a stellar origin cannot attain masses in the range of 50-135 solar masses in isolation. We argue here that this mass gap is filled in by black holes that grow by gas accretion in dense stellar…

星系天体物理 · 物理学 2019-12-24 Zacharias Roupas , Demosthenes Kazanas

It has been shown that black holes can be quantized by using Bohr's idea of quantizing the motion of an electron inside the atom. We apply these ideas to the universe as a whole. This approach reinforces the suggestion that it may be a way…

综合物理 · 物理学 2012-01-17 Màrius Josep Fullana i Alfonso , Antonio Alfonso-Faus

We discuss the production of primordial black holes in an early matter dominated era, which typically takes place in string inspired early universe cosmological models. In particular, we consider a pre-big bang scenario (extending previous…

广义相对论与量子宇宙学 · 物理学 2023-08-14 Pietro Conzinu , Giovanni Marozzi

We present a model for the formation of massive black holes ($\sim 1000 \msun$) due to stellar-dynamical processes in the first stellar clusters formed at early cosmic times ($z\sim10-20$). The high redshift black hole seeds form as a…

天体物理学 · 物理学 2009-11-13 Bernadetta Devecchi , Marta Volonteri

In some respects the black hole plays the same role in gravitation that the atom played in the nascent quantum mechanics. This analogy suggests that black hole mass $M$ might have a discrete spectrum. I review the physical arguments for the…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Jacob D. Bekenstein