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We outline a new production mechanism for dark matter that we dub "recycling": dark sector particles are kinematically trapped in the false vacuum during a dark phase transition; the false pockets collapse into primordial black holes…

高能物理 - 唯象学 · 物理学 2024-03-22 Thomas C. Gehrman , Barmak Shams Es Haghi , Kuver Sinha , Tao Xu

Recently, in the series of works a new effect of acceleration of particles by black holes was found. Under certain conditions, the energy in the centre of mass frame can become infinitely large. The essential ingredient of such effect is…

广义相对论与量子宇宙学 · 物理学 2011-03-28 Oleg B. Zaslavskii

If string theory describes nature, then charged black holes are not described by the Reissner-Nordstrom solution. This solution must be modified to include a massive dilaton. In the limit of vanishing dilaton mass, the new solution can be…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Gary T. Horowitz

It is known that a solution of remnant were suggested for black hole ground state after surface gravity is corrected by loop quantum effect. On the other hand, a Schwarzschild black hole in asymptotic Anti-de Sitter space would tunnel into…

高能物理 - 理论 · 物理学 2015-12-29 Wen-Yu Wen , Shang-Yu Wu

We propose a mechanism that can convert a sizeable fraction of neutron stars into black holes with mass $\sim 1M_\odot$, too light to be produced via standard stellar evolution. We show that asymmetric fermionic dark matter of mass $\sim$…

高能天体物理现象 · 物理学 2018-12-05 Chris Kouvaris , Peter Tinyakov , Michel H. G. Tytgat

Recently, it was shown in [1] that black holes are the source of dark energy. In [2-5], the truth or falsity of this concept has been discussed. We briefly state the arguments raised in each of these papers, but our main goal is not to…

广义相对论与量子宇宙学 · 物理学 2023-05-23 Jafar Sadeghi , Saeed Noori Gashti , Mohammad Reza Alipour , Mohammad Ali S. Afshar

We deal with phantom energy accretion onto the Schwarzschild de-Sitter black hole. The energy flux conservation, relativistic Bernoulli equation and mass flux conservation equation are formulated to discuss the phantom accretion. We discuss…

广义相对论与量子宇宙学 · 物理学 2017-08-23 M. Sharif , G. Abbas

A supermassive rotating toroidal black hole (TBH) is proposed as the fundamental structure of quasars and other jet-producing active galactic nuclei. Rotating protogalaxies gather matter from the central gaseous region leading to the birth…

天体物理学 · 物理学 2010-11-19 Robin J. Spivey

The black hole model with a self-gravitating charged spherical symmetric dust thin shell as a source is considered. The Schroedinger-type equation for such a model is derived. This equation appeared to be a finite differences equation. A…

广义相对论与量子宇宙学 · 物理学 2014-11-17 V. A. Berezin

The simplest possible equation for Hawking radiation, and other black hole radiated power is derived in terms of black hole density. Black hole density also leads to the simplest possible model of a gas of elementary constituents confined…

综合物理 · 物理学 2007-05-23 Mario Rabinowitz

This paper studies the interpretation of physics near a Schwarzschild black hole. A scenario for creation and growth is proposed that avoids the conundrum of information loss. In this picture the horizon recedes as it is approached and has…

广义相对论与量子宇宙学 · 物理学 2014-05-27 Christian Fronsdal

It has been thought for decades that rotating black holes (BHs) power the energetic gamma-ray bursts (GRBs) and active galactic nuclei (AGNs), but the mechanism that extracts the BH energy has remained elusive. We here show that the…

高能天体物理现象 · 物理学 2023-10-17 J. A. Rueda , R. Ruffini

Dilaton coupled electromagnetic field is essential element of low-energy string effective action or it may be considered as result of spherical compactification of Maxwell theory in higher dimensions. The large $N$ and large curvature…

高能物理 - 理论 · 物理学 2009-09-17 Andrei A. Bytsenko , Shin'ichi Nojiri , Sergei D. Odintsov

We argue that a primordial black hole is a natural and unique candidate for all dark matter. We show that, in a smooth-hybrid new double inflation model, a right amount of the primordial black holes, with a sharply-defined mass, can be…

高能物理 - 唯象学 · 物理学 2015-05-18 Paul H. Frampton , Masahiro Kawasaki , Fuminobu Takahashi , Tsutomu T. Yanagida

In the classical theory of general relativity black holes can only absorb and not emit particles. When quantum mechanical effects are taken into account, then the black holes emit particles as hot bodies with temperature proportional to…

广义相对论与量子宇宙学 · 物理学 2019-11-04 N. S. M. de Santi , R. Santarelli

Nathan Rosen's quantization approach to the gravitational collapse is applied in the simple case of a pressureless "star of dust" by finding the gravitational potential, the Schrodinger equation and the solution for the collapse's energy…

广义相对论与量子宇宙学 · 物理学 2024-03-27 Christian Corda , Fabiano Feleppa

We investigate the charging performance of a quantum battery coupled to a scalar field in the background of a three-dimensional rotating black hole. We show that for Dirichlet boundary conditions, the black hole rotation enhances the…

广义相对论与量子宇宙学 · 物理学 2025-10-28 Xiaofang Liu , Zehua Tian , Jieci Wang

We calculate the quantum radiation power of black holes which are asymptotic to the Einstein-de Sitter universe at spatial and null infinities. We consider two limiting mass accretion scenarios, no accretion and significant accretion. We…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Hiromi Saida , Tomohiro Harada , Hideki Maeda

We show that primordial black holes - in the observationally allowed mass window with $f_{\rm pbh}=1$ - formed from late nucleating patches in a first order phase transition imply upcoming gravitational wave interferometers will see a large…

高能物理 - 唯象学 · 物理学 2024-01-26 Iason Baldes , María Olalla Olea-Romacho

We present a natural mechanism which may induce an electric charge into an accretting black hole in the presence of a strong, high energy radiation field. We study this mechanism using Newtonian physics, and we also discuss the process…

天体物理学 · 物理学 2016-08-16 José A. de Diego , Deborah Dultzin-Hacyan , Jesús Galindo Trejo , Darío Núñez
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