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In this paper we present an exact solution of Einstein's field equations describing the Schwarzschild black hole in dark energy background. It is also regarded as an embedded solution that the Schwarzschild black hole is embedded into the…

广义相对论与量子宇宙学 · 物理学 2014-09-30 Ngangbam Ishwarchandra , Ng. Ibohal , K. Yugindro Singh

This study derives a novel family of charged black hole solutions featuring short- and long-range modifications. These ones are achieved through a Yukawa-like gravitational potential modification and a nonsingular electric potential…

广义相对论与量子宇宙学 · 物理学 2025-03-05 A. A. Araújo Filho , Kimet Jusufi , B. Cuadros-Melgar , Genly Leon , Abdul Jawad , C. E. Pellicer

A different reason for the apparent weakness of the gravitational interaction is advanced, and its consequences for Hawking evaporation of a Schwarzschild black hole are investigated. Proceeding from some fundamental thermodynamic…

高能物理 - 理论 · 物理学 2009-05-12 D. G. Coyne , D. C. Cheng

It is shown that in the Schwarzschild background there exists direct counterpart of the Ba\~{n}ados-Silk-West effect for spinning particles. This means that if two particles collide near the black hole horizon, their energy in the centre of…

广义相对论与量子宇宙学 · 物理学 2016-06-22 O. B. Zaslavskii

Observation of an exploding black hole would provide the first direct evidence of primordial black holes, the first direct evidence of Hawking radiation, and definitive information on the particles present in nature. However, indirect…

高能物理 - 唯象学 · 物理学 2025-10-08 Michael J. Baker , Joaquim Iguaz Juan , Aidan Symons , Andrea Thamm

I present an elementary primer of black hole physics, including its general relativity basis, all peppered with astrophysical illustrations. Following a brief review of the process stellar collapse to a black hole, I discuss the…

天体物理学 · 物理学 2007-05-23 Jacob D. Bekenstein

We investigate the idea that ultrahigh energy gamma-rays (E>10 TeV) can be produced when charged particles are accelerated by microscopic black holes. We begin by showing that microscopic black holes may exist as remnants of primordial…

天体物理学 · 物理学 2009-11-07 Roberto Casadio , Benjamin Harms , Octavian Micu

Starting from a discussion of the black hole information loss paradox, we argue that Primordial Black Hole Remnants (PBHRs) of Planck mass, should they exist, are a plausible candidate for dark energy. We call this proposal the PBHR model.…

广义相对论与量子宇宙学 · 物理学 2019-04-09 Dimitris S. Kallifatides

Zajacek et al made an interesting theoretical prediction on the electrification of a non-rotating black hole; if a non-rotating black hole is surrounded by plasma composed of protons and electrons, it will acquire electric charge due to the…

广义相对论与量子宇宙学 · 物理学 2024-09-27 Ken-ichi Nakao , Kenta Matsuo , Hirotaka Yoshino , Hideki Ishihara

The probability of a charged particle production by the electric field of a charged black hole depends essentially on the particle energy. This probability is found in the nonrelativistic and ultrarelativistic limits. The range of values…

广义相对论与量子宇宙学 · 物理学 2009-10-31 I. B. Khriplovich

We construct several charged regular black hole metrics employing mass distribution functions which are inspired by continuous probability distributions. Some of these metrics satisfy the weak energy condition and asymptotically behave as…

广义相对论与量子宇宙学 · 物理学 2014-12-24 Leonardo Balart , Elias C. Vagenas

Particles with negative energies are considered for three different cases: inside of horizon of Schwarzschild black hole, Milne's coordinates in flat Minkowski space-time (Milne's universe using nonsynchronous coordinates) and in…

广义相对论与量子宇宙学 · 物理学 2023-05-04 A. A. Grib , Yu. V. Pavlov

Primordial black holes are analytically and numerically discussed based on the extended McVittie spacetime solution. By assuming that dark matter and radiation are the only sources of energy accreted by the forming central object, it is…

广义相对论与量子宇宙学 · 物理学 2020-12-09 F. Ruiz , C. Molina , J. A. S. Lima

Contrary to a prevailing assumption that black holes would swiftly discharge, we argue that black holes can charge preferentially when boosted through an ambient magnetic field. Though the details are very different, the preference for…

广义相对论与量子宇宙学 · 物理学 2022-12-06 Prakruth Adari , Roman Berens , Janna Levin

The stationary, spherically symmetric accretion of dark energy onto a Schwarzschild black hole is considered in terms of relativistic hydrodynamics. The approximation of an ideal fluid is used to model the dark energy. General expressions…

天体物理学 · 物理学 2014-10-13 E. Babichev , V. Dokuchaev , Yu. Eroshenko

We obtain electrically charged black hole solutions of the Einstein equations in arbitrary dimensions with a nonlinear electrodynamics source. The matter source is deriving from a Lagrangian given by an arbitrary power of the Maxwell…

高能物理 - 理论 · 物理学 2008-11-26 Mokhtar Hassaine , Cristian Martinez

Our goal in this paper is to explain the internal properties of the black hole by considering its density as a function of the reciprocal of its radius and the temperature as a function of the reciprocal of the density. We then set the…

广义相对论与量子宇宙学 · 物理学 2021-12-07 J. Enrique H. Ramírez

We examine Schwarzschild black holes within the framework of gravitational thermodynamics, introducing an ``energy layer'' picture for black-hole mass-energy and exploring a possible energy-extraction mechanism termed…

广义相对论与量子宇宙学 · 物理学 2026-02-26 Wen-Xiang Chen

Spinning black holes create electromagnetic storms when immersed in ambient magnetic fields, illuminating the otherwise epically dark terrain. In an electromagnetic extension of the Penrose process, tremendous energy can be extracted,…

广义相对论与量子宇宙学 · 物理学 2021-11-17 Kshitij Gupta , Y. T. Albert Law , Janna Levin

It has been suggested that maximally spinning black holes can serve as particle accelerators, reaching arbitrarily high center-of-mass energies. Despite several objections regarding the practical achievability of such high energies, and…

广义相对论与量子宇宙学 · 物理学 2015-06-12 Sean T. McWilliams