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相关论文: Dark Energy Effects on Charged and Rotating Black …

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The new, rapidly developing field of theoretical research --- studies of dark energy interacting with black holes (and, in particular, accreting onto black holes) --- is reviewed. The term `dark energy' is meant to cover a wide range of…

广义相对论与量子宇宙学 · 物理学 2014-06-11 E. O. Babichev , V. I. Dokuchaev , Yu. N. Eroshenko

The "lost" information of black hole through the Hawking radiation was discovered being stored in the correlation among the non-thermally radiated particles [Phys. Rev. Lett 85, 5042 (2000), Phys. Lett. B 675, 1 (2009)]. This correlation…

广义相对论与量子宇宙学 · 物理学 2018-05-22 Yu-Han Ma , Jin-Fu Chen , Chang-Pu Sun

The energy of a test particle orbiting a Schwarzschild black hole is quantized owing to the quantization of the angular momentum. For smallest stable circular orbit, the excitation energy is found to resemble closely the expression for the…

广义相对论与量子宇宙学 · 物理学 2012-09-19 Eugen Simanek

We investigate the effect of quantum correction on Hawking radiation for Schwarzschild black holes. We consider Hawking temperature and entropy to order G^2 and find that the area law of black holes should be modified. We think of Hawking…

广义相对论与量子宇宙学 · 物理学 2022-01-04 Yang Liu

Acoustic black holes are very interesting non-gravitational objects which can be described by the geometrical formalism of General Relativity. These models can be useful to experimentally test effects otherwise undetectable, as for example…

广义相对论与量子宇宙学 · 物理学 2015-06-25 S. Fagnocchi

We extend our previous analysis of the modification of the spectrum of black hole radiance due to the simplest and probably most quantitatively important back-reaction effect, that is self-gravitational interaction, to the case of charged…

高能物理 - 理论 · 物理学 2010-04-06 Per Kraus , Frank Wilczek

We derive the metric for a Schwarzschild black hole with global monopole charge by relaxing asymptotic flatness of the Schwarzschild field. We then study the effect of global monopole charge on particle orbits and the Hawking radiation. It…

广义相对论与量子宇宙学 · 物理学 2009-10-30 Naresh Dadhich , K. Narayan , U. A. Yajnik

We compute the effects on the temperature and precise spectrum of Hawking radiation from a Schwarzschild black hole when the emitted object is taken to be spatially extended. We find that in the low-momentum regime, the power emitted is…

高能物理 - 理论 · 物理学 2018-12-31 George Johnson , John March-Russell

Black holes, dark energy, and the Higgs field are all currently established, exciting, and mysterious, each in its own way. Cosmological data show that dark energy may evolve with time. The electroweak phase transition during stellar…

宇宙学与河外天体物理 · 物理学 2025-02-11 Steve P. Ahlen , James W. Rohlf , Gregory Tarlé

It has been shown that the nonthermal spectrum of Hawking radiation will lead to information-carrying correlations between emitted particles in the radiation. The mutual information carried by such correlations can not be locally observed…

广义相对论与量子宇宙学 · 物理学 2022-05-02 Yu-Xiao Liu , Yu-Han Ma , Yong-Qiang Wang , Shao-Wen Wei , Chang-Pu Sun

The problem of the existence of particles with negative energies inside and outside of Schwarzschild, charged and rotating black holes is investigated. Different definitions of the energy of the particle inside the Schwarzschild black hole…

广义相对论与量子宇宙学 · 物理学 2011-08-19 A. A. Grib , Yu. V. Pavlov

We investigate the effects of accretion of phantom energy onto primordial black holes. Since Hawking radiation and phantom energy accretion contribute to a {\it decrease} of the mass of the black hole, the primordial black hole that would…

广义相对论与量子宇宙学 · 物理学 2011-03-28 Mubasher Jamil , Asghar Qadir

In this paper we study the accretion of dark energy onto a black hole in the cases that dark energy is equipped with a positive cosmological constant and when the space-time is described by a Schwarzschild-de Sitter metric. It is shown…

广义相对论与量子宇宙学 · 物理学 2009-12-04 Prado Martín-Moruno , Az-Eddine L. Marrakchi , Salvador Robles-Pérez , Pedro F. González-Díaz

Limits on the dark matter fraction of small mass primordial black holes from Hawking radiation are predominantly derived from the assumption of a Schwarzschild black hole evaporating. However, astrophysical black holes are usually much more…

广义相对论与量子宇宙学 · 物理学 2026-04-03 Sebastian Schuster , Jessica Santiago , Justin Feng , Matt Visser

This study investigates the evaporation process of a Schwarzschild black hole, incorporating quantum corrections arising from conformal anomaly and vacuum polarization. We demonstrate that these corrections significantly alter the Hawking…

高能物理 - 理论 · 物理学 2026-05-26 Moslem Shafiee , Ahmad Sheykhi

We consider the effects of off-shell Hawking radiation on scattering processes involving black holes coupled to quantum fields. The focus here is to the case of gravitational scattering of a scalar field mediated by the exchange of virtual…

高能物理 - 理论 · 物理学 2020-11-25 Walter D. Goldberger , Ira Z. Rothstein

In this work, we examine the optical behaviors and thermodynamic phase structures using shadow analysis for four $\mathbb{S}\mathbb{T}\mathbb{U}$ black holes. The study is conducted for four cases of charge configurations on the parameter…

广义相对论与量子宇宙学 · 物理学 2025-03-25 Yassine Sekhmani , Dhruba Jyoti Gogoi , Ratbay Myrzakulov , Giuseppe Gaetano Luciano , Javlon Rayimbaev

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 study the Hawking radiation of black holes by considering the canonical typicality. For the universe consisting of black holes and their outer part, we directly obtain a non-thermal radiation spectrum of an arbitrary black hole from its…

量子物理 · 物理学 2018-06-21 Yu-Han Ma , Qing-Yu Cai , Hui Dong , Chang-Pu Sun

We consider the corrections due to quantum fluctuations of fields on charged black holes induced from the energy-momentum trace anomaly. Although the number of horizons stays unchanged and their positions receive only finite corrections,…

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