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In a recent letter, the authors presented a unified derivation of the electric Schwinger effect and a generalized Hawking effect with an additional radiation component. The approach discloses a radial profile of black hole pair production…

广义相对论与量子宇宙学 · 物理学 2025-02-26 Michael F. Wondrak , Walter D. van Suijlekom , Heino Falcke

We present a new avenue to black hole evaporation using a heat-kernel approach analogous as for the Schwinger effect. Applying this method to an uncharged massless scalar field in a Schwarzschild spacetime, we show that spacetime curvature…

广义相对论与量子宇宙学 · 物理学 2023-06-05 Michael F. Wondrak , Walter D. van Suijlekom , Heino Falcke

We summarise recent work on the quantum production of black holes in the inflationary era. We describe, in simple terms, the Euclidean approach used, and the results obtained both for the pair creation rate and for the evolution of the…

广义相对论与量子宇宙学 · 物理学 2011-04-15 Raphael Bousso , Stephen W. Hawking

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

We investigate the general process of black hole pair creation in a cosmological background, considering the creation of charged and rotating black holes. We motivate the use of Kerr-Newmann-deSitter solutions to investigate this process,…

广义相对论与量子宇宙学 · 物理学 2009-10-31 I. S. Booth , R. B. Mann

It is well known that massive black holes may form through the gravitational collapse of a massive astrophysical body. Less known is the fact that a black hole can be produced by the quantum process of pair creation in external fields.…

广义相对论与量子宇宙学 · 物理学 2017-08-23 Oscar J. C. Dias

We investigate the effects of pair creation on the internal geometry of a black hole, which forms during the gravitational collapse of a charged massless scalar field. Classically, strong central Schwarzschild-like singularity forms, and a…

广义相对论与量子宇宙学 · 物理学 2014-11-17 Evgeny Sorkin , Tsvi Piran

Primordial black holes are considered to be pair created quantum-mechanically during inflation. In the context of General Relativity (GR), it has been shown that the pair creation rate is exponentially decreasing during inflation.…

广义相对论与量子宇宙学 · 物理学 2018-06-27 Konstantinos F. Dialektopoulos , Antonios Nathanail , Athanasios G. Tzikas

This is the second paper in a series where we examine the physics of pair producing gaps in low-luminosity accreting supermassive black hole systems. In this paper, we carry out time-dependent self-consistent fully general relativistic 1D…

高能天体物理现象 · 物理学 2020-06-10 Alexander Y. Chen , Yajie Yuan

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. A simple analytical formulation predicts that…

高能物理 - 理论 · 物理学 2007-05-23 D. G. Coyne

The probability for quantum creation of an inflationary universe with a pair of black holes is computed in a modified gravitational theory. Considering a gravitational action which includes a cosmological constant ($\Lambda$) in addition to…

高能物理 - 理论 · 物理学 2008-11-26 B. C. Paul , Dilip Paul

Electron-positron pairs may be produced near accreting black holes by a variety of physical processes, and the resulting pair plasma may be accelerated and collimated into a relativistic jet. Here we use a self-consistent dynamical and…

高能天体物理现象 · 物理学 2015-05-27 Monika Moscibrodzka , Charles F. Gammie , Joshua C. Dolence , Hotaka Shiokawa

We analyze the possibility of black holes pair creation induced by three dimensional wormholes. Although this spacetime configuration is nowadays hard to suppose, it can be very important in the early universe, when the wormhole spacetime…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Remo Garattini

The Weak Gravity Conjecture (WGC) is usually formulated in terms of the stability of extremal black-holes or in terms of long distance Coulomb/Newton potentials. However one can think of other physical processes to compare the relative…

高能物理 - 理论 · 物理学 2020-12-30 Eduardo Gonzalo , Luis E. Ibáñez

We conjecture that the neutral black hole pair production is related to the vacuum fluctuation of pure gravity via the Casimir-like energy. Implications on the foam-like structure of spacetime are discussed.

广义相对论与量子宇宙学 · 物理学 2009-10-31 Remo Garattini

In this talk I presented a previously published work concerning the evaporation of (4+n)-dimensional non-rotating black holes into gravitons. In this work we calculated the energy emission rate for gravitons in the bulk obtaining analytical…

高能物理 - 理论 · 物理学 2008-11-26 O. Efthimiou

The pair-production process for a black hole (BH) is discussed within the framework of a recently proposed semiclassical model of BH evaporation. Our emphasis is on how the requirements of unitary evolution and strong subadditivity act to…

高能物理 - 理论 · 物理学 2015-03-19 Ram Brustein , A. J. M. Medved

Spontaneous pair production from background fields or spacetimes is one of the most prominent phenomena predicted by quantum field theory. The Schwinger mechanism of production of charged pairs by a strong electric field and the Hawking…

高能物理 - 理论 · 物理学 2016-11-28 Sang Pyo Kim

I consider a truncation of low-energy string theory which contains two $U(1)$ gauge fields. After making some general comments on the theory, I describe a previously-obtained instanton for the pair creation of black holes when both gauge…

广义相对论与量子宇宙学 · 物理学 2009-10-28 Simon F. Ross

Black holes came into existence together with the universe through the quantum process of pair creation in the inflationary era. We present the instantons responsible for this process and calculate the pair creation rate from the no…

广义相对论与量子宇宙学 · 物理学 2009-07-09 Raphael Bousso , Stephen W. Hawking
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