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相关论文: Charge Influence On Mini Black Hole's Cross Sectio…

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The cross section for black hole production in hadron colliders is calculated using a factorization hypothesis in which the parton-level process is integrated over the parton density functions of the protons. The mass, spin, charge, colour,…

高能物理 - 唯象学 · 物理学 2010-10-27 Douglas M. Gingrich

We study black hole formation in the head-on collision of ultrarelativistic charges. The metric of charged particles is obtained by boosting the Reissner-Nordstr\"om spacetime to the speed of light. Using the slice at the instant of…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Hirotaka Yoshino , Robert B. Mann

Black hole production at the Large Hadron Collider (LHC) is an interesting consequence of TeV-scale gravity models. The predicted values, or lower limits, for the fundamental Planck scale and number of extra dimensions will depend directly…

高能物理 - 唯象学 · 物理学 2010-11-03 Douglas M. Gingrich

Possible consequences of the production of small black holes at the LHC for different scenarios with large extra dimensions are investigated. The effects from black hole production on some standard jet observables are examined,…

高能物理 - 唯象学 · 物理学 2009-11-11 Leif Lonnblad , Malin Sjodahl , Torsten Akesson

We analyse the formation and evolution of the event horizon of a black hole binary merger when the black holes are charged. We find that the presence of charge influences the properties of the merger and can be useful for investigating the…

广义相对论与量子宇宙学 · 物理学 2022-04-20 D. Marín Pina , M. Orselli , D. Pica

We study exact stationary and axisymmetric solutions describing charged rotating black holes localized on a 3-brane in the Randall-Sundrum braneworld. The charges of the black holes are considered to be of two types, the first being an…

高能物理 - 理论 · 物理学 2009-11-11 A. N. Aliev , A. E. Gumrukcuoglu

The Galactic centre supermassive black hole (SMBH), in sharp contrast with its complex environment, is characterized by only three classical parameters -- mass, spin, and electric charge. Its charge is poorly constrained. It is, however,…

星系天体物理 · 物理学 2018-08-24 Michal Zajaček , Arman Tursunov , Andreas Eckart , Silke Britzen

We perform fully non-linear numerical simulations of charged-black-hole collisions, described by the Einstein-Maxwell equations, and contrast the results against analytic expectations. We focus on head-on collisions of non-spinning black…

广义相对论与量子宇宙学 · 物理学 2012-07-06 Miguel Zilhão , Vitor Cardoso , Carlos Herdeiro , Luis Lehner , Ulrich Sperhake

The effects of the tidal charge of black holes predicted in the Randall-Sundrum brane-world scenario on the electromagnetic cross sections and emission rate is studied. Although quantitatively different, the cross sections and emission…

广义相对论与量子宇宙学 · 物理学 2020-11-04 Ednilton S. de Oliveira

The first fully non-linear numerical simulations of colliding charged black holes in D=4 Einstein-Maxwell theory were recently reported arXiv:1205.1063. These collisions were performed for black holes with equal charge-to-mass ratio, for…

广义相对论与量子宇宙学 · 物理学 2014-02-19 Miguel Zilhão , Vitor Cardoso , Carlos Herdeiro , Luis Lehner , Ulrich Sperhake

Though a black hole can theoretically possess a very big charge ($Q/(\sqrt{G} M) \simeq 1$), the charge of the real astrophysical black holes is usually considered to be negligible. This supposition is based on the fact that an…

高能天体物理现象 · 物理学 2010-01-06 A. N. Baushev , P. Chardonnet

Based on the idea that tensor unparticles can enhance the gravitational interactions between standard model particles, potential black hole formation in high energy collisions is examined. Modifications to the horizon radius $r_H$ are…

高能物理 - 唯象学 · 物理学 2008-11-26 J. R. Mureika

To study the dynamics of discharge of a brane black hole in TeV gravity scenarios, we obtain the approximate electromagnetic field due to the charged black hole, by solving Maxwell's equations perturbatively on the brane. In addition,…

高能物理 - 理论 · 物理学 2011-08-02 Marco O. P. Sampaio

In models of minicharged dark matter associated with a hidden $U(1)$ symmetry, astrophysical black holes may acquire a "dark" charge, in such a way that the inspiral dynamics of binary black holes can be formally described by an…

广义相对论与量子宇宙学 · 物理学 2021-09-29 Pawan Kumar Gupta , Thomas F. M. Spieksma , Peter T. H. Pang , Gideon Koekoek , Chris Van Den Broeck

Microscopic black hole production at future hadron colliders is a promising avenue to explore low scale gravity models like ADD. This study investigates production cross-sections and final state properties of these black holes using the…

高能物理 - 唯象学 · 物理学 2024-04-17 Halil Gamsızkan

We perform numerical-relativity simulations of high-energy head-on collisions of charged black holes with the same charge-to-mass ratio $\lambda$. We find that electromagnetic interactions have subdominant effects already at low Lorentz…

广义相对论与量子宇宙学 · 物理学 2022-02-14 Gabriele Bozzola

The generalization of the black hole in three-dimensional spacetime to include an electric charge Q in addition to the mass M and the angular momentum J is given. The field equations are first solved explicitly when Q is small and the…

高能物理 - 理论 · 物理学 2009-10-31 Cristian Martinez , Claudio Teitelboim , Jorge Zanelli

Computations in general relativity have revealed an interesting phase diagram for the black hole - black string phase transition, with three different black objects present for a range of mass values. We can add charges to this system by…

高能物理 - 理论 · 物理学 2008-11-26 Borun D. Chowdhury , Stefano Giusto , Samir D. Mathur

We examine the rates for the production of black holes(BH) at the LHC in light of the exponential suppression of the geometric cross section estimate recently proposed by Voloshin. We show that the resulting production rates will still be…

高能物理 - 唯象学 · 物理学 2014-11-17 Thomas G. Rizzo

Charged Black holes in Gauss-Bonnet extended gravity are studied. The electromagnetic field is coupled non-minimally, as in U(2,2) Chern-Simons theory. We find that the geometrical properties of the solution exhibit ``phase transitions" as…

高能物理 - 理论 · 物理学 2010-11-19 Maximo Banados
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