Energy absorption problem of a brane-world black hole

Liu, Lihui; Wang, Bin; Gao, Yang

doi:10.1103/physrevd.76.064014

Cited by 24 publications

(9 citation statements)

References 65 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…Recent investigations indicate that the extra dimension can imprint in the quasinormal modes originated from the perturbation around high dimensional black holes [1][2][3][4], which could be tested in the gravitational wave probe in the near future. Moreover, the spectrum of Hawking radiation from the high dimensional black holes could provide another possible way to observe the extra dimension, which is expected to be detected in particle accelerator experiments [5][6][7][8][9][10][11][12][13].…”

Section: Introductionmentioning

confidence: 99%

Strong gravitational lensing in a squashed Kaluza-Klein black hole spacetime

2010

View full text Add to dashboard Cite

We investigate the strong gravitational lensing in a Kaluza-Klein black hole with squashed horizons. We find the size of the extra dimension imprints in the radius of the photon sphere, the deflection angle, the angular position and magnification of the relativistic images. Supposing that the gravitational field of the supermassive central object of the Galaxy can be described by this metric, we estimated the numerical values of the coefficients and observables for gravitational lensing in the strong field limit.

show abstract

Section: Introductionmentioning

confidence: 99%

Strong gravitational lensing in a squashed Kaluza-Klein black hole spacetime

2010

View full text Add to dashboard Cite

show abstract

“…In addition a construction leading to an emergent gravity in a quantum field theory or a gauge theory has been proposed [9]. Interestingly, the near horizon black hole geometries have been explored on a BPS D-brane in type II superstring theories [11][12][13][14][15][16][17][18][19][20][21][22][23][24][25][26][27]. In the context, the external geometries on a D-brane sourced by a zero mode of a two form may be exploited further to address some of the non-external quantum black holes underlying generalized non-perturbation formalism.…”

Section: Introductionmentioning

confidence: 99%

Emergent Gravity/Non-linear U (1) Gauge Theory Correspondence

Pandey

Singh

et al. 2014

J Astrophys Aerospace Technol

View full text Add to dashboard Cite

We revisit a five dimensional Kaluza-Klein gravity, in presence of a cosmological constant, with a renewed interest in a type IIA string theory. An irreducible space-time curvature scalar K, leading to a non-perturbation theory of emergent quantum gravity, is addressed on a D 4-brane underlying a two form gauge theory. An appropriate ansatz for a two form in the non-linear U (1) gauge theory is explored to obtain a nontrivial geometric torsion in a second order formalism. The quantum geometries, underlying torsion, in a low energy limit is shown to describe an AdS 5-brane black hole in Einstein vacuum. In the limit, we analyze the non-perturbation curvature K on S 1 and argue for a plausible strong-weak coupling duality between a five dimensional non-perturbation curvature theory and the 4D perturbation non-linear gauge theory.

show abstract

“…These solutions carry a tidal charge instead of an electric charge, thereby transmitting the gravitational signature of the extra spacelike dimension into the four-dimensional world on the brane. Further developments in this direction can be found in [16,17,18,19,20,21,22,23,24,25].…”

Section: Introductionmentioning

confidence: 99%

Gravitational Effects of Rotating Braneworld Black Holes

Aliev,

Talazan

2009

Preprint

View full text Add to dashboard Cite

We study the light deflection effect and the relativistic periastron and frame-dragging precessions for a rotating black hole localized on the brane in the Randall-Sundrum braneworld scenario.Focusing on a light ray, which passes through the field of the black hole in its equatorial plane, we first calculate the deflection angle in the weak field limit. We obtain an analytical formula, involving the related perturbative parameters of the field up to the second order. We then proceed with the numerical calculation of the deflection angle in the strong field limit, when the light ray passes at the closest distance of approach to the limiting photon orbit. We show that the deflection angles for the light ray, winding maximally rotating Kerr and braneworld black holes in the same direction as their rotation, become essentially indistinguishable from each other for a specific value of the negative tidal charge. The same feature occurs in the relativistic precession frequencies at characteristic radii, for which the radial epicyclic frequency of the test particle motion attains its highest value. Thus, the crucial role in a possible identification of the maximally rotating Kerr and braneworld black holes would play their angular momentum, which in the latter case breaches the Kerr bound in general relativity. * Dedicated to Sergei Odintsov on the occasion of his fiftieth birthday.

show abstract

Energy absorption problem of a brane-world black hole

Cited by 24 publications

References 65 publications

Strong gravitational lensing in a squashed Kaluza-Klein black hole spacetime

Strong gravitational lensing in a squashed Kaluza-Klein black hole spacetime

Emergent Gravity/Non-linear U (1) Gauge Theory Correspondence

Gravitational Effects of Rotating Braneworld Black Holes

Contact Info

Product

Resources

About