Hawking Radiation from a (4+n)-Dimensional Rotating Black Hole on the Brane

  title={Hawking Radiation from a (4+n)-Dimensional Rotating Black Hole on the Brane},
  author={Christopher M. Harris and Panagiota Kanti},
  journal={Physics Letters B},

Figures from this paper

Brane decay of a (4+n)-dimensional rotating black hole: spin-0 particles

In this work, we study the ‘scalar channel’ of the emission of Hawking radiation from a (4+ n )-dimensional, rotating black hole on the brane. We numerically solve both the radial and angular part of

Brane decay of a (4+n)-dimensional rotating black hole. III: spin-1/2 particles

In this work, we study the `scalar channel' of the emission of Hawking radiation from a (4+n)-dimensional, rotating black hole on the brane. We numerically solve both the radial and angular part of

Bulk Decay of (4 + n)-Dimensional Simply Rotating Black Holes: Tensor-Type Gravitons

We study the emission in the bulk of tensor-type gravitons by a simply rotating (4 + n)-dimensional black hole. The decoupling of the radial and angular part of the graviton field equation makes it

Greybody factors in a rotating black-hole background: Fermions and gauge bosons

We study the emission of fermion and gauge boson degrees of freedom on the brane by a rotating higher-dimensional black hole. Using matching techniques, for the near-horizon and far-field regime

Greybody factors for brane scalar fields in a rotating black hole background

We study the evaporation of ($4+n$)-dimensional rotating black holes into scalar degrees of freedom on the brane. We calculate the corresponding absorption probabilities and cross sections obtaining

Charge and mass effects on the evaporation of higher-dimensional rotating black holes

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

Hawking Radiation from Higher-Dimensional Black Holes

We review the quantum field theory description of Hawking radiation from evaporating black holes and summarize what is known about Hawking radiation from black holes in more than four space-time

Angular profile of particle emission from a higher-dimensional black hole: analytic results

A bstractDuring the spin-down phase of the life of a higher-dimensional black hole, the emission of particles on the brane exhibits a strong angular variation with respect to the rotation axis of the



Hawking radiation from a (4+n)-dimensional black hole: exact results for the Schwarzschild phase

We start our analysis by deriving a master equation that describes the motion of a field with arbitrary spin s on a 3-brane embedded in a non-rotating, uncharged (4+n)-dimensional black hole

Black Holes in Theories with Large Extra Dimensions

We start by reviewing the existing literature on the creation of black holes during high-energy particle collisions, both in the absence and in the presence of extra, compact, spacelike dimensions.

Black hole as a point radiator and recoil effect on the brane world.

A field theory model is constructed in which a small black hole attached to a brane in a higher-dimensional space emitting quanta into the bulk may leave the brane as a result of a recoil, and the thermal emission of the black holes could be terminated and the energy nonconservation can be observed in theBrane experiments.

Quantum Radiation from a 5-Dimensional Rotating Black Hole

We study a massless scalar field propagating in the background of a five-dimensional rotating black hole. We show that in the Myers-Perry metric describing such a black hole the massless field

Calculable Corrections to Brane Black Hole Decay II: Greybody Factors for Spin 1/2 and 1

The production of black holes in extra-dimensional brane-world theories can lead to detectable signals via the Hawking evaporation of the black hole to brane-localized standard model modes. We

Black hole radiation in the brane world and the recoil effect

A black hole attached to a brane in a higher dimensional space emitting quanta into the bulk may leave the brane as a result of a recoil. We study this effect. We consider black holes which have a

Black holes radiate mainly on the brane.

It is shown that the masses of many Kaluza-Klein modes are much smaller than the Hawking temperature of the black hole, and this raises the possibility of observing Hawking radiation in future high energy colliders if there are large extra dimensions.

Rotating black holes at future colliders: Greybody factors for brane fields

We study theoretical aspects of the rotating black hole production and evaporation in the extra dimension scenarios with TeV scale gravity, within the mass range in which the higher dimensional Kerr

Calculable corrections to brane black hole decay: The scalar case

It is a remarkable fact that in brane-world theories the true scale M * of quantum gravity may be substantially lower than the traditional Planck scale M pl , possibly approaching the TeV scale, and

High-energy colliders as black hole factories: The End of short distance physics

If the fundamental Planck scale is of order of a TeV, as is the case in some extra-dimension scenarios, future hadron colliders such as the CERN Large Hadron Collider will be black hole factories.