54 research outputs found
Magnetised Kerr/CFT correspondence
The tools of Kerr/CFT correspondence are applied to the Kerr black hole
embedded in an axial external magnetic field. Its extremal near horizon
geometry remains a warped and twisted product of . The central
charge of the Virasoro algebra, generating the asymptotic symmetries of the
near horizon geometry, is found. It is used to reproduce, via the Cardy
formula, the Bekenstein-Hawking entropy of the magnetised Kerr black hole as
the statistical microscopic entropy of a dual CFT. The presence of the
background magnetic field makes available also a second dual CFT picture, based
on the electromagnetic symmetry, instead of the only rotational one of
the standard non-magnetised Kerr spacetime. A Meissner-like effect, where at
extremality the external magnetic field is expelled out of the black hole,
allows us to infer the value of the mass for these magnetised extremal black
holes. The generalisation to the CFT dual for the magnetised extreme
Kerr-Newman black hole is also presented.Comment: 16 pages, v4 final versio
CFT Duals for Accelerating Black Holes
The near horizon geometry of the rotating C-metric, describing accelerating
Kerr-Newman black holes, is analysed. It is shown that, at extremality, even
though not it is isomorphic to the extremal Kerr-Newman, it remains a warped
and twisted product of . Therefore the methods of the
Kerr/CFT correspondence can successfully be applied to build a CFT dual model,
whose entropy reproduce, through the Cardy formula, the Beckenstein-Hawking
entropy of the accelerating black hole. The mass of accelerating Kerr-Newman
black hole, which fulfil the first law of thermodynamics, is presented. Further
generalisation in presence of an external Melvin-like magnetic field, used to
regularise the conical singularity characteristic of the C-metrics, shows that
the Kerr/CFT correspondence can be applied also for the accelerating and
magnetised extremal black holes.Comment: 21 pages, published versio
Removal of conical singularities from rotating C-metrics and dual CFT entropy
We show how to remove from the rotating C-metric spacetime, which describes
accelerating Kerr black holes, both conical singularities. This can be done by
embedding the metric into a swirling gravitational universe, through a proper
Ehlers transformation. The spin-spin interaction between the external
rotational background and the black hole provides the source of the
acceleration without the need of rods or strings. The physical properties and
entropy of the new solution are studied using near horizon and dual conformal
techniques of the Kerr/CFT correspondence. The charged case is also analysed:
Accelerating Reissner-Nordstrom and Accelerating Kerr-Newman space-times
embedded in a swirling universe are also generated.Comment: 18 pages, no figure
Accelerating and Charged Type I Black Holes
A new, exact and analytical class of accelerating and charged black holes is
built, in the Einstein-Maxwell theory, thanks to the Harrison transformation.
The diagonal metric does not belong to the Petrov type D classification,
therefore it is not part of the Plebanski-Demianski spacetimes. The simplest
subcase of this family recovers the Reissner-Nordstrom black hole in the
vanishing acceleration limit and the standard C-metric in the limit of null
electric charge. More general cases can have two independent electric charges,
which can be tuned as desired, even to remain with an uncharged black hole,
such as Petrov Type I Schwarzschild, in an accelerating charged Rindler
background. Magnetic, dyonic and NUTty extensions are also discussed. Conical
singularities can be possibly removed in extremal configurations.Comment: 20 page
Hairy AdS black holes with a toroidal horizon in 4D Einstein-nonlinear -model system
An exact hairy asymptotically locally AdS black hole solution with a flat
horizon in the Einstein-nonlinear sigma model system in (3+1) dimensions is
constructed. The ansatz for the nonlinear field is regular everywhere
and depends explicitly on Killing coordinates, but in such a way that its
energy-momentum tensor is compatible with a metric with Killing fields. The
solution is characterized by a discrete parameter which has neither topological
nor Noether charge associated with it and therefore represents a hair. A
gauge field interacting with Einstein gravity can also be included. The
thermodynamics is analyzed. Interestingly, the hairy black hole is always
thermodynamically favored with respect to the corresponding black hole with
vanishing Pionic field.Comment: 15 pages, 1 figure. Accepted for publication in Physics Letters
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