Concentric black rings

By J. Gauntlett, J. Gutowski. 2004

163 citations recorded by the source corpus.

We present new supersymmetric solutions of five-dimensional minimal supergravity that describe concentric black rings with an optional black hole at the common center. Configurations of two black rings are found which have the same conserved charges as a single rotating black hole; these black rings can have a total horizon area less than, equal to, or greater than the black hole with the same charges. A numerical investigation of these particular black-ring solutions suggests that they do not have closed timelike curves.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics

View Paper: https://www.semanticscholar.org/paper/3a877a2ac57378d35ed225dce4a00156a193f06f

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Citations in the corpus

Bicycling black rings (2007, background): “Supersymmetric versions of saturns, di-rings, bi-rings and many-ring systems can be constructed via superposition of the harmonic functions that characterize the individual black hole components of the system. This was first done for rings in [ 21 ].”
Black holes, black rings and their microstates (2007, background): “Adding more sources on the z axis corresponds to making concentric black rings [76, 55].”
Universal spectrum of 2d conformal field theory in the large c limit (2014, background): “These are similar to the enigmatic phases discussed in [28, 29] so we adopt this terminology.”
Black Holes in Higher Dimensions (2008, background): “Supersymmetric solutions describing stationary superpositions of multiple concentric black rings have also been constructed [99, 100].”
A classification of near-horizon geometries of extremal vacuum black holes (2008, background): “For Λ < 0 it was shown that it is a direct product (3)Our analysis also covers multi-black holes in the sense that one can take a near-horizon limit with respect to each connected component of the horizon – in this limit the effects of the other components of the horizon is lost (see [5] for a super”
General Concentric Black Rings (2004, methodology): “The S(1) direction of the rings all lie on an orbit of the tri-holomorphic Killing vector ∂5 and hence describe concentric rings (see [7] for further comments).”
Exotic Branes in String Theory (2012, background): “The black ring solution [88,89,98] is the manifestation of this puffing up actually occurring.”
Mergers and typical black hole microstates (2006, background): “1) and the standard approach to their constructing starts by taking the four-dimensional spatial base metric hmn to be that of flat R 4 [22,9,23,6,10,7].”
One Ring to Rule Them All ... and in the Darkness Bind Them (2004, methodology): “In [11], solutions describing concentric BPS black rings with arbitrary charges and dipole charges in a BMPV black-hole background were found, generalizing earlier equal-charge multi-BPS-black-ring solutions [ 12 ].”
Plumbing the Abyss: Black ring microstates (2007, background): “The classical un-bubbled solution to which this bubbled solution corresponds was first constructed in [37,45].”
Black Saturn (2007, methodology): “The supersymmetric concentric black hole - black ring solutions of [15] can be”
The phase transition between caged black holes and black strings (2004, background): “In [88] this point of view seems to have been accepted: “It was conjectured by Kol [14] that the nonuniform black strings should meet the squashed black holes at a point corresponding to a static solution with a singular horizon, and this appears to be the case [15].”
Supersymmetric black rings and three-charge supertubes (2004, methodology): “f regularity of the horizon (appendix D). N.B. While this paper was being written up, we learned of work on supersymmetric solutions of minimal supergravity describing multiple concentric black rings [21].2 2 Three-charge black supertube in M-theory The most symmetric realization of a supertube with”
Bubbling supertubes and foaming black holes (2005, unknown): “May, 2005”
The fuzzball proposal for black holes (2008, background): “In the case of hyper-Kähler base spaces with a U(1) isometry which is preserved, the equations can however be integrated [110].”