Supersymmetric black rings and three-charge supertubes

By Henriette Elvang, Roberto Emparan, D. Mateos, Harvey Reall. 2004

257 citations recorded by the source corpus.

We present supergravity solutions for $1/8$-supersymmetric black supertubes with three charges and three dipoles. Their reduction to five dimensions yields supersymmetric black rings with regular horizons and two independent angular momenta. The general solution contains seven independent parameters and provides the first example of nonuniqueness of supersymmetric black holes. In ten dimensions, the solutions can be realized as D1-D5-P black supertubes. We also present a worldvolume construction of a supertube that exhibits three dipoles explicitly. This description allows an arbitrary cross section but captures only one of the angular momenta.

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

View Paper: https://www.semanticscholar.org/paper/80c294a6467f97ec2b61b66f3e9d90067f88d8b2

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Citations in the corpus

Global structure of five-dimensional fuzzballs (2013, background): “It is fairly common to go to a system of units in which the five-dimensional Planck length, 5, is unity and this means (see, for example, [98, 99]): G5 = π 4 .”
Black holes as effective geometries (2008, methodology): “As we have defined it the fuzzball proposal does not follow from AdS/CFT.”
Black Saturn (2007, background): “CTCs tend to appear when solutions are over-spinning, at least that is the case for supersymmetric black holes [36, 31, 32, 33, 15].”
A classification of near-horizon geometries of extremal vacuum black holes (2008, background): “In recent years, great progress has been made in the construction of supersymmetric black holes both in ungauged supergravity [1–9] and gauged supergravity [10–16], largely due to systematic classification techniques available for BPS solutions [1, 11, 17].”
Bicycling black rings (2007, background): “This is similar to the case of supersymmetric black rings [32, 33, 34, 21].”
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].”
Black hole bound states in AdS(3) x S**2 (2008, background): “A similar situation was encountered for instance in [35], where a similar decoupling limit is defined for the three charge super tubes.”
One Ring to Rule Them All ... and in the Darkness Bind Them (2004, background): “Note added: A day after this paper appeared on the arxiv, two more papers appeared that overlap with our section 4. In [ 9 ], the solution describing a circular BPS black ring with three charges and three-dipole charge was found and analyzed.”
Black hole entropy function, attractors and precision counting of microstates (2007, methodology): “The entropy function method can also be used to compute entropies of higher dimensional black holes with non-spherical horizons where such solutions are known to exist even for two derivative action [41, 42].”
Plumbing the Abyss: Black ring microstates (2007, background): “Note that because of the infinite non-uniqueness of BPS black rings [35,36,37], a solution with black ring charges and angular momenta is not necessarily a black ring microstate.”
The fuzzball proposal for black holes (2008, background): “Let us now consider the supersymmetric black rings found and analyzed in [112, 110, 88, 113, 111].”
Exotic Branes in String Theory (2012, background): “The black ring solution [88,89,98] is the manifestation of this puffing up actually occurring.”
Nonsupersymmetric smooth geometries and D1-D5-P bound states (2005, unknown): “ semi-classical picture of a black hole [14]. 2Three-charge states were previously studied in the supertube description [24, 25] in [26, 27]. Othersupersymmetricthree-chargesolutionshavebeen found in [28, 29, 30], but the regularsolutions have not yet been identiﬁed or related to CFT states. 3We sho”
Black holes, black rings and their microstates (2007, background): “One is to take a near-horizon limit in which the black ring solution becomes asymptotically AdS3 × S(3) × T 4 [54, 37], and to describe the ring in the D1-D5-P CFT dual to this system.”
Bubbling supertubes and foaming black holes (2005, methodology): “A side-effect of the study of three-charge supertubes was the prediction [9,14] and subsequent discovery [15,11,16,17] of BPS black rings, which by themselves have opened up new windows into black-hole physics [18–29].”
Non-supersymmetric attractors (2005, background): “3), is consistent with the near horizon geometries of the solutions of [55, 56, 57, 58] as discussed in section 5.”
Black Holes in Higher Dimensions (2008, background): “This was then generalized to a supersymmetric black ring solution of the U(1)(3) supergravity in [106, 107, 108].”
Supergravity microstates for BPS black holes and black rings (2005, methodology): “If we use the nomenclature in [5], we see that the parameters qi which appear in the expression for the horizon area only appear as R(2)qi in the asymptotics, where R is the inner radius of the ring.”