3-charge geometries and their CFT duals

By S. Giusto, Samir D. Mathur, A. Saxena. 2004

222 citations recorded by the source corpus.

Abstract We consider two families of D1–D5–P states and find their gravity duals. In each case the geometries are found to ‘cap off’ smoothly near r = 0 ; thus there are no horizons or closed timelike curves. These constructions support the general conjecture that the interior of black holes is nontrivial all the way up to the horizon.

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

View Paper: https://www.semanticscholar.org/paper/29395b1633aa6b9b3793348c10580b2aa8c67b90

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

In Nuclear and High Energy Physics

In Statistical and Nonlinear Physics

Citations in the corpus

Black hole bound states in AdS(3) x S**2 (2008, background): “the (4,4) D1-D5 CFT, these geometries were further studied in detail in [47, 48].”
Bubbling supertubes and foaming black holes (2005, background): “In this limit, our solutions reduce to the bound state solutions constructed by Mathur and collaborators [5,6,7] by taking novel extremal limits of the non-extremal rotating three-charge black hole [34].”
The fuzzball proposal for black holes (2008, background): “In particular, one can generate certain 3-charge D1-D5-P geometries from 2-charge D1-D5 geometries in this way [86, 87, 68, 89].”
Comments on black holes I: the possibility of complementarity (2012, background): “String theory provides a microscopic explanation for the entropy of black holes [9], and the fuzzball structure of microstates provides a solution to the information paradox [10–31].”
Supersymmetric black rings and three-charge supertubes (2004, background): “This proposal has motivated a number of interesting studies on the D1-D5 system and supertubes [ 13 , 14, 15, 16, 17] including the first examples of non-singular three-charge supergravity supertubes without horizons [13, 14].”
Nonsupersymmetric smooth geometries and D1-D5-P bound states (2005, unknown): “sting that it be y→ y+ 2πR. We also have orbifolds similar to the two-charged ones if one or both of mand nare not relatively prime to k. In particular, the simple supersymmetric orbifolds studied in [23] correspond to taking m= kn′ + 1, n= kn′ for some integer n′.5 The preserved supersymmetries in ”
Plumbing the Abyss: Black ring microstates (2007, background): “These calculations have been very successful both for two-charge solutions [1,3], and for simple three-charge solutions [17].”
One Ring to Rule Them All ... and in the Darkness Bind Them (2004, methodology): “From both the Born–Infeld description of three-charge supertubes [2, 22] and from the physics of other three-charge geometries [1, 10, 17 , 23], we can see that three-charge solutions can also have brane dipole moments.”
The library of Babel: on the origin of gravitational thermodynamics (2005, methodology): “We also discuss particular observables which are more efficient at discriminating between different microstates, but argue against the feasibility of (1)Our work is related to the proposals of Mathur and others [6, 7, 8, 9, 10, 11, 12] in the context of the microstates of the D1-D5 system.”
Mergers and typical black hole microstates (2006, methodology): “It would be very interesting to examine this issue in greater depth by finding, at least approximate solutions to the wave equation in these backgrounds, or performing a time-of-flight analysis along the lines of [33,34,15].”
Supergravity microstates for BPS black holes and black rings (2005, methodology): “Thus the states [12] are in a subclass of the generic two pole solution.”
Black holes, black rings and their microstates (2007, background): “This is essentially what happens in the microstate solutions constructed and analyzed by [23, 24].”
Black holes as effective geometries (2008, background): “The first success was achieved in [14] which was followed by other works [106, 107, 111].”