Nonsupersymmetric smooth geometries and D1-D5-P bound states

By Vishnu Jejjala, Owen Madden, S. Ross, Georgina Titchener. 2005

237 citations recorded by the source corpus.

We construct smooth nonsupersymmetric soliton solutions with D1-brane, D5-brane, and momentum charges in type IIB supergravity compactified on ${T}^{4}\ifmmode\times\else\texttimes\fi{}{S}^{1}$, with the charges along the compact directions. This generalizes previous studies of smooth supersymmetric solutions. The solutions are obtained by considering a known family of $U(1)\ifmmode\times\else\texttimes\fi{}U(1)$ invariant metrics, and studying the conditions imposed by requiring smoothness. We discuss the relation of our solutions to states in the CFT describing the D1-D5 system and describe various interesting features of the geometry.

Subfields: Astronomy and Astrophysics, Mathematical Physics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/fe885c5adaadcb335d2f3f882c3124f480c377db

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Citations in the corpus

Black holes, black rings and their microstates (2007, methodology): “The most direct support for the smooth microstate structure of non-extremal black holes would be the construction and counting of smooth, non-extremal geometries generalizing those presented here, like those constructed in [ 74 ].”
Plumbing the Abyss: Black ring microstates (2007, background): “for a review), and there is now very signiﬁcant progress on the three-charge system (see [14–25] and [26] for a review), as well as for the four-dimensional [27–31] and non-BPS black-hole microstates [32,33]. One of the key steps in understanding three-charge microstate geometries was the realizatio”
The library of Babel: on the origin of gravitational thermodynamics (2005, background): “eometry with complex topological structures (diﬀerent S3s expanding) spaced randomly in the x1–x2 plane. We might call this a classical foam. 22Similar comments apply to the non-singular solutions of [6, 7, 8, 11, 12] in the D1-D5 setting. 47 However, because the typical structures will be at the ~ ”
Black holes as effective geometries (2008, background): “On the other hand, less work has been done on non-BPS solutions [ 119 ,120,121,122,94].”
Comments on black holes I: the possibility of complementarity (2012, background): “For simple microstates this radiation has been explicitly computed, and it arises from ‘ergoregion emission’ [50–54] near the boundary.”
Global structure of five-dimensional fuzzballs (2013, methodology): “The approach to finding this soliton is rather reminiscent of the construction of the soliton in [104–106] except that the solution of [104] is only regular in six dimensions while the solution of [105, 106, 110] are smooth in five dimensions.”
Supergravity microstates for BPS black holes and black rings (2005, background): “In [15] some finite temperature (non-supersymmetric) generalizations appear for these which correspond to black holes with finite size horizons; we are interested in finding microstates for BPS black holes which have already have finite size horizons for zero temperature.”
Bubbling supertubes and foaming black holes (2005, methodology): “The generic microstate solution is specified by a four-dimensional hyper-Kähler geometry of a certain signature, and contains a “foam” of non-trivial two-spheres.”