Adding momentum to D1-D5 system
By O. Lunin. 2004
177 citations recorded by the source corpus.
We construct the first example of asymptotically flat solution which carries three charges (D1, D5 and momentum) and which is completely regular everywhere. The construction utilizes the relation between gravity solutions and spectral flow in the dual CFT. We show that the solution has the right properties to describe one of the microscopic states which are responsible for the entropy of the black hole with three charges.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics
View Paper: https://www.semanticscholar.org/paper/2bd842f3b6ab1ef1be984b4baa8afec719782526
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In Astronomy and Astrophysics
- N. Warner
- I. Bena
- S. El-Showk
- I. Messamah
- Vijay Balasubramanian
- Chih-Wei Wang
- Henriette Elvang
- Roberto Emparan
In Nuclear and High Energy Physics
- N. Warner
- I. Bena
- Vijay Balasubramanian
- S. El-Showk
- I. Messamah
- Chih-Wei Wang
- Henriette Elvang
- T. S. Levi
In Statistical and Nonlinear Physics
Citations in the corpus
- Black holes as effective geometries (2008, background): “Much of what will be discussed is a review of work by other authors [2, 6, 9, 11, 13, 14, 17] (see also the other references cited earlier and throughout the remainder of the text).”
- Supergravity microstates for BPS black holes and black rings (2005, background): “Recently, Mathur et al [11, 12, 13] uncovered some three charge supergravity solutions with no horizon (see also [14]).”
- Supersymmetric black rings and three-charge supertubes (2004, background): “ supertubes might similarly account for the microstates of supersymmetric five-dimensional black holes [12]. This proposal has motivated anumber of interesting studies on the D1-D5system andsupertubes [13, 14, 15, 16, 17] including the first examples of non-singular three-charge supergravity supertube”
- One Ring to Rule Them All ... and in the Darkness Bind Them (2004, background): “IosifB ena1 and N icholas P.W arner 2 1 Departm entofPhysicsand Astronom y University ofCalifornia LosAngeles,CA 90095,USA 2 Departm entofPhysicsand Astronom y University ofSouthern California LosAngeles,CA 90089,USA iosif@physics.ucla.edu, warner@usc.edu”
- Nonsupersymmetric smooth geometries and D1-D5-P bound states (2005, unknown): “ form played an important role in understanding the relation between these solutions and supertubes in [18] and in an attempt to generate new asymptotically flat three-charge solutions by spectral flow [35]. The supersymmetric three-charge solutions were also written in this form in [36]. Of course, i”
- 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.”
- 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].”
- Mergers and typical black hole microstates (2006, methodology): “This is essentially what happens in the microstate solutions constructed and analyzed by [13,14,15,16].”