Mergers and typical black hole microstates
By I. Bena, Chih-Wei Wang, N. Warner. 2006
192 citations recorded by the source corpus.
We use mergers of microstates to obtain the first smooth horizonless microstate solutions corresponding to a BPS three-charge black hole with a classically large horizon area. These microstates have very long throats, that become infinite in the classical limit; nevertheless, their curvature is everywhere small. Having a classically-infinite throat makes these microstates very similar to the typical microstates of this black hole. A rough CFT analysis confirms this intuition, and indicates a possible class of dual CFT microstates. We also analyze the properties and the merging of microstates corresponding to zero-entropy BPS black holes and black rings. We find that these solutions have the same size as the horizon size of their classical counterparts, and we examine the changes of internal structure of these microstates during mergers.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics
View Paper: https://www.semanticscholar.org/paper/084a80a22aca16ffb6f8b7b9f6b796ff65a8f444
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
- Marika Taylor
- N. Warner
- I. Bena
- Kostas Skenderis
- J. Boer
- S. El-Showk
- I. Messamah
- Vijay Balasubramanian
In Nuclear and High Energy Physics
In Statistical and Nonlinear Physics
- N. Warner
- Marika Taylor
- I. Bena
- Kostas Skenderis
- Vijay Balasubramanian
- S. El-Showk
- I. Messamah
- J. Boer
Citations in the corpus
- Quantizing N = 2 multicenter solutions (2008, background): “1 Scaling Solutions As noted in [35] and [15], for certain choices of charges it is possible to have points in the solution space where the coordinate distances between the centers goes to zero.”
- Global structure of five-dimensional fuzzballs (2013, background): “42) coming from individual bubbles, then [11, 30, 33]”
- Black holes as effective geometries (2008, background): “As noted in [35, 70], for certain choices of charges it is possible to have points in the solution space where the coordinate distances between the centres go to zero.”
- The fuzzball proposal for black holes (2008, background): “The bubbling geometries [93, 95, 96, 97, 98, 99, 100, 101, 102] are viewed as the most promising candidates for duals to typical black hole microstates.”
- Habemus superstratum! A constructive proof of the existence of superstrata (2015, background): “In the gravity dual, excitations with this energy gap are known to come from fluctuations of “deep, scaling” geometries in which the wavelength of the fluctuation is approximately the scale of the horizon [26, 70–72].”
- Wall crossing from Boltzmann black hole halos (2010, background): “Note that this also proves that scaling solutions [7, 49, 9], whose existence does not depend on the moduli, cannot exist for charges α1, .”
- Plumbing the Abyss: Black ring microstates (2007, methodology): “We thus obtain the analogs for black rings of the results that were found for black holes in [23].”
- Black holes, black rings and their microstates (2007, methodology): “One can learn more about reversible mergers of microstates in Section 6 of [34].”