Gravity solutions for the D1-D5 system with angular momentum
By O. Lunin, J. Maldacena, Liat Maoz. 2002
319 citations recorded by the source corpus.
We construct a large family of supergravity solutions that describe BPS excitations on AdS_3 x S^3 with angular momentum on S^3. These solutions take into account the full backreaction on the metric. We find that as we increase the energy of the excitation, the energy gap to the next non-BPS excitation decreases. These solutions can be viewed as Kaluza-Klein monopole ``supertubes'' which are completely non-singular geometries. We also make some remarks on supertubes in general.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/1ccfec01821351181710fc0c2a97436143d5d57a
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
- N. Warner
- I. Bena
- V. Hubeny
- Marika Taylor
- Kostas Skenderis
- Roberto Emparan
- M. Rangamani
- Vijay Balasubramanian
In Nuclear and High Energy Physics
- N. Warner
- I. Bena
- V. Hubeny
- Marika Taylor
- Kostas Skenderis
- J. Maldacena
- Ashoke Sen
- Vijay Balasubramanian
Citations in the corpus
- 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].”
- Black holes as effective geometries (2008, background): “In [7] it was shown that the geometries corresponding to a classical curve are regular provided |F′(s)| is different from 0 and the curve is not self-intersecting.”
- Global structure of five-dimensional fuzzballs (2013, background): “Mathur and collaborators went on to demonstrate that these fuzzball geometries could reproduce many of the properties of BPS black holes and of near-BPS black holes (see [1, 5, 6] for further discussion of this).”
- The Search for a Holographic Dual to AdS(3)xS(3)xS(3)xS(1) (2004, background): “It is possible that these states correspond to conical defect geometries smoothed out into supertubes, along the lines described in [27].”
- Bubbling supertubes and foaming black holes (2005, background): “However, based on the microscopic description of supertubes [35,36,18] we expect the solutions that correspond to multiple supertubes to be dual to CFT states with longer effective strings than the solutions that come from only one supertube.”
- Supersymmetric black rings and three-charge supertubes (2004, background): “at the non-singular, horizon-free supergravity solutions describing these objects are in one-to-one correspondence with the Ramond-sector ground states of the supersymmetric D1-D5 string intersection [9, 10, 11]. It has been conjectured that supergravity solutions for three-charge supertubes might s”
- Nonsupersymmetric smooth geometries and D1-D5-P bound states (2005, unknown): “It has been shown in [34] that the general supersymmetric solution in minimal six-dimensional supergravity could be written as a fibration over a four-dimensional hyper-K¨ahler base, and writing the supersymmetric two-charge solutions in this form played an important role in understanding the relati”
- Fuzzballs with internal excitations (2007, methodology): “1 Introduction Over the last few years an interesting new proposal for the gravitational nature of black hole microstates has emerged [1, 2, 3]; see also [4, 5, 6], and [7].”
- Adding momentum to D1-D5 system (2004, methodology): “It is interesting that for a somewhat simpler system which has only two charges (D1 and D5, but no momentum), one can actually construct the geometries corresponding to all microscopic states [5, 6].”
- The Phase Structure of Higher-Dimensional Black Rings and Black Holes (2007, background): “These integrals take simple forms only when n is odd [41], while for even n they involve elliptic functions [42].”
- One Ring to Rule Them All ... and in the Darkness Bind Them (2004, background): “Unlike the two-charge supertube solutions [8, 24, 25 , 26], these solutions cannot be found by usual solution generating techniques because the three charges can be generically dissolved into fluxes (as in the Klebanov–Strassler solution [21]).”