Metric of the multiply wound rotating string

By O. Lunin, Samir D. Mathur. 2001

283 citations recorded by the source corpus.

Abstract We consider a string wrapped many times around a compact circle in space, and let this string carry a right-moving wave which imparts momentum and angular momentum to the string. The angular momentum causes the strands of the ‘multiwound’ string to separate and cover the surface of a torus. We compute the supergravity solution for this string configuration. We map this solution by dualities to the D1–D5 system with angular momentum that has been recently studied. We discuss how constructing this multiwound string solution may help us to relate the microscopic and macroscopic pictures of black hole absorption.

Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/7bd5693a62669a8fc33a176c35924a115ffd7dfd

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In Astronomy and Astrophysics

1. N. Warner
2. I. Bena
3. Marika Taylor
4. Kostas Skenderis
5. J. Boer
6. S. Raju
7. Vijay Balasubramanian
8. S. El-Showk

In Atomic and Molecular Physics, and Optics

1. Marika Taylor
2. Ingmar Kanitscheider
3. N. Warner
4. I. Bena
5. D. Mateos
6. S. Raju
7. Kostas Skenderis
8. S. El-Showk

In Nuclear and High Energy Physics

1. N. Warner
2. I. Bena
3. Marika Taylor
4. Kostas Skenderis
5. Vijay Balasubramanian
6. S. El-Showk
7. S. Raju
8. J. Boer

Citations in the corpus

• Supersymmetric black rings and three-charge supertubes (2004, background): “6]. 12These ¯r, θ¯ are the same as introduced in the near-horizon study of appendix D. 24 6.3 Simpler supertubes 6.3.1 Two charges and one dipole The original supergravity supertube solutions in D= 5 [36, 37, 7] correspond to setting Q3 = 0 and therefore q1 = q2 = 0. In this case Jφ = 0 and Jψ = (π/”
• Fuzzballs with internal excitations (2007, background): “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].”
• Black holes as effective geometries (2008, methodology): “The authors are very grateful to Eric Gimon for providing useful feedback on these notes and to Samir Mathur for some insightful discussions.”
• Holographic anatomy of fuzzballs (2006, background): “over the last few years [1, 2, 3]; see also [ 4 , 5, 6], and [7] for a review.”
• Lessons from the information paradox (2020, background): “These solutions are called “microstate geometries”, and large and interesting classes of these solutions have been found, starting with [227, 228], and including the recent multi-charge solutions [229–231].”
• One Ring to Rule Them All ... and in the Darkness Bind Them (2004, background): “For the D1–D5 system, the smooth bulk supergravity solutions dual to microstates of the boundary CFT have been classified and shown to precisely account for the entropy of this theory [24].”
• Supergravity microstates for BPS black holes and black rings (2005, background): “Recently, Mathur and Lunin have made a stronger conjecture [9] (see [10] for a recent review) which holds that black hole microstates are characterized by string theory backgrounds with no horizons.”
• Quantizing N = 2 multicenter solutions (2008, background): “In some cases, notably for half-BPS states in N = 4 SYM [2][3] and for half-BPS states in the D1-D5 system [4] one can do much better and show that the phase space of classical smooth supergravity solutions with the same quantum numbers as the black hole agrees with (the supersymmetric sector of) th”
• Exotic Branes in String Theory (2012, unknown): “The tension of the product brane, F1(ψ), is T ∼ 1/α′, while the size of the puffed up configuration is R ∼ α′1/2 [91].”
• Gravity solutions for the D1-D5 system with angular momentum (2002, unknown): “Solutions in different dimensions In order to analyze such systems, we start with the F1-P1 system in R1,d×S1×T 8−d (with the appropriate powers in the harmonic functions) , integrate the string sources along a ring (as explained in [21]), and then perform some dualities on it to get the desired sys”
• The fuzzball proposal for black holes (2008, background): “Thus the harmonic functions appropriate for describing strings with only bosonic condensates are [61]”
• 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.”
• Nonsupersymmetric smooth geometries and D1-D5-P bound states (2005, unknown): “s were constructed in [15, 16], and correspond to the Ramond-Ramond (RR) ground state obtained by spectral flow from the Neveu-Schwarz–Neveu-Schwarz (NSNS) vacuum state. This was subsequently extended [17, 10, 18] to find a family of smooth geometries corresponding to the whole family of RR ground sta”
• An infalling observer in AdS/CFT (2012, background): “It is useful to consider the example of 2-charge solutions [5, 4] which can be identified with the Ramond ground states of the D1−D5 CFT.”
• Black holes, black rings and their microstates (2007, background): “Upon dualizing, the shape of the momentum wave on the F1 string can be mapped into the shape of the supertube [17].”