A Note on D1-D5-J System and 5D Small Black Ring

Abstract

The ``small'' black ring in 5D obtained by giving angular momentum to the D1-D5 system compactified on S^1 x K3 is a very interesting object in the sense that it does not have an event horizon in the supergravity limit whereas it microscopically has a finite entropy. The microscopic origin of this small black ring can be analyzed in detail since it is constructed by adding angular momentum to the well-studied D1-D5 system. On the other hand, its macroscopic, geometrical picture is difficult to study directly. In this note, by duality transformations and the 4D-5D connection, we relate this 5D small black ring to a 4D small non-rotating black hole, where the latter is known to develop a non-vanishing horizon due to stringy R^2 corrections to the supergravity action. This gives an indirect evidence that a non-vanishing horizon is formed for the 5D small black ring. We also show that the entropy of the 4D small black hole agrees with the microscopic entropy of the 5D small black ring, which supports that the 4D-5D connection is indeed valid even for small black objects.

12 pages, LaTeX. v2: minor corrections

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• Spinning Strings as Small Black Rings
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• Precision Microstate Counting of Small Black Rings
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• The Gravitational Description of Coarse Grained Microstates
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• A microstate for the 3-charge black ring
• Near the horizon of 5D black rings
• Journey to the Center of the Fuzzball
• Are There Four-Dimensional Small Black Rings?
• Higher-derivative corrections to small black rings
• Black rings with fourth dipole cause less hair loss
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