A Note on D1-D5-J System and 5D Small Black Ring
Norihiro Iizuka, Masaki Shigemori

TL;DR
This paper explores the microscopic and macroscopic properties of the 5D small black ring, relating it to a 4D black hole via duality, and provides evidence for horizon formation due to stringy corrections, aligning microscopic and macroscopic entropies.
Contribution
It establishes a connection between 5D small black rings and 4D black holes, showing horizon formation and matching entropies through duality and stringy corrections.
Findings
The 4D-5D connection holds for small black objects.
Stringy R^2 corrections induce horizon formation.
Microscopic entropy matches macroscopic calculations.
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…
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