An infinite-dimensional family of black-hole microstate geometries

被引:38
作者
Bena, Iosif [1 ]
Bobev, Nikolay [2 ]
Giusto, Stefano [3 ]
Ruef, Clement [1 ]
Warner, Nicholas P. [2 ]
机构
[1] CEA Saclay, CNRS, Inst Phys Theor, URA 2306, F-91191 Gif Sur Yvette, France
[2] Univ So Calif, Dept Phys & Astron, Los Angeles, CA 90089 USA
[3] Univ Genoa, Dipartimento Fis, I-16146 Genoa, Italy
关键词
Black Holes in String Theory; Models of Quantum Gravity; D-branes; FUZZBALL PROPOSAL;
D O I
10.1007/JHEP03(2011)022
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We construct the first explicit, smooth, horizonless black-hole microstate geometry whose moduli space is described by an arbitrary function of one variable and is thus infinite-dimensional. This is achieved by constructing the scalar Green function on a simple D6-(D6) over bar background, and using this Green function to obtain the fully back-reacted solution for a supertube with varying charge density in this background. We show that this supertube can store parametrically more entropy than in flat space, confirming the entropy enhancement mechanism that was predicted using brane probes. We also show that all the local properties of the fully back-reacted solution can, in fact, be obtained using the DBI action of an appropriate brane probe. In particular, the supergravity and the DBI analysis yield identical functional bubble equations that govern the relative locations of the centers. This indicates that there is a non-renormalization theorem that protects these functional equations as one moves in moduli space. Our construction creates configurations that are beyond the scope of recent arguments that appear to put strong limits on the entropy that can be found in smooth supergravity solutions.
引用
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页数:47
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