Journal
JOURNAL OF HIGH ENERGY PHYSICS
Volume -, Issue 10, Pages -Publisher
SPRINGER
DOI: 10.1007/JHEP10(2014)140
Keywords
Black Holes in String Theory; AdS-CFT Correspondence; Supergravity Models; D-branes
Categories
Funding
- Simons Foundation
- ERC Starting Independent Researcher Grant [240210-String-QCD-BH]
- John Templeton Foundation Grant: String Theory and the Anthropic Universe [48222]
- Foundational Questions Institute (FQXi) Fund [RFP3-1321]
- Japan Society for the Promotion of Science (JSPS) [24740159]
- DOE grant [DE-FG03-84ER-40168]
- Grants-in-Aid for Scientific Research [24740159] Funding Source: KAKEN
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There are, by now, several arguments that superstrata, which represent D1-D5-P bound states that depend upon arbitrary functions of two variables and that preserve four supersymmetries, exist in string theory, and that their gravitational back-reaction results in smooth horizonless solutions. In this paper we examine the shape and density modes of the superstratum and give strong evidence that the back-reacted supergravity solution allows for fluctuation modes whose quantization reproduces the entropy growth of black holes as a function of the charges. In particular, we argue that the shape modes of the superstratum that lie purely within the non-compact space-time directions account for at least of the entropy of the D1-D5-P black hole and propose a way in which the rest of the entropy could be captured by superstratum fluctuations. We complete the picture by conjecturing a relationship between bound states of multiple superstrata and momentum excitations of different twisted sectors of the dual CFT.
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