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Cited by 176

The DOI matches its Crossref record; 2 of the 2 references it cites were found in a registry or an index.

Strings as solitons & black holes as strings

Open access
Dabholkar, Atish, Gauntlett, Jerome P., Harvey, Jeffrey A., Waldram, Daniel·1996·Nuclear Physics B

Abstract

Abstract Supersymmetric closed string theories contain an infinite tower of BPS-saturated, oscillating, macroscopic strings in the perturbative spectrum. When these theories have dual formulations, this tower of states must exist nonperturbatively as solitons in the dual theories. We present a general class of exact solutions of low-energy supergravity that corresponds to all these states. After dimensional reduction they can be interpreted as supersymmetric black holes with a degeneracy related to the degeneracy of the string states. For example, in four dimensions we obtain a point-like solution which is asymptotic to a stationary, rotating, electrically-charged black hole with Regge-bounded angular momentum and with the usual ring-singularity replaced by a string source. This further supports the idea that the entropy of supersymmetric black holes can be understood in terms of counting of string states. We also discuss some applications of these solutions to string duality.

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Metadata

Authors
Dabholkar, A., Gauntlett, J. P., Harvey, J. A., & Waldram, D.
Venue
Nuclear Physics B
Publisher
Elsevier BV
Published
1996-08
Volume
474
Issue
1
Pages
85-121
ISSN
0550-3213 (ISSN-L)
OpenAlex
W2083402873
Cited by
176
References
2
FWCI
8.63
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Strings as solitons & black holes as strings. https://app.cochat.ai/papers/10.1016/0550-3213(96)00266-0
The paper
Dabholkar, A., Gauntlett, J. P., Harvey, J. A., & Waldram, D. (1996). Strings as solitons & black holes as strings. Nuclear Physics B. https://doi.org/10.1016/0550-3213(96)00266-0

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

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