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Near-extremal black hole entropy and fluctuating 3-branes
High Energy Physics - Theory · Submitted 13 Jul 1996
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim We further suggest that the entropy of configurations reducing to 1-charge D=4 black holes is due to 3-branes moving within 5-branes.
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The abstract, sentence by sentence
We discuss the known microscopic interpretations of the Bekenstein-Hawking entropy for configurations of intersecting M-branes. In some cases the entropy scales as that of a massless field theory on the intersection. A different situation, found for configurations which reduce to 1-charge D=5 black holes or 2-charge D=4 black holes, is explained by a gas of non-critical strings at their Hagedorn temperature. We further suggest that the entropy of configurations reducing to 1-charge D=4 black holes is due to 3-branes moving within 5-branes.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We discuss the known microscopic interpretations of the Bekenstein-Hawking entropy for configurations of intersecting M-branes. | background 0.93 | 0.17 | 0.05 | asserted 0.70 |
| s1 | In some cases the entropy scales as that of a massless field theory on the intersection. | background 0.80 | 0.12 | 0.06 | asserted 0.75 |
| s2 | A different situation, found for configurations which reduce to 1-charge D=5 black holes or 2-charge D=4 black holes, is explained by a gas of non-critical strings at their Hagedorn temperature. | interpretation 0.58 | 0.21 | 0.11 | asserted 1.00 |
| s3 | We further suggest that the entropy of configurations reducing to 1-charge D=4 black holes is due to 3-branes moving within 5-branes. | interpretation 0.75 | 0.68 | 0.52 | hedged possibility 0.93 |
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Original abstract
We discuss the known microscopic interpretations of the Bekenstein-Hawking entropy for configurations of intersecting M-branes. In some cases the entropy scales as that of a massless field theory on the intersection. A different situation, found for configurations which reduce to 1-charge D=5 black holes or 2-charge D=4 black holes, is explained by a gas of non-critical strings at their Hagedorn temperature. We further suggest that the entropy of configurations reducing to 1-charge D=4 black holes is due to 3-branes moving within 5-branes.
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