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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.

how it is stated · hedged possibility 0.93 read the record →

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arXiv IDhep-th/9607107 (version 2)
Pith ID7FUZ4XZ5, Pith's permanent record of this paper and its review
CitationA.A. Tseytlin, I.R. Klebanov. "Near-extremal black hole entropy and fluctuating 3-branes." arXiv:hep-th/9607107 (1996). https://pith.science/paper/7FUZ4XZ5
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What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.10 · human participants 0.01 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.06 · compares with prior results 0.60 · mentions code or data availability 0.01.

The abstract, sentence by sentence

arXiv listing abstract v2. Results and the main claim are underlined; .

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

What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
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

What kind of paper the classifier reports this is: position or commentary 0.54 · evidence from argument 0.73.

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Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper
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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2 arXiv papers cite this in 2 sentences

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

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