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Black Hole Attractors and Pure Spinors

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Paper breakdownThe authors' claims, conditions and measurements, as JSON Signed receiptProof this review has not been altered
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Jonathan P. Hsu, Alexander Maloney, Alessandro Tomasiello

High Energy Physics - Theory · Submitted 15 Feb 2006

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim We construct black hole attractor solutions for a wide class of N=2 compactifications.

how it is stated · asserted 1.00 read the record →

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arXiv IDhep-th/0602142 (version 1)
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CitationAlessandro Tomasiello, Alexander Maloney, Jonathan P. Hsu. "Black Hole Attractors and Pure Spinors." arXiv:hep-th/0602142 (2006). https://pith.science/paper/CPCORPHG
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The compiled record

The paper's own sentences, arranged. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.

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Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 4,835 input tokens, $0.0002 reported.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.10 · human participants 0.01 · controlled comparison 0.04 · randomized assignment 0.01 · states quantitative result 0.11 · compares with prior results 0.73 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v1. Results and the main claim are underlined; .

We construct black hole attractor solutions for a wide class of N=2 compactifications. The analysis is carried out in ten dimensions and makes crucial use of pure spinor techniques. This formalism can accommodate non-Kaehler manifolds as well as compactifications with flux, in addition to the usual Calabi-Yau case. At the attractor point, the charges fix the moduli according to sum_k f_k = Im(C Phi), where Phi is a pure spinor of odd (even) chirality in IIB (A). For IIB on a Calabi-Yau, Phi=Omega and the equation reduces to the usual one. Methods in generalized complex geometry can be used to study solutions to the attractor equation.

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 construct black hole attractor solutions for a wide class of N=2 compactifications. contribution 1.00 0.95 0.29 asserted 1.00
s1 The analysis is carried out in ten dimensions and makes crucial use of pure spinor techniques. method 0.98 0.88 0.06 asserted 1.00
s2 This formalism can accommodate non-Kaehler manifolds as well as compactifications with flux, in addition to the usual Calabi-Yau case. contribution 0.73 0.48 0.10 asserted 0.53
s3 At the attractor point, the charges fix the moduli according to sum_k f_k = Im(C Phi), where Phi is a pure spinor of odd (even) chirality in IIB (A). result 0.99 0.83 0.47 asserted 1.00
s4 For IIB on a Calabi-Yau, Phi=Omega and the equation reduces to the usual one. result 0.53 0.63 0.07 asserted 1.00
s5 Methods in generalized complex geometry can be used to study solutions to the attractor equation. method 0.68 0.18 0.07 hedged possibility 0.84

What kind of paper the classifier reports this is: theoretical result 0.92 · evidence from proof or derivation 1.00.

What was examined, and what was not

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not examined
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  • figures and tables
  • references and citing sentences
  • relations to other papers
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  • P abstract
not run
  • S sections
  • T body sentences
  • C citations
  • R cross-paper relations

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 construct black hole attractor solutions for a wide class of N=2 compactifications. The analysis is carried out in ten dimensions and makes crucial use of pure spinor techniques. This formalism can accommodate non-Kaehler manifolds as well as compactifications with flux, in addition to the usual Calabi-Yau case. At the attractor point, the charges fix the moduli according to sum_k f_k = Im(C Phi), where Phi is a pure spinor of odd (even) chirality in IIB (A). For IIB on a Calabi-Yau, Phi=Omega and the equation reduces to the usual one. Methods in generalized complex geometry can be used to study solutions to the attractor equation.

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References
How the literature uses it

5 arXiv papers cite this in 6 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

Papers citing it · 3 sentences without a confident label

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