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Black diholes

High Energy Physics - Theory · Submitted 21 Jun 1999

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

The authors' main claim We present and analyze exact solutions of the Einstein-Maxwell and Einstein-Maxwell-Dilaton equations that describe static pairs of oppositely charged extremal black holes, i.e., black diholes.

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arXiv IDhep-th/9906160 (version 3)
Pith IDUWGVYBAX, Pith's permanent record of this paper and its review
CitationRoberto Emparan. "Black diholes." arXiv:hep-th/9906160 (1999). https://pith.science/paper/UWGVYBAX
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What the abstract itself states, as probabilities: claims first 0.04 · states limitation 0.08 · human participants 0.01 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.04 · compares with prior results 0.22 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v3. Results and the main claim are underlined; .

We present and analyze exact solutions of the Einstein-Maxwell and Einstein-Maxwell-Dilaton equations that describe static pairs of oppositely charged extremal black holes, i.e., black diholes. The holes are suspended in equilibrium in an external magnetic field, or held apart by cosmic strings. We comment as well on the relation of these solutions to brane-antibrane configurations in string and M-theory.

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 present and analyze exact solutions of the Einstein-Maxwell and Einstein-Maxwell-Dilaton equations that describe static pairs of oppositely charged extremal black holes, i.e., black diholes. contribution 1.00 0.96 0.50 asserted 1.00
s1 The holes are suspended in equilibrium in an external magnetic field, or held apart by cosmic strings. result 0.85 0.63 0.15 asserted 0.99
s2 We comment as well on the relation of these solutions to brane-antibrane configurations in string and M-theory. interpretation 0.97 0.55 0.07 unclear 0.77

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

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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 present and analyze exact solutions of the Einstein-Maxwell and Einstein-Maxwell-Dilaton equations that describe static pairs of oppositely charged extremal black holes, i.e., black diholes. The holes are suspended in equilibrium in an external magnetic field, or held apart by cosmic strings. We comment as well on the relation of these solutions to brane-antibrane configurations in string and M-theory.

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References
How the literature uses it

12 arXiv papers cite this in 13 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 · 9 sentences without a confident label

Compares with it 2 papers
  • It would, indeed be quite interesting to study in detail the horizon (and ergosphere) geometry of these solutions.[The fact that the extremality limit has $|J|>M^2$ has a counterpart for the charged dihole [ref] wherein the extremal limit has $|Q|>M$.

    On the interaction between two Kerr black holes · Physical interpretation · 0.93

  • Our construction is also distinct from the “black dihole” [ref] implementations of Kerr, which are simply just real metrics and involve no self-duality relation between mass and NUT charge.

    Newman-Janis Algorithm from Taub-NUT Instantons · Introduction · 0.96

Cites it as background 2 papers
  • Physical properties of a pair of identical black holes with opposite charges (black diholes) have been studied in detail by Emparan and Teo [ref] , where they managed to find out a compact expression for the horizon area and the surface gravity of the components.

    Thermodynamics of two black holes · Introduction · 0.84

  • Emparan �tudia notamment un "dipole" constitu� de deux trous noirs extr�maux mais de charges oppos�es dans la th�orie d'Einstein-Maxwell avec et sans la pr�sence d'un dilaton [ref] .

    Black hole solutions of modified gravity theories · La structure de barre de la solution de Schwarzschild et les multi-trous noirs · 0.93

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