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Black holes with halos

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Ruben Monten, Chiara Toldo

High Energy Physics - Theory · Submitted 7 Dec 2016

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

The authors' main claim These configurations have nonzero temperature and are moreover surrounded by a massive vector field halo.

how it is stated · asserted 1.00 read the record →

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arXiv ID1612.02399 (version 2)
Pith IDV6M3I4DN, Pith's permanent record of this paper and its review
CitationChiara Toldo, Ruben Monten. "Black holes with halos." arXiv:1612.02399 (2016). https://pith.science/paper/V6M3I4DN
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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-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-23: 1 request, 4,310 input tokens.

What the abstract itself states, as probabilities: claims first 0.05 · states limitation 0.13 · human participants 0.01 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.07 · compares with prior results 0.06 · mentions code or data availability 0.02.

The abstract, sentence by sentence

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

We present new AdS4 black hole solutions in N = 2 gauged supergravity coupled to vector and hypermultiplets. We focus on a particular consistent truncation of M-theory on the homogeneous Sasaki-Einstein seven-manifold M111, characterized by the presence of one Betti vector multiplet. We numerically construct static and spherically symmetric black holes with electric and magnetic charges, corresponding to M2 and M5 branes wrapping non-contractible cycles of the internal manifold. These configurations have nonzero temperature and are moreover surrounded by a massive vector field halo. For these solutions we verify the first law of black hole mechanics and we analyze the thermodynamics and phase transitions in the canonical ensemble, interpreting the process in the corresponding dual field 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 new AdS4 black hole solutions in N = 2 gauged supergravity coupled to vector and hypermultiplets. contribution 1.00 0.95 0.12 asserted 1.00
s1 We focus on a particular consistent truncation of M-theory on the homogeneous Sasaki-Einstein seven-manifold M111, characterized by the presence of one Betti vector multiplet. method 0.61 0.50 0.06 asserted 0.97
s2 We numerically construct static and spherically symmetric black holes with electric and magnetic charges, corresponding to M2 and M5 branes wrapping non-contractible cycles of the internal manifold. contribution 0.78 0.94 0.10 asserted 1.00
s3 These configurations have nonzero temperature and are moreover surrounded by a massive vector field halo. result 1.00 0.87 0.29 asserted 1.00
s4 For these solutions we verify the first law of black hole mechanics and we analyze the thermodynamics and phase transitions in the canonical ensemble, interpreting the process in the corresponding dual field theory. contribution 0.78 0.95 0.23 asserted 1.00

What kind of paper the classifier reports this is: theoretical result 0.75 · evidence from simulation or computation 1.00.

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  • references and citing sentences
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  • 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 present new AdS4 black hole solutions in N = 2 gauged supergravity coupled to vector and hypermultiplets. We focus on a particular consistent truncation of M-theory on the homogeneous Sasaki-Einstein seven-manifold M111, characterized by the presence of one Betti vector multiplet. We numerically construct static and spherically symmetric black holes with electric and magnetic charges, corresponding to M2 and M5 branes wrapping non-contractible cycles of the internal manifold. These configurations have nonzero temperature and are moreover surrounded by a massive vector field halo. For these solutions we verify the first law of black hole mechanics and we analyze the thermodynamics and phase transitions in the canonical ensemble, interpreting the process in the corresponding dual field theory.

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References
How the literature uses it

5 arXiv papers cite this in 16 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 · 13 sentences without a confident label

Builds on it 1 paper
  • The truncation on $M^111$ used in [ref] can be obtained from the reduction on $Q^111$ upon setting to zero one of the two Betti multiplets, by suitably identifying two gauge fields $A^3=A^1$ and two scalar fields $t^3=t^1$.

    On the Search for Multicenter AdS Black Holes from M-theory · Four-dimensional Supergravity setup and uplift in 11d · 0.84

Uses its method or tool 1 paper
Cites it as background 1 paper

What it cites · 63 sentences without a confident label

Builds on 1 paper
  • The black holes we present here correspond to nonzero temperature generalizations of the black holes of [ref] and are found by solving the Einstein, Maxwell and scalar equations of motion.

    BPS Black Holes in AdS4 from M-theory · Introduction · 0.97

Uses the method or tool of 6 papers
  • Therefore, it is sufficient to take into account [equation] Finally, following the prescription of [ref] , the presence of the massive vector field requires the presence of an additional counterterm of the form [equation] However, in our subspace of solutions this counterterm does not give any finite contribution to the renormalized action, as one can see from the asymptotic expansion of $ζ$ in [ref].

    Holographic Renormalization and Ward Identities with the Hamilton-Jacobi Method · Renormalized on-shell action · 0.89

  • Therefore, it is sufficient to take into account [equation] Finally, following the prescription of [ref] , the presence of the massive vector field requires the presence of an additional counterterm of the form [equation] However, in our subspace of solutions this counterterm does not give any finite contribution to the renormalized action, as one can see from the asymptotic expansion of $ζ$ in [ref].

    Holographic Renormalization · Renormalized on-shell action · 0.89

  • We now compute the on-shell value of the renormalized action for purely electric black holes, following [ref] .

    Black hole mass and Hamilton-Jacobi counterterms · Electric solution · 0.98

Uses data or values from 1 paper
  • The spectrum then contains (see Table 7 of [ref] ) * the gravity multiplet, containing the metric $g_μν$ and a massless vector, * a Betti vector multiplet, containing the massless vector and a complex scalar (two real fields) of mass $m^2 l^2 = -2$ (in our conventions, the Breitenlohner-Freedman bound is $m^2 l^2 ≥-9/4$), each with $Δ=(2,1)$, * a massive vector multiplet, containing a massive vector of mass $m^2 l^2=12$ (which corresponds holographically to a vector operator with weight $Δ=5$), which has eaten its axion $a$ and five scalars of mass $m^2 l^2=(18,10,10,10,4)$ corresponding to $Δ=(6,5,5,5,4)$.

    All homogeneous N=2 M-theory truncations with supersymmetric AdS4 vacua · Model M111 · 0.95

Compares with 17 papers
Cites as background 32 papers
  • Zero-temperature, 1/4 BPS black hole solutions for various models, including $Q^111$ and $M^111$, were found in [ref] , in the form of flows from $AdS_4$ to $AdS_2 ×S^2$ near-horizon geometries, by solving the BPS equations.

    BPS Black Holes in AdS4 from M-theory · Introduction · 0.86

  • The first example of static supersymmetric AdS$_4$ black holes was analytically constructed in [ref] , while previous studies [ref] yielded naked singularities.

    Anti-de Sitter Black Holes in Gauged N=8 Supergravity · Introduction · 0.88

  • The first example of static supersymmetric AdS$_4$ black holes was analytically constructed in [ref] , while previous studies [ref] yielded naked singularities.

    Supersymmetric AdS_4 black holes and attractors · Introduction · 0.88

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