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Four-dimensional black hole entropy from F-theory
High Energy Physics - Theory · Submitted 15 Aug 2018
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim The induced corrections turn out to contribute at leading order to the central charges and levels, which in turn determine the black hole entropy.
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The abstract, sentence by sentence
We study the central charges and levels of a two-dimensional $N=(0,4)$ superconformal field theory describing four-dimensional BPS black holes in F-theory. These arise from D3-branes wrapping a curve in the base of an elliptically fibered Calabi-Yau threefold times a circle, and probe a transverse Taub-NUT space. The near horizon geometry of these D3-branes is AdS$_3 \times \text{S}^3/\mathbb{Z}_m$, where $m$ is the NUT charge. Starting from a six-dimensional supergravity effective action we compute three-dimensional Chern-Simons terms to deduce the central charges and levels. We find that it is crucial to integrate out an infinite tower of massive Kaluza-Klein states on S$^3/\mathbb{Z}_m$ to match the expected microscopic results. The induced corrections turn out to contribute at leading order to the central charges and levels, which in turn determine the black hole entropy.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We study the central charges and levels of a two-dimensional $N=(0,4)$ superconformal field theory describing four-dimensional BPS black holes in F-theory. | contribution 1.00 | 0.91 | 0.08 | asserted 0.95 |
| s1 | These arise from D3-branes wrapping a curve in the base of an elliptically fibered Calabi-Yau threefold times a circle, and probe a transverse Taub-NUT space. | background 0.50 | 0.21 | 0.03 | asserted 1.00 |
| s2 | The near horizon geometry of these D3-branes is AdS$_3 \times \text{S}^3/\mathbb{Z}_m$, where $m$ is the NUT charge. | background 0.67 | 0.24 | 0.05 | asserted 1.00 |
| s3 | Starting from a six-dimensional supergravity effective action we compute three-dimensional Chern-Simons terms to deduce the central charges and levels. | method 0.99 | 0.95 | 0.06 | asserted 1.00 |
| s4 | We find that it is crucial to integrate out an infinite tower of massive Kaluza-Klein states on S$^3/\mathbb{Z}_m$ to match the expected microscopic results. | result 0.79 | 0.93 | 0.40 | asserted 1.00 |
| s5 | The induced corrections turn out to contribute at leading order to the central charges and levels, which in turn determine the black hole entropy. | result 0.79 | 0.92 | 0.55 | asserted 1.00 |
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The paper
Original abstract
We study the central charges and levels of a two-dimensional $N=(0,4)$ superconformal field theory describing four-dimensional BPS black holes in F-theory. These arise from D3-branes wrapping a curve in the base of an elliptically fibered Calabi-Yau threefold times a circle, and probe a transverse Taub-NUT space. The near horizon geometry of these D3-branes is AdS$_3 \times \text{S}^3/\mathbb{Z}_m$, where $m$ is the NUT charge. Starting from a six-dimensional supergravity effective action we compute three-dimensional Chern-Simons terms to deduce the central charges and levels. We find that it is crucial to integrate out an infinite tower of massive Kaluza-Klein states on S$^3/\mathbb{Z}_m$ to match the expected microscopic results. The induced corrections turn out to contribute at leading order to the central charges and levels, which in turn determine the black hole entropy.
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References
How the literature uses it
11 arXiv papers cite this in 43 sentences
Papers citing it · 30 sentences without a confident label
Contests it 1 paper
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However, it was shown in [ref] that this is not the full story and does not generically reproduce the correct microscopic results.
Black Holes and (0,4) SCFTs from Type IIB on K3 · Macroscopics of 6d strings · contest 0.75
Builds on it 1 paper
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The macroscopic computations for Taub-NUT performed in [ref] straightforwardly extend to the ALE and ALF transverse spaces considered here.
Black Holes and (0,4) SCFTs from Type IIB on K3 · Conclusion and outlook · 0.99
Uses its method or tool 2 papers
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Instead the correct procedure is to reduce the action on the compact part of the asymptotic geometry [ref] .
Anomalies of (0,4) SCFTs from F-theory · Classical contributions · 0.81
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Following [ref] we use zeta-function regularization.
Black Holes and (0,4) SCFTs from Type IIB on K3 · Contribution of massive KK modes to one-loop Chern–Simons terms · 1.00
Compares with it 2 papers
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We expect that the left level can be computed by adapting the techniques in [ref] .
Black Holes and (0,4) SCFTs from Type IIB on K3 · Transverse ALF spaces: AD-series · 0.95
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We can see that if we specify the ALF result to Taub-NUT we recover the classical results of [ref] as expected.
Anomalies of (0,4) SCFTs from F-theory · Total classical contributions · 0.97
Cites it as support 1 paper
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In [ref] for similar settings, this assumption was shown to lead to results which agree with the microscopic predictions.
Anomalies of (0,4) SCFTs from F-theory · Quantum contributions to levels · 0.96
Cites it as background 2 papers
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More recently black holes in F-theory [ref] have been given further consideration in [ref] for example.
Black Holes and (0,4) SCFTs from Type IIB on K3 · Introduction · 0.96
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In a tangential direction, there have been further advancements in studying black strings in F-theory probing various four-dimensional asymptotically flat spaces [ref] using their AdS$_3$ near-horizon geometries.
On Type IIA AdS$_3$ solutions and massive GK geometries · Introduction · 0.98
What it cites · 20 sentences without a confident label
Builds on 3 papers
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In [ref] the authors extended the study of [ref] to the case of five-dimensional spinning black holes that previously only had been studied in compactifications of type II strings on T$^5$ and K$3 ×S^1$ [ref] .
F-Theory, Spinning Black Holes and Multi-string Branches · Introduction · 0.97
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In [ref] the authors extended the study of [ref] to the case of five-dimensional spinning black holes that previously only had been studied in compactifications of type II strings on T$^5$ and K$3 ×S^1$ [ref] .
D--branes and Spinning Black Holes · Introduction · 0.97
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In [ref] the authors extended the study of [ref] to the case of five-dimensional spinning black holes that previously only had been studied in compactifications of type II strings on T$^5$ and K$3 ×S^1$ [ref] .
Black Holes and Calabi-Yau Threefolds · Introduction · 0.97
Uses the method or tool of 1 paper
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The microscopic analysis was carried out by mapping the F-theory setup to the MSW setting [ref] .
Black Hole Entropy in M-Theory · Introduction · 0.84
Compares with 4 papers
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From a six-dimensional supergravity perspective we reproduced the central charges and levels of the CFT corresponding to the long wavelength limit of this set-up, which were calculated from a microscopic viewpoint via M-theory in [ref] .
Black String Entropy and Fourier-Mukai Transform · Discussion · 0.88
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[equation] Comparing conventions in [ref] and [ref] we find that we need $A^0→qiA^0$ in the counterterm above.
One-loop Chern-Simons terms in five dimensions · 6D to 5D one-loop corrections · 0.96
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On the CFT side the main difference between [ref] and [ref] is the identification of an $𝔰𝔲(2)_L$ current algebra in spite of the absence of supersymmetry in the left-moving sector.
F-Theory, Spinning Black Holes and Multi-string Branches · Introduction · 0.99
Cites as background 13 papers
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In particular, we use the regularized sums [equation] It is worth noting that regularizing the contributions arising from integrating out infinitely many massive modes is in general very subtle.[See [ref] for a recent detailed discussion.] Firstly, applying zeta-function regularization is only possible if the higher-dimensional theory is anomaly free [ref] .
Infinite Distances in Field Space and Massless Towers of States · One-loop Chern-Simons terms from KK spectrum · 0.83
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In particular, we use the regularized sums [equation] It is worth noting that regularizing the contributions arising from integrating out infinitely many massive modes is in general very subtle.[See [ref] for a recent detailed discussion.] Firstly, applying zeta-function regularization is only possible if the higher-dimensional theory is anomaly free [ref] .
Chiral anomalies on a circle and their cancellation in F-theory · One-loop Chern-Simons terms from KK spectrum · 0.83
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This is the four-dimensional side of the correspondence in [ref] .
Exploring the relation between 4D and 5D BPS solutions · Introduction · 0.90
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