2019
DOI: 10.1007/jhep01(2019)037
|View full text |Cite
|
Sign up to set email alerts
|

Four-dimensional black hole entropy from F-theory

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 × S 3 /Z m , where m is the NUT charge. Starting from a sixdimensional supergravity effective action we compute three-dimensional Chern-Simons te… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1

Citation Types

4
49
1

Year Published

2019
2019
2024
2024

Publication Types

Select...
7

Relationship

3
4

Authors

Journals

citations
Cited by 16 publications
(54 citation statements)
references
References 62 publications
4
49
1
Order By: Relevance
“…We will see that it will also shed light on why Kaluza‐Klein modes happen to also satisfy the distance conjecture. This analysis is mostly based on unpublished work [], and we refer also to [] for relevant work on this topic.…”
Section: The Emergence Proposalmentioning
confidence: 99%
“…We will see that it will also shed light on why Kaluza‐Klein modes happen to also satisfy the distance conjecture. This analysis is mostly based on unpublished work [], and we refer also to [] for relevant work on this topic.…”
Section: The Emergence Proposalmentioning
confidence: 99%
“…, (4.2) where we denote the scalars collectively as φ i , with a ij some functions of the scalars 8 and F 2 (a) = F (a) µν F µν (a) . We are interested in finding solutions to the equations of motion derived from (4.2) describing the near-horizon region of an extremal black hole.…”
Section: Compactification Of the Supergravity Theorymentioning
confidence: 99%
“…In order to make the comparison with previous literature transparent, the dimensional reduction of this section uses a different parametrization of the scalars than that of section 3.2 8. In the family of near-horizon solutions that we consider the scalars are constant, so the σ-model will play no role.…”
mentioning
confidence: 99%
“…This was later extended to five-dimensional non-spinning black holes in M-theory on a Calabi-Yau threefold [2] and four-dimensional black holes in Mtheory on the product of a Calabi-Yau threefold with a circle by MSW [3]. More recently black holes in F-theory [4] have been given further consideration in [5][6][7] for example.In this paper we are interested in compactifications of type IIB string theory on K3 and the black strings emerging in this theory. The goal is to match macroscopic data with a complimentary microscopic description.…”
mentioning
confidence: 99%
“…In this paper we compute the central charges and levels corresponding to the settings described above both from a macroscopic and microscopic viewpoint.Macroscopically we shall work exclusively in six-dimensional N = (2, 0) supergravity [9,10] which is obtained by compactifying type IIB on K3 [11]. The techniques for computing the various central charges and current algebra levels corresponding to the black string solutions of this theory were developed in [5,7,[12][13][14][15]. Concretely, we reduce the classical six-dimensional action to three dimensions in the black string background.…”
mentioning
confidence: 99%