Self-dual black holes in celestial holography

Author:

Crawley ErinORCID,Guevara Alfredo,Himwich Elizabeth,Strominger Andrew

Abstract

Abstract We construct two-dimensional quantum states associated to four-dimensional linearized rotating self-dual black holes in (2, 2) signature Klein space. The states are comprised of global conformal primaries circulating on the celestial torus, the Kleinian analog of the celestial sphere. By introducing a generalized tower of Goldstone operators we identify the states as coherent exponentiations carrying an infinite tower of w1+ charges or soft hair. We relate our results to recent approaches to black hole scattering, including a connection to Wilson lines, $$ \mathcal{S} $$ S -matrix results, and celestial holography in curved backgrounds.

Publisher

Springer Science and Business Media LLC

Subject

Nuclear and High Energy Physics

Cited by 6 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Phase diagrams of quasinormal frequencies for Schwarzschild, Kerr, and Taub-NUT black holes;Physical Review D;2024-08-23

2. w1+∞ in 4D gravitational scattering;Journal of High Energy Physics;2024-07-22

3. Celestial holography: An asymptotic symmetry perspective;Physics Reports;2024-06

4. The ambient space formalism;Journal of High Energy Physics;2024-05-27

5. Kleinian black holes;Physical Review D;2024-02-05

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