Rotating structure of the Euler-Heisenberg black hole

authored by: Nora Bretón, Claus Lämmerzahl, Alfredo Macías
Abstract: In this work, we deal with the QED interpretation of the Euler-Heisenberg nonlinear electrodynamics as the effective theory after a one-loop of nonperturbative quantization. It endows the vacuum with an effective dielectric constant, the polarizability and magnetizability of which are determined by clouds of virtual charges surrounding the real currents and charges. Therefore, we study the Euler-Heisenberg nonlinear electrodynamics as a screened Maxwell theory. We generate a rotating electrically charged Einstein-Euler-Heisenberg black hole solution and interpret it as a Kerr-Newman-like one with screened electric charge, as it happens for the static electrically charged black hole Einstein-Euler-Heisenberg solution, which is considered as a Reissner-Nordström-like solution with screened electric charge.
External Organisation(s): Center for Research and Advanced Studies of the National Polytechnic Institute
Universidad Autonoma Metropolitana (UAM)
Center of Applied Space Technology and Microgravity (ZARM)
Type: Article
Journal: Physical Review D
Volume: 105
ISSN: 2470-0010
Publication date: 24.05.2022
Publication status: Published
Peer reviewed: Yes
ASJC Scopus subject areas: Physics and Astronomy (miscellaneous)
Electronic version(s): https://doi.org/10.1103/physrevd.105.104046 (Access: Closed)

BibTeX

@article{8180c0670f544b06806c9d7ab5b35f86,
title = "Rotating structure of the Euler-Heisenberg black hole",
abstract = "In this work, we deal with the QED interpretation of the Euler-Heisenberg nonlinear electrodynamics as the effective theory after a one-loop of nonperturbative quantization. It endows the vacuum with an effective dielectric constant, the polarizability and magnetizability of which are determined by clouds of virtual charges surrounding the real currents and charges. Therefore, we study the Euler-Heisenberg nonlinear electrodynamics as a screened Maxwell theory. We generate a rotating electrically charged Einstein-Euler-Heisenberg black hole solution and interpret it as a Kerr-Newman-like one with screened electric charge, as it happens for the static electrically charged black hole Einstein-Euler-Heisenberg solution, which is considered as a Reissner-Nordstr{\"o}m-like solution with screened electric charge. ",
author = "Nora Bret{\'o}n and Claus L{\"a}mmerzahl and Alfredo Mac{\'i}as",
note = "Funding Information: We thank the unknown Referee for his/her positive and constructive report. This work was partially supported by DAAD fellowships: A. M. (Ref. No. 91699151) and N. B. (Ref. No. 91834104). N. B. also acknowledges partial support by CONACyT (Mexico) Grant No. 284489. C. L. is supported by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) under Germany{\textquoteright}s Excellence Strategy-EXC-2123 “QuantumFrontiers”-Grant No. 390837967, the CRC 1464 “Relativistic and Quantum-based Geodesy” (TerraQ), and by the Research Training Group GRK1620 “Models of Gravity.” ",
year = "2022",
month = may,
day = "24",
doi = "10.1103/physrevd.105.104046",
language = "English",
volume = "105",
journal = "Physical Review D",
issn = "2470-0010",
publisher = "American Institute of Physics",
number = "10",
}