Thermodynamics of the Einstein-Euler-Heisenberg rotating black hole

verfasst von

Daniel Amaro, Nora Breton, Claus Lämmerzahl, Alfredo Macías

Abstract

We study the thermodynamic properties of a rotating electrically charged Einstein-Euler-Heisenberg black hole solution. This describes a QED generalization of the Kerr-Newman solution, which endows the vacuum with an effective dielectric constant. The QED-induced modifications to the thermodynamic quantities are presented and discussed. The Penrose process and the extraction of energy from the black hole at the event horizon are reviewed. We also analyze the Euler-Heisenberg nonlinear effects in the cases of supermassive, stellar, and primordial black holes. The evaporation of the black hole is analyzed as blackbody radiation.

Externe Organisation(en)

Universität Bremen
Universidad Autonoma Metropolitana (UAM)
Center for Research and Advanced Studies of the National Polytechnic Institute
Zentrum für angewandte Raumfahrt­technologie und Mikro­gravitation (ZARM)

Typ

Artikel

Journal

Physical Review D

Band

110

ISSN

2470-0010

Publikationsdatum

15.12.2024

Publikationsstatus

Veröffentlicht

Peer-reviewed

Ja

ASJC Scopus Sachgebiete

Kern- und Hochenergiephysik

Elektronische Version(en)

https://doi.org/10.1103/PhysRevD.110.124020 (Zugang: Unbekannt)