Investigating QED effects on the thin accretion disk properties around rotating Euler–Heisenberg black holes

Abstract The Einstein–Euler–Heisenberg (EEH) black hole model represents an extension of classical black hole solutions in general relativity by incorporating quantum electrodynamic (QED) corrections. These corrections are introduced through the inclusion of the Euler–Heisenberg Lagrangian, which ac...

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Bibliographic Details
Main Authors: Kourosh Nozari, Sara Saghafi, Fatemeh Aliyan
Format: Article
Language:English
Published: SpringerOpen 2025-07-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-025-14433-1
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