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Physics Letters B

Quantum entanglement in the Dirac field quantization around charged black holes

Abdessamie Chhieb, Chaimae Banouni, Saliha Abdessamie, M. Ouchrif

Published Jun 12, 2026• 0 citations
Publisher

Abstract

We investigate the quantum entanglement properties of the Dirac field near a charged Reissner–Nordström black hole, incorporating the effects of Hawking radiation within the framework of quantum field theory in curved spacetime. Using concurrence C and Bures distance B as measures of entanglement, we analyze how quantum correlations evolve with respect to the electric charge Q of the black hole, the frequency ω of fermionic modes, and the initial entanglement angle θ . Our results show that the electric charge Q enhances decoherence inside the event horizon while, counterintuitively, temporarily increasing accessible entanglement outside. The Hawking effect induces an apparent loss of entanglement for an external observer, due to correlation transfer to inaccessible regions. High-frequency modes ω exhibit greater resilience to gravitational effects, maintaining robust correlations near the horizon. These findings highlight the redistribution of entanglement in a multipartite system in curved spacetime, with significant implications for quantum information in relativistic and gravitational contexts.

DOI
10.1016/j.physletb.2026.140629

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We investigate the quantum entanglement properties of the Dirac field near a charged Reissner–Nordström black hole, incorporating the effects of Hawking radiation within the framework of quantum field theory in curved spacetime. Using concurrence C and Bures distance B as measures of entanglement, we analyze how quantum correlations evolve with respect to the electric charge Q of the black hole, the frequency ω of fermionic modes, and the initial entanglement angle θ . Our results show that the electric charge Q enhances decoherence inside the event horizon while, counterintuitively, temporarily increasing accessible entanglement outside. The Hawking effect induces an apparent loss of entanglement for an external observer, due to correlation transfer to inaccessible regions. High-frequency modes ω exhibit greater resilience to gravitational effects, maintaining robust correlations near the horizon. These findings highlight the redistribution of entanglement in a multipartite system in curved spacetime, with significant implications for quantum information in relativistic and gravitational contexts.
We investigate the quantum entanglement properties of the Dirac field near a charged Reissner--Nordström black hole, incorporating the effects of Hawking radiation within the framework of quantum field theory in curved spacetime. Using concurrence C C C and Bures distance B B B as measures of entanglement, we analyze how quantum correlations evolve with respect to the electric charge Q Q Q of the black hole, the frequency ω ωω of fermionic modes, and the initial entanglement angle θ θθ. Our results show that the electric charge Q Q Q enhances decoherence inside the event horizon while, counterintuitively, temporarily increasing accessible entanglement outside. The Hawking effect induces an apparent loss of entanglement for an external observer, due to correlation transfer to inaccessible regions. High-frequency modes ω ωω exhibit greater resilience to gravitational effects, maintaining robust correlations near the horizon. These findings highlight the redistribution of entanglement in a multipartite system in curved spacetime, with significant implications for quantum information in relativistic and gravitational contexts.
ABSTRACT We investigate the influence of the Hawking effect on quantum entanglement by incorporating the spin degrees of freedom of Dirac fields in the background of a Garfinkle–Horowitz–Strominger (GHS) dilaton black hole. By analyzing the redistribution of correlations between causally accessible and inaccessible regions, we obtain analytical results showing that, as the dilaton increases, the physically accessible spin entanglement decreases monotonically while the inaccessible counterpart grows correspondingly, revealing a constrained transfer of quantum correlations across the event horizon rather than independent creation or destruction. From an information‐theoretic perspective, we demonstrate that the Hawking effect does not permit arbitrary redistribution of spin entanglement, but instead enforces a well‐defined monogamy relation that strictly governs how entanglement is shared among different bipartitions under gravitational evolution. These results indicate that the correlations initially shared by the observers are redistributed between accessible and inaccessible sectors through the Hawking‐induced Bogoliubov transformation, providing further insight into the structure of spin quantum correlations in curved spacetime and the role of horizon‐induced effects in reshaping quantum correlations. PACS numbers: 04.70.Dy, 03.65.Ud,04.62.+v
We investigate bipartite quantum correlations of Dirac fields in the spacetime of a Hayward regular black hole. Using the Wootters concurrence and the CHSH Bell parameter, we analyze the influence of Hawking radiation on an entangled state shared by an inertial observer and a near-horizon observer. We show that, unlike the bosonic case, fermionic correlations remain nonzero even in the infinite-temperature limit owing to the Pauli exclusion principle, while part of the entanglement is redistributed to inaccessible modes inside the horizon. The accessible modes exhibit Bell nonlocality for all finite Hawking temperatures, whereas the interior modes never violate Bell's inequality. The Hayward regularity parameter ggg affects the correlations only through the Hawking temperature, whose decrease with increasing ggg enhances the preservation of quantum information. These results suggest a close connection between singularity resolution and the robustness of fermionic quantum correlations in regular black-hole spacetimes.
Abstract The black hole information paradox arises from the tension between the thermal spectral properties of Hawking radiation and the unitarity principle in quantum mechanics. To explore the dynamical evolution characteristics of quantum fields in this context, we employ the standard quantization formalism for Dirac fields in Schwarzschild spacetime and investigate the coupling structure of particle and antiparticle modes within a framework that transcends the single-mode approximation. By calculating the states of externally observable subsystems, we systematically derive the evolution of concurrence and first-order coherence as functions of the Hawking temperature. Additionally, we assess the impact of varying initial parameters on these quantities. We further contrast the quantum entanglement differences between the observable exterior region and the black hole interior across diverse temperature regimes. These results provide valuable insights into the evolution of entanglement and coherence in curved spacetime.
Abstract We investigate how the Hawking effect reshapes distinct quantum resources of Dirac fields in Schwarzschild spacetime beyond the single-mode approximation. By quantifying quantum entanglement and coherence using the negativity, the l 1 -norm of coherence and the relative entropy of coherence, we observe a significant asymmetry in their response to gravitational effects. While the Hawking effect monotonically degrades entanglement and drives it toward a finite residual value, quantum coherence is instead monotonically amplified with increasing Hawking temperature, revealing the black hole as an effective decohering environment for nonlocal correlations but a coherence-enhancing mechanism for local superposition. Notably, we further find that under the influence of the Hawking effect, the maximally entangled state does not necessarily correspond to the largest initial negativity. In fact, its value may even be smaller than that of certain non-maximally entangled states. Our results demonstrate that gravity acts in a highly nonuniform manner on different facets of quantumness and highlight the necessity of resource-adapted state engineering for relativistic quantum information processing near the event horizon of the black hole.
Quantum information science has been broadly explored in Einstein gravity and in various modified gravity theories; however, its extension to quantum gravity settings remains largely unexplored. Motivated by this gap, in this paper we investigate the degradation of quantum entanglement of scalar and Dirac fields in the third-type black hole geometry arising from effective quantum gravity, which incorporates generic quantum gravitational corrections beyond classical general relativity. This quantum corrected spacetime is free of a Cauchy horizon and can be cast into a Rindler form in the near-horizon regime, allowing a direct identification of vacuum modes and a clear correspondence with the framework developed for uniformly accelerated observers. Within this framework, we compute the quantum entanglement and mutual information of uniformly entangled detector pairs in terms of the quantum parameter ζ~\tildeζζ~​, the mode frequency ω~\tildeωω~, and Bob's radial position R0R_0R0​. The quantum parameter ζ~\tildeζζ~​ consistently weakens the horizon-induced loss of correlations. For scalar fields this effect is pronounced, producing clear departures from the classical behavior, whereas for Dirac fields the familiar correlation pattern remains intact but its degradation is noticeably reduced. Overall, ζ~\tildeζζ~​ acts as a universal protective factor against gravitational suppression of quantum correlations. The third-type effective quantum black hole therefore provides a controlled and physically transparent arena for probing how quantum-gravity corrections influence relativistic quantum information.