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This research investigates reflected entropy and Markov gaps in bosonic fields across non-inertial frames, revealing distinct divergence behaviors compared to fermionic systems when applied to black hole spacetimes. The study provides closed-form solutions for specific quantum states that clarify how classical correlations persist even as entanglement vanishes asymptotically near horizons. These findings advance the theoretical understanding of quantum information dynamics in curved spacetime and holographic contexts.
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Surviving correlations across a horizon: reflected entropy for bosonic fields in non-inertial frames and black hole spacetimes

arXiv2 min read

arXiv:2608.05473v1 Announce Type: cross Abstract: We study the reflected entropy and the Markov gap for modes of a free bosonic field shared by inertial observers (Alice, Charlie) and a uniformly accelerated one (Bob), for a bipartite Bell state and the tripartite Werner (W) and Greenberger--Horne--Zeilinger (GHZ) states. The bosonic Bogoliubov transformation spans an infinite-dimensional Fock space with an unbounded squeezing parameter unlike the fermionic case. By identifying a conserved charge, we block-diagonalize the reduced density matrices into exact two-dimensional sectors, yielding closed or semi-analytic forms for all three states. Although bosonic entanglement is known to vanish asymptotically, the Alice--Bob reflected entropy instead saturates at a nonzero saturation floor, retaining the surviving classical correlation, and converges to the value Alice shares with Bob's causally disconnected partner. Crucially, only the inter-wedge reflected entropy diverges, linearly in the squeezing parameter---the sharp distinction from the fermionic case, where it stays bounded---while the Markov gaps saturate. The construction transfers verbatim to a Schwarzschild black hole, where the saturation values become mass-independent constants.

arXiv:2608.05473 (hep-th)

Abstract:We study the reflected entropy and the Markov gap for modes of a free bosonic field shared by inertial observers (Alice, Charlie) and a uniformly accelerated one (Bob), for a bipartite Bell state and the tripartite Werner (W) and Greenberger--Horne--Zeilinger (GHZ) states. The bosonic Bogoliubov transformation spans an infinite-dimensional Fock space with an unbounded squeezing parameter unlike the fermionic case. By identifying a conserved charge, we block-diagonalize the reduced density matrices into exact two-dimensional sectors, yielding closed or semi-analytic forms for all three states. Although bosonic entanglement is known to vanish asymptotically, the Alice--Bob reflected entropy instead saturates at a nonzero saturation floor, retaining the surviving classical correlation, and converges to the value Alice shares with Bob's causally disconnected partner. Crucially, only the inter-wedge reflected entropy diverges, linearly in the squeezing parameter---the sharp distinction from the fermionic case, where it stays bounded---while the Markov gaps saturate. The construction transfers verbatim to a Schwarzschild black hole, where the saturation values become mass-independent constants.

arXiv:2608.05473 [hep-th]

(or arXiv:2608.05473v1 [hep-th] for this version)

https://doi.org/10.48550/arXiv.2608.05473 arXiv-issued DOI via DataCite (pending registration)

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Full text under the publisher's open licence · 251 words

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