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Relativistic Quantum Information: developments in Quantum Information in general relativistic scenarios

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arxiv 1106.0280 v1 pith:SNEYJM4K submitted 2011-06-01 quant-ph gr-qc

Relativistic Quantum Information: developments in Quantum Information in general relativistic scenarios

classification quant-ph gr-qc
keywords quantuminformationeffectsentanglementgravityrelativisticspacetimeaccelerated
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Recently, there has been increased interest in understanding entanglement and quantum communication in black hole spacetimes and in using quantum information techniques to address questions in gravity. Studies on relativistic entanglement show the emergence of conceptually important qualitative differences to a non-relativistic treatment. For instance, entanglement was found to be an observer-dependent property that changes from the perspective of accelerated observers moving in flat spacetime. Relativisitic quantum information theory uses well-known tools coming from quantum information and quantum optics to study quantum effects provoked by gravity to learn information about the spacetime. We can take advantage of our knowledge about quantum correlations and effects produced by the gravitational interaction to set the basis for experimental proposals ultimately aiming at finding corrections due to quantum gravity effects, too mild to be directly observed. This doctoral thesis dissertation summarises most of the research carried out during my PhD on this topic.

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Cited by 2 Pith papers

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  1. Entangled quantum clocks as operational probes of spacetime curvature

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    A CHSH protocol using binarized Peres-time observables, calibrated to S=2 for any state in flat space, yields S>2 for a fixed Bell state in constant-curvature 1+1D backgrounds.

  2. Nonlocal correlations for bosonic fields in black hole quantum atmosphere

    quant-ph 2026-04 unverdicted novelty 5.0

    Bosonic nonlocal correlations degrade at finite radial distances from the event horizon and vanish at larger distances when the quantum atmosphere is accounted for, showing stronger response than in fermionic cases.