The fate of non-trivial entanglement under gravitational collapse
arXiv:1205.1263 · doi:10.1088/0264-9381/29/22/224006
Abstract
We analyse the evolution of the entanglement of a non-trivial initial quantum field state (which, for simplicity, has been taken to be a bipartite state made out of vacuum and the first excited state) when it undergoes a gravitational collapse. We carry out this analysis by generalising the tools developed to study entanglement behaviour in stationary scenarios and making them suitable to deal with dynamical spacetimes. We also discuss what kind of problems can be tackled using the formalism spelled out here as well as single out future avenues of research.
9 pages, 2 figures. v2: Added Journal reference and small changes to match published version
References in corpus (10)
- Entanglement of Dirac fields in non-inertial frames
- Non-local density correlations as signal of Hawking radiation in BEC acoustic black holes
- Entanglement in an expanding spacetime
- Continuous variable entanglement sharing in non-inertial frames
- Biaxially symmetric solutions to 4D higher-spin gravity
- Voyage to Alpha Centauri: Entanglement degradation of cavity modes due to motion
- Fermionic entanglement that survives a black hole
- Motion generates entanglement
- Residual entanglement of accelerated fermions is not nonlocal
- Localised projective measurement of a relativistic quantum field in non-inertial frames
Cited by in corpus (9)
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- Fundamental limitations to information transfer in accelerated frames
- Motion and gravity effects in the precision of quantum clocks
- Relativistic Quantum Communication