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Designing spin-channel geometries for entanglement distribution

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PhysRevA.94.032302.pdf (481.0Kb)
Date
01/09/2016
Author
Levi, Elliott Kendrick
Kirton, Peter George
Lovett, Brendon William
Keywords
QC Physics
TK Electrical engineering. Electronics Nuclear engineering
DAS
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Abstract
We investigate different geometries of spin-1/2 nitrogen impurity channels for distributing entanglement between pairs of remote nitrogen vacancy centers (NVs) in diamond. To go beyond the system size limits imposed by directly solving the master equation, we implement a matrix product operator method to describe the open system dynamics. In so doing, we provide an early demonstration of how the time-evolving block decimation algorithm can be used for answering a problem related to a real physical system that could not be accessed by other methods. For a fixed NV separation there is an interplay between incoherent impurity spin decay and coherent entanglement transfer: Long-transfer-time, few-spin systems experience strong dephasing that can be overcome by increasing the number of spins in the channel. We examine how missing spins and disorder in the coupling strengths affect the dynamics, finding that in some regimes a spin ladder is a more effective conduit for information than a single-spin chain.
Citation
Levi , E K , Kirton , P G & Lovett , B W 2016 , ' Designing spin-channel geometries for entanglement distribution ' , Physical Review. A, Atomic, molecular, and optical physics , vol. 94 , no. 3 , 032302 . https://doi.org/10.1103/PhysRevA.94.032302
Publication
Physical Review. A, Atomic, molecular, and optical physics
Status
Peer reviewed
DOI
https://doi.org/10.1103/PhysRevA.94.032302
ISSN
1050-2947
Type
Journal article
Rights
© 2016, American Physical Society. This work is made available online in accordance with the publisher’s policies. This is the author created, accepted version manuscript following peer review and may differ slightly from the final published version. The final published version of this work is available at journals.aps.org / https://dx.doi.org/10.1103/PhysRevA.94.032302
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  • University of St Andrews Research
URI
http://hdl.handle.net/10023/9477

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