Optimising the interconnection of free-space to fibre quantum networks

Optimising the interconnection between free-space and fibre links will be necessary for future quantum communication networks. In daylight free-space quantum communication based on direct detection, the required Field Of View (FoV) of the receiver system needs to be minimised to reduce solar backgro...

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Main Authors: Ocampos-Guillén Alejandro, Denisenko Natalia, Fernández-Mármol Verónica
Format: Article
Language:English
Published: EDP Sciences 2019-01-01
Series:EPJ Web of Conferences
Online Access:https://doi.org/10.1051/epjconf/201919800007
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spelling doaj-f6d09517127c410bb8eb0436c6450b322021-08-02T07:35:36ZengEDP SciencesEPJ Web of Conferences2100-014X2019-01-011980000710.1051/epjconf/201919800007epjconf_qtech2018_00007Optimising the interconnection of free-space to fibre quantum networksOcampos-Guillén Alejandro0Denisenko Natalia1Fernández-Mármol Verónica2Spanish National Research Council (CSIC), Institute of Physical and Information Technologies (ITEFI)Spanish National Research Council (CSIC), Institute of Physical and Information Technologies (ITEFI)Spanish National Research Council (CSIC), Institute of Physical and Information Technologies (ITEFI)Optimising the interconnection between free-space and fibre links will be necessary for future quantum communication networks. In daylight free-space quantum communication based on direct detection, the required Field Of View (FoV) of the receiver system needs to be minimised to reduce solar background noise coupling into the detectors. Reducing the FoV requires minimising beam wander effects caused by atmospheric turbulence through active optics. We implement a fine tracking system designed to correct tip and tilt wavefront aberrations, using two feedback loops; each of them consisting of a quadrant detector and a fast steering mirror for stabilising the beam in the whole optical axis of the receiver. We test the performance of the tracking system with different optical fibres in order to evaluate the reduction in the quantum bit error rate (QBER) caused by solar background noise. A reduction of 75% for single mode fibre was obtained, and 45% reduction for a 25 µm core diameter fibre, both cases for strong turbulence (Cn2~10-12 – 10-13 m-2/3) and 100 m propagating channel. These results look promising for enabling free-space Quantum Key Distribution (QKD) in wireless networks for realistic/adverse conditions such as daylight and strong turbulent regimes.https://doi.org/10.1051/epjconf/201919800007
collection DOAJ
language English
format Article
sources DOAJ
author Ocampos-Guillén Alejandro
Denisenko Natalia
Fernández-Mármol Verónica
spellingShingle Ocampos-Guillén Alejandro
Denisenko Natalia
Fernández-Mármol Verónica
Optimising the interconnection of free-space to fibre quantum networks
EPJ Web of Conferences
author_facet Ocampos-Guillén Alejandro
Denisenko Natalia
Fernández-Mármol Verónica
author_sort Ocampos-Guillén Alejandro
title Optimising the interconnection of free-space to fibre quantum networks
title_short Optimising the interconnection of free-space to fibre quantum networks
title_full Optimising the interconnection of free-space to fibre quantum networks
title_fullStr Optimising the interconnection of free-space to fibre quantum networks
title_full_unstemmed Optimising the interconnection of free-space to fibre quantum networks
title_sort optimising the interconnection of free-space to fibre quantum networks
publisher EDP Sciences
series EPJ Web of Conferences
issn 2100-014X
publishDate 2019-01-01
description Optimising the interconnection between free-space and fibre links will be necessary for future quantum communication networks. In daylight free-space quantum communication based on direct detection, the required Field Of View (FoV) of the receiver system needs to be minimised to reduce solar background noise coupling into the detectors. Reducing the FoV requires minimising beam wander effects caused by atmospheric turbulence through active optics. We implement a fine tracking system designed to correct tip and tilt wavefront aberrations, using two feedback loops; each of them consisting of a quadrant detector and a fast steering mirror for stabilising the beam in the whole optical axis of the receiver. We test the performance of the tracking system with different optical fibres in order to evaluate the reduction in the quantum bit error rate (QBER) caused by solar background noise. A reduction of 75% for single mode fibre was obtained, and 45% reduction for a 25 µm core diameter fibre, both cases for strong turbulence (Cn2~10-12 – 10-13 m-2/3) and 100 m propagating channel. These results look promising for enabling free-space Quantum Key Distribution (QKD) in wireless networks for realistic/adverse conditions such as daylight and strong turbulent regimes.
url https://doi.org/10.1051/epjconf/201919800007
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