An adaptation method to improve secret key rates of time-frequency QKD in atmospheric turbulence channels

Research output: Chapter in Book/Report/Conference proceedingConference contribution

2 Citations (Scopus)

Abstract

Free-space optical (FSO) channels can be characterized by random power fluctuations due to atmospheric turbulence, which is known as scintillation. Weak coherent source based FSO quantum key distribution (QKD) systems suffer from the scintillation effect because during the deep channel fading the expected detection rate drops, which then gives an eavesdropper opportunity to get additional information about protocol by performing photon number splitting (PNS) attack and blocking single-photon pulses without changing QBER. To overcome this problem, in this paper, we study a large-alphabet QKD protocol, which is achieved by using pulse-position modulation (PPM)-like approach that utilizes the time-frequency uncertainty relation of the weak coherent photon state, called here TF-PPM-QKD protocol. We first complete finite size analysis for TF-PPM-QKD protocol to give practical bounds against non-negligible statistical fluctuation due to finite resources in practical implementations. The impact of scintillation under strong atmospheric turbulence regime is studied then. To overcome the secure key rate performance degradation of TF-PPM-QKD caused by scintillation, we propose an adaptation method for compensating the scintillation impact. By changing source intensity according to the channel state information (CSI), obtained by classical channel, the adaptation method improves the performance of QKD system with respect to the secret key rate. The CSI of a time-varying channel can be predicted using stochastic models, such as autoregressive (AR) models. Based on the channel state predictions, we change the source intensity to the optimal value to achieve a higher secret key rate. We demonstrate that the improvement of the adaptation method is dependent on the prediction accuracy.

Original languageEnglish (US)
Title of host publicationFree-Space Laser Communication and Atmospheric Propagation XXVIII
PublisherSPIE
Volume9739
ISBN (Electronic)9781628419740
DOIs
StatePublished - 2016
EventFree-Space Laser Communication and Atmospheric Propagation XXVIII - San Francisco, United States
Duration: Feb 15 2016Feb 16 2016

Other

OtherFree-Space Laser Communication and Atmospheric Propagation XXVIII
CountryUnited States
CitySan Francisco
Period2/15/162/16/16

Fingerprint

Quantum cryptography
Quantum Key Distribution
Atmospheric turbulence
Atmospheric Turbulence
atmospheric turbulence
Scintillation
Pulse Position Modulation
Pulse position modulation
pulse position modulation
scintillation
Photon
Photons
Channel state information
Distribution System
Channel State Information
Free Space
Fluctuations
photons
Time-varying Channels
Uncertainty Relation

Keywords

  • adaptation method
  • atmospheric turbulence
  • free-space optical channel
  • Quantum key distribution (QKD)
  • secret key rate
  • time-frequency QKD

ASJC Scopus subject areas

  • Electronic, Optical and Magnetic Materials
  • Condensed Matter Physics
  • Computer Science Applications
  • Applied Mathematics
  • Electrical and Electronic Engineering

Cite this

An adaptation method to improve secret key rates of time-frequency QKD in atmospheric turbulence channels. / Sun, Xiaole; Djordjevic, Ivan B; Neifeld, Mark A.

Free-Space Laser Communication and Atmospheric Propagation XXVIII. Vol. 9739 SPIE, 2016. 97390Z.

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Sun, X, Djordjevic, IB & Neifeld, MA 2016, An adaptation method to improve secret key rates of time-frequency QKD in atmospheric turbulence channels. in Free-Space Laser Communication and Atmospheric Propagation XXVIII. vol. 9739, 97390Z, SPIE, Free-Space Laser Communication and Atmospheric Propagation XXVIII, San Francisco, United States, 2/15/16. https://doi.org/10.1117/12.2213035
Sun, Xiaole ; Djordjevic, Ivan B ; Neifeld, Mark A. / An adaptation method to improve secret key rates of time-frequency QKD in atmospheric turbulence channels. Free-Space Laser Communication and Atmospheric Propagation XXVIII. Vol. 9739 SPIE, 2016.
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N2 - Free-space optical (FSO) channels can be characterized by random power fluctuations due to atmospheric turbulence, which is known as scintillation. Weak coherent source based FSO quantum key distribution (QKD) systems suffer from the scintillation effect because during the deep channel fading the expected detection rate drops, which then gives an eavesdropper opportunity to get additional information about protocol by performing photon number splitting (PNS) attack and blocking single-photon pulses without changing QBER. To overcome this problem, in this paper, we study a large-alphabet QKD protocol, which is achieved by using pulse-position modulation (PPM)-like approach that utilizes the time-frequency uncertainty relation of the weak coherent photon state, called here TF-PPM-QKD protocol. We first complete finite size analysis for TF-PPM-QKD protocol to give practical bounds against non-negligible statistical fluctuation due to finite resources in practical implementations. The impact of scintillation under strong atmospheric turbulence regime is studied then. To overcome the secure key rate performance degradation of TF-PPM-QKD caused by scintillation, we propose an adaptation method for compensating the scintillation impact. By changing source intensity according to the channel state information (CSI), obtained by classical channel, the adaptation method improves the performance of QKD system with respect to the secret key rate. The CSI of a time-varying channel can be predicted using stochastic models, such as autoregressive (AR) models. Based on the channel state predictions, we change the source intensity to the optimal value to achieve a higher secret key rate. We demonstrate that the improvement of the adaptation method is dependent on the prediction accuracy.

AB - Free-space optical (FSO) channels can be characterized by random power fluctuations due to atmospheric turbulence, which is known as scintillation. Weak coherent source based FSO quantum key distribution (QKD) systems suffer from the scintillation effect because during the deep channel fading the expected detection rate drops, which then gives an eavesdropper opportunity to get additional information about protocol by performing photon number splitting (PNS) attack and blocking single-photon pulses without changing QBER. To overcome this problem, in this paper, we study a large-alphabet QKD protocol, which is achieved by using pulse-position modulation (PPM)-like approach that utilizes the time-frequency uncertainty relation of the weak coherent photon state, called here TF-PPM-QKD protocol. We first complete finite size analysis for TF-PPM-QKD protocol to give practical bounds against non-negligible statistical fluctuation due to finite resources in practical implementations. The impact of scintillation under strong atmospheric turbulence regime is studied then. To overcome the secure key rate performance degradation of TF-PPM-QKD caused by scintillation, we propose an adaptation method for compensating the scintillation impact. By changing source intensity according to the channel state information (CSI), obtained by classical channel, the adaptation method improves the performance of QKD system with respect to the secret key rate. The CSI of a time-varying channel can be predicted using stochastic models, such as autoregressive (AR) models. Based on the channel state predictions, we change the source intensity to the optimal value to achieve a higher secret key rate. We demonstrate that the improvement of the adaptation method is dependent on the prediction accuracy.

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