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Quantum Cryptography Approaching the Classical Limit

Christian Weedbrook, Stefano Pirandola, Seth Lloyd, Timothy C. Ralph

arXiv:1004.3345v3quant-ph

TL;DR

Deriving the paper’s main-text results requires Gaussian formalisms for continuous-variable quantum information. The paper provides a self-contained treatment and uses symplectic eigenvalues to characterize Gaussian systems, with a simplified expression for a specified two-mode covariance matrix.

Abstract

from arXiv · show

We consider the security of continuous-variable quantum cryptography as we approach the classical-limit, i.e., when the unknown preparation noise at the sender's station becomes significantly noisy or thermal (even by as much as 10,000 times the variance of the vacuum mode). We show that, provided the channel transmission losses do not exceed 50%, the security of quantum cryptography is not dependent on the channel transmission, and is therefore, incredibly robust against significant amounts of excess preparation noise. We extend these results to consider for the first time quantum cryptography at wavelengths considerably longer than optical and find that regions of security still exist all the way down to the microwave.

Introduction to Gaussian Formalisms

This section introduces a self-contained Gaussian formalism for analyzing continuous-variable quantum systems. It uses displacement and correlation matrices to characterize states, with symplectic eigenvalues supporting entropy and other system calculations.

Introduction to Gaussian Formalisms

Reverse Reconciliation

Reverse reconciliation with homodyne detection defines the key rate from Alice–Bob information minus Bob–Eve information. The channel model incorporates transmission and excess noise into Bob’s received quadratures.

Reverse Reconciliation

V = VS + V0, (31)

This section calculates Alice–Bob mutual information and Eve’s information using conditional variances and covariance matrices. It then obtains reverse-reconciliation key rates numerically for different preparation-noise values.

V = VS + V0, (31)

  • Bob’s estimate of Alice’s signal uses the signal quadrature rather than Alice’s signal-plus-noise variable.The resulting conditional variance is (1 − T)W + TV0.Source: V = VS + V0, (31) · p. 6
  • Eve’s information is calculated with the Holevo quantity from Eve’s and conditional Eve covariance matrices and their symplectic spectra.Source: V = VS + V0, (31) · pp. 6–7
  • The reverse-reconciliation key rate is calculated numerically for different preparation-noise values.Source: V = VS + V0, (31) · p. 7

Direct Reconciliation

Direct reconciliation with homodyne detection defines the key rate using Alice–Bob mutual information and Eve–Alice information. The Eve term is calculated from a conditional covariance matrix.

Direct Reconciliation

  • The direct-reconciliation key rate subtracts Eve–Alice information from Alice–Bob mutual information.Source: Direct Reconciliation · p. 7
  • The passage states that I(XA : XB) has already been calculated in Eq. (34), but does not provide the subsequent expression defining Eve’s contribution.Source: Direct Reconciliation · p. 7
  • For homodyne detection, Eve’s conditional covariance matrix is used to calculate S(E|XA).Source: Direct Reconciliation · p. 7

VE|QA = VE(V0, V ), (51)

This section gives the conditional Eve-mode symplectic spectrum and the expressions used to calculate the direct-reconciliation secret key rate numerically.

VE|QA = VE(V0, V ), (51)

  • The conditional symplectic spectrum νE|XA is specified using VE, defined in Eq. (36).The section identifies F and G as coefficients in the spectrum expressions.Source: VE|QA = VE(V0, V ), (51) · p. 7
  • The final direct-reconciliation secret key rate is calculated numerically using Eq. (49).The calculation is repeated for various preparation-noise values.Source: VE|QA = VE(V0, V ), (51) · p. 7
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