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Quantum Information Theory with Gaussian Systems

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characteristic function<br />

χrand(ξ) = tr <br />

1<br />

T(ρ)Wξ = dη e<br />

c<br />

−ηT ·G·η/4<br />

tr Wη ρ W ∗ η Wξ<br />

<br />

= 1<br />

<br />

dη e<br />

c<br />

−ηT ·G·η/4 iσ(η,ξ)<br />

e χin(ξ)<br />

= exp −ξ T<br />

· (σ T<br />

G −1 σ) · ξ/4 χin(ξ).<br />

5.1 Setup<br />

In the Heisenberg picture, T maps Weyl operators to multiples of themselves, so it is<br />

a completely positive map: Wξ ↦→ Wξ exp −ξ T ·(σ T G −1 σ)·ξ/4 , where σ T G −1 σ ≥ 0<br />

(cf. Section 2.3). Since the factor c assures normalization, it is even a channel. A<br />

<strong>Gaussian</strong> input state <strong>with</strong> covariance matrix γ and displacement α is transformed<br />

into a <strong>Gaussian</strong> state <strong>with</strong> characteristic function<br />

χrand(ξ) = exp −ξ T<br />

· (γ + σ T<br />

G −1 σ) · ξ/4 − iσ(ξ, α) , (5.2)<br />

i.e. the covariance matrix is changed according to γ ↦→ γ + σ T G −1 σ, but the (average)<br />

displacement is not affected. This is visualized in Fig. 5.1: an initial coherent<br />

state |α〉〈α| is represented by alollipop stick, where amplitude and phase are depicted<br />

by the vector α and the uncertainty is indicated by the circle corresponding<br />

to the covariance matrix γ = (cf. Section 2.2); adding classical, uncorrelated <strong>Gaussian</strong><br />

noise <strong>with</strong> isotropic variance g, i.e. <strong>with</strong> covariance matrix G = /g, enlarges<br />

the uncertainty by σ T G −1 σ = g and hence the radius of the circle by g (the dotted<br />

and dashed circles for medium and larger g). Since the displacement is not affected,<br />

these circles are centered around the endpoint of α.<br />

In view of the discretization we define two variants of the above channel, a cutoff<br />

version T [ ] where the integration is restricted to phase space translations <strong>with</strong> absolute<br />

value |ξ| ≤ a and its discretized counterpart T Σ, which replaces the integration<br />

by a summation over a finite set of phase space displacements {ξk}k=1,...,K suitable<br />

to approximate the integral:<br />

T [](ρ) = 1<br />

c [ ]<br />

T Σ(ρ) = 1<br />

c Σ<br />

<br />

|ξ|≤a<br />

K<br />

k=1<br />

dξ e −ξT ·G·ξ/4 Wξ ρ W ∗ ξ , (5.3)<br />

e −ξT k ·G·ξk/4<br />

Wξk ρ W∗ , (5.4)<br />

ξk<br />

where c [ ] and c Σ provide normalization. The set {ξk} and the cutoff radius a remain<br />

to be determined below. For convenience, we introduce a short-hand notation for<br />

randomized coherent input states |α〉〈α| of Nf modes,<br />

T(α) = T |α〉〈α| <br />

and likewise for T [ ](α) and T Σ(α). Furthermore, we can write T(α) = W α T(0)W ∗ α<br />

for all three flavors of T.<br />

105

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