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ENTANGLEMENT OF GAUSSIAN STATES Gerardo Adesso

ENTANGLEMENT OF GAUSSIAN STATES Gerardo Adesso

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32 2. Gaussian states: structural properties<br />

Hilbert space H Phase space Γ<br />

dimension<br />

structure<br />

<br />

∞ 2N<br />

<br />

description ϱ χs, Ws<br />

Table 2.I. Schematic comparison between Hilbert-space and phase-space<br />

pictures for N-mode continuous variable systems.<br />

2.2. Mathematical description of Gaussian states<br />

The set of Gaussian states is, by definition, the set of states with Gaussian characteristic<br />

functions and quasi-probability distributions on the multimode quantum<br />

phase space. Such states are at the heart of information processing in CV systems<br />

[GA22, GA23, 40] and are the main subject of this Dissertation.<br />

2.2.1. Covariance matrix formalism<br />

From the definition it follows that a Gaussian state ϱ is completely characterized<br />

by the first and second statistical moments of the quadrature field operators,<br />

which will be denoted, respectively, by the vector of first moments ¯ <br />

R =<br />

〈 ˆ R1〉, 〈 ˆ R1〉, . . . , 〈 ˆ RN〉, 〈 ˆ <br />

Rn〉 and by the covariance matrix (CM) σ of elements<br />

σij = 1<br />

2 〈 ˆ Ri ˆ Rj + ˆ Rj ˆ Ri〉 − 〈 ˆ Ri〉〈 ˆ Rj〉 . (2.17)<br />

First moments can be arbitrarily adjusted by local unitary operations, namely<br />

displacements in phase space, i.e. applications of the single-mode Weyl operator<br />

Eq. (2.9) to locally re-center the reduced Gaussian corresponding to each single<br />

mode 5 . Such operations leave any informationally relevant property, such as entropy<br />

and entanglement, invariant: therefore, first moments are unimportant to the whole<br />

scope of our analysis and from now on (unless explicitly stated) we will set them<br />

to 0 without any loss of generality.<br />

With this position, the Wigner function of a Gaussian state can be written as<br />

follows in terms of phase-space quadrature variables<br />

W (R) =<br />

e− 1<br />

2 Rσ−1 R T<br />

π √ Det σ<br />

, (2.18)<br />

where R stands for the real phase-space vector (q1, p1, . . . , qN , pN) ∈ Γ. Despite the<br />

infinite dimension of the Hilbert space in which it lives, a complete description of an<br />

arbitrary Gaussian state (up to local unitary operations) is therefore encoded in the<br />

2N × 2N CM σ, which in the following will be assumed indifferently to denote the<br />

matrix of second moments of a Gaussian state, or the state itself. In the formalism<br />

of statistical mechanics, the CM elements are the two-point truncated correlation<br />

functions between the 2N canonical continuous variables. We notice also that the<br />

entries of the CM can be expressed as energies by multiplying them by the quantity<br />

ωk, where ωk is the frequency of each mode k, in such a way that Tr σ is related<br />

to the mean energy of the state, i.e. the average of the non-interacting Hamiltonian<br />

Eq. (2.2). This mean energy is generally unbounded in CV systems.<br />

5 Recall that the reduced state obtained from a Gaussian state by partial tracing over a subset<br />

of modes is still Gaussian.

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