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ENTANGLEMENT OF GAUSSIAN STATES Gerardo Adesso

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

where Ω is the symplectic form<br />

N<br />

Ω = ω , ω =<br />

k=1<br />

0 1<br />

−1 0<br />

<br />

. (2.8)<br />

The space Hk is spanned by the Fock basis {|n〉k} of eigenstates of the number<br />

operator ˆnk = â †<br />

k âk, representing the Hamiltonian of the non-interacting mode via<br />

Eq. (2.2). The Hamiltonian of any mode is bounded from below, thus ensuring the<br />

stability of the system, so that for any mode a vacuum state |0〉k ∈ Hk exists, for<br />

which âk|0〉k = 0. The vacuum state of the global Hilbert space will be denoted by<br />

|0〉 = <br />

k |0〉k. In the single-mode Hilbert space Hk, the eigenstates of âk constitute<br />

the important set of coherent states [259], which is overcomplete in Hk. Coherent<br />

states result from applying the single-mode Weyl displacement operator ˆ Dk to the<br />

vacuum |0〉k, |α〉k = ˆ Dk(α)|0〉k, where<br />

ˆDk(α) = e αâ†<br />

k −α∗ âk , (2.9)<br />

and the coherent amplitude α ∈ satisfies âk|α〉k = α|α〉k. In terms of the Fock<br />

basis of mode k a coherent state reads<br />

1 −<br />

|α〉k = e 2 |α|2<br />

∞ αn √ |n〉k . (2.10)<br />

n!<br />

Tensor products of coherent states of different modes are obtained by applying the<br />

N-mode Weyl operators ˆ Dξ to the global vacuum |0〉. For future convenience, we<br />

define the operators ˆ Dξ in terms of the canonical operators ˆ R,<br />

n=1<br />

ˆDξ = e i ˆ R T Ωξ , with ξ ∈ 2N . (2.11)<br />

One has then |ξ〉 = ˆ Dξ|0〉, which entails âk|ξ〉 = (ξk + iξk+1)|ξ〉.<br />

2.1.1. Quantum phase-space picture<br />

The states of a CV system are the set of positive trace-class operators {ϱ} on the<br />

Hilbert space H , Eq. (2.1). However, the complete description of any quantum<br />

state ϱ of such an infinite-dimensional system can be provided by one of its s-ordered<br />

characteristic functions [16]<br />

χs(ξ) = Tr [ϱ ˆ Dξ] e sξ2 /2 , (2.12)<br />

with ξ ∈ 2N , · standing for the Euclidean norm of 2N . The vector ξ belongs<br />

to the real 2N-dimensional space Γ = ( 2N , Ω), which is called phase space, in<br />

analogy with classical Hamiltonian dynamics. One can see from the definition of<br />

the characteristic functions that in the phase space picture, the tensor product<br />

structure is replaced by a direct sum structure, so that the N-mode phase space is<br />

Γ = <br />

k Γk, where Γk = ( 2 , ω) is the local phase space associated with mode k.<br />

The family of characteristic functions is in turn related, via complex Fourier<br />

transform, to the quasi-probability distributions Ws, which constitute another set<br />

of complete descriptions of the quantum states<br />

Ws(ξ) = 1<br />

π2 <br />

κχs(κ) e iκTΩξ 2N<br />

d . (2.13)<br />

2N<br />

As well known, there exist states for which the function Ws is not a regular probability<br />

distribution for any s, because it can in general be singular or assume negative

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