ENTANGLEMENT OF GAUSSIAN STATES Gerardo Adesso
ENTANGLEMENT OF GAUSSIAN STATES Gerardo Adesso
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