ENTANGLEMENT OF GAUSSIAN STATES Gerardo Adesso
ENTANGLEMENT OF GAUSSIAN STATES Gerardo Adesso
ENTANGLEMENT OF GAUSSIAN STATES Gerardo Adesso
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6.2. Monogamy of distributed entanglement in N-mode Gaussian states 117<br />
systems with an arbitrary number N of modes and parties S1, . . . , SN , thus generalizing<br />
the results of the previous subsection.<br />
As a measure of bipartite entanglement, we employ the Gaussian tangle τG<br />
defined via the square of negativity, Eqs. (6.14, 6.15), in direct analogy with the<br />
case of N-qubit systems [169]. Our proof is based on the symplectic analysis of<br />
CMs (see Chapter 2) and on the properties of Gaussian entanglement measures (see<br />
Sec. 3.2.2). The monogamy constraint has important implications on the structural<br />
characterization of entanglement sharing in CV systems [GA10, GA11, GA16, GA15],<br />
in the context of entanglement frustration in harmonic lattices [272], and for practical<br />
applications such as secure key distribution and communication networks with<br />
continuous variables (see Part V).<br />
Given an arbitrary N-mode Gaussian state ϱS1|S2...SN , we now prove the general<br />
monogamy inequality<br />
τG(ϱS1|S2...SN ) ≥<br />
N<br />
l=2<br />
τG(ϱS1|Sl ) , (6.21)<br />
where we have in general renamed the modes so that the probe subsystem in<br />
Eq. (6.17) is S1, for mere convenience.<br />
To this end, we can assume without loss of generality that the reduced two-mode<br />
states ϱS1|Sl = TrS2...Sl−1Sl+1...SN ϱS1|S2...SN of subsystems (S1Sl) (l = 2, . . . , N)<br />
are all entangled. In fact, if for instance ϱS1|S2 is separable, then τG(ϱS1|S3...SN ) ≤<br />
τG(ϱS1|S2...SN ) because the partial trace over the subsystem S2 is a local Gaussian<br />
operation that does not increase the Gaussian entanglement. Furthermore, by<br />
the convex roof construction of the Gaussian tangle, it is sufficient to prove the<br />
monogamy inequality for any pure Gaussian state ϱ p<br />
(see also Refs. [59,<br />
S1|S2...SN<br />
169]). Therefore, in the following we can always assume that ϱS1|S2...SN is a pure<br />
Gaussian state for which the reduced states ϱS1|Sl (l = 2, . . . , N) are all entangled.<br />
We start by computing the left-hand side of Eq. (6.21). Since ϱS1|S2...SN is<br />
a 1 × (N − 1) pure Gaussian state, its CM σ is characterized by the condition<br />
Eq. (2.55), which implies<br />
Det α +<br />
N<br />
Det γl = 1 , (6.22)<br />
l=2<br />
where γl is the matrix encoding intermodal correlations between mode 1 and mode<br />
l in the reduced state ϱS1|Sl (l = 2, . . . , N), described by a CM [see Eq. (4.1)]<br />
σ S1|Sl =<br />
⎛<br />
⎜<br />
⎝<br />
σ1,1 σ1,2 σ1,2l−1 σ1,2l<br />
σ2,1 σ2,2 σ2,2l−1 σ2,2l<br />
σ2l−1,1 σ2l−1,2 σ2l−1,2l−1 σ2l−1,2l<br />
σ2l,1 σ2l,2 σ2l,2l−1 σ2l,2l<br />
⎞<br />
⎟<br />
⎠ =<br />
α γl<br />
γ T l<br />
β l<br />
<br />
. (6.23)<br />
As ϱ S1|Sl is entangled, Det γ l is negative [218], see Eq. (4.16). It is useful to<br />
introduce the auxiliary quantities<br />
such that one has Det α = 1 + <br />
l Υl/4 .<br />
Υl = −4Det γl > 0 , (6.24)