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ENTANGLEMENT OF GAUSSIAN STATES Gerardo Adesso

ENTANGLEMENT OF GAUSSIAN STATES Gerardo Adesso

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8.2. Entanglement in partially symmetric four-mode Gaussian states 149<br />

by reversing time in the subspace of any chosen single subsystem [218, 265] (PPT<br />

criterion, see Sec. 3.1.1). This inseparability condition is readily verified for the<br />

family of states in Eq. (8.1) yielding that, for all nonzero values of the squeezings<br />

s and a, σ is entangled with respect to any global bipartition of the modes. This<br />

follows from the global purity of the state, together with the observation that the<br />

determinant of each reduced one- and two-mode CM obtainable from Eq. (8.1) is<br />

strictly bigger than 1 for any nonzero squeezings. The state is thus said to be fully<br />

inseparable [111], i.e. it contains genuine four-partite entanglement.<br />

Following our previous studies on CV entanglement sharing (see Chapters 6 and<br />

7) we choose to measure bipartite entanglement by means of the Gaussian contangle<br />

Gτ , an entanglement monotone under Gaussian LOCC, computable according to<br />

Eq. (6.13).<br />

In the four-mode state with CM σ, we can evaluate the bipartite Gaussian<br />

contangle in closed form for all pairwise reduced (mixed) states of two modes i<br />

and j, described by a CM σ i|j. By applying again PPT criterion (see Sec. 3.1.1),<br />

one finds that the two-mode states indexed by the partitions 1|3, 2|4, and 1|4, are<br />

separable. For the remaining two-mode states the computation is possible thanks to<br />

the results of Sec. 4.5.2. Namely, the reduced state of modes 2 and 3, σ23, belongs<br />

to the class of GMEMS (defined in Sec. 4.3.3.1); for it Eq. (4.76) yields 21<br />

m 2|3 =<br />

−1+2 cosh 2 (2a) cosh 2 s+3 cosh(2s)−4 sinh 2 a sinh(2s)<br />

4[cosh 2 a+e 2s sinh 2 a] , a < arcsinh[ √ tanh s] ;<br />

1, otherwise.<br />

(8.2)<br />

On the other hand, the states σ 1|2 and σ 3|4 are GMEMMS (defined in Sec. 4.3.2),<br />

i.e. simultaneous GMEMS and GLEMS, for which either Eq. (4.74) or Eq. (4.76)<br />

give<br />

m 1|2 = m 3|4 = cosh 2a . (8.3)<br />

Accordingly, one can compute the pure-state entanglements between one probe<br />

mode and the remaining three modes. In this case one has simply m i|(jkl) = Det σi.<br />

One finds from Eq. (8.1),<br />

m 1|(234) = m 4|(123) = cosh 2 a + cosh(2s) sinh 2 a ,<br />

m 2|(134) = m 3|(124) = sinh 2 a + cosh(2s) cosh 2 a .<br />

(8.4)<br />

Concerning the structure of bipartite entanglement, Eqs. (6.13, 8.3) imply that<br />

the Gaussian contangle in the mixed two-mode states σ1|2 and σ3|4 is 4a2 , irrespective<br />

of the value of s. This quantity is exactly equal to the degree of entanglement<br />

in a pure two-mode squeezed state Si,j(a)S T i,j<br />

(a) of modes i and j generated with<br />

the same squeezing a. In fact, the two-mode mixed state σ 1|2 (and, equivalently,<br />

σ 3|4) serves as a proper resource for CV teleportation [39, 89], realizing a perfect<br />

transfer (unit fidelity 22 ) in the limit of infinite squeezing a.<br />

21 We refer to the notation of Eq. (6.13) and write, for each partition i|j, the corresponding<br />

parameter m i|j involved in the optimization problem which defines the Gaussian contangle.<br />

22 The fidelity F ≡ 〈ψ in |ϱ out |ψ in 〉 (“in” and “out” being input and output state, respectively)<br />

quantifies the teleportation success, as detailed in Chapter 12. For single-mode coherent input<br />

states and σ 1|2 or σ 3|4 employed as entangled resources, F = (1+e −2a cosh 2 s) −1 . It reaches unity<br />

for a ≫ 0 even in presence of high interpair entanglement (s ≫ 0), provided that a approaches<br />

infinity much faster than s.

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