-
2
-
-
4243059985
-
-
10.1103/PhysRevLett.70.1895;
-
C. H. Bennett, G. Brassard, C. Crepeau, R. Jozsa, A. Peres, and W. K. Wootters, Phys. Rev. Lett. 70, 1895 (1993) 10.1103/PhysRevLett.70.1895
-
(1993)
Phys. Rev. Lett.
, vol.70
, pp. 1895
-
-
Bennett, C.H.1
Brassard, G.2
Crepeau, C.3
Jozsa, R.4
Peres, A.5
Wootters, W.K.6
-
3
-
-
4243789313
-
-
10.1103/PhysRevLett.76.722
-
C. H. Bennett, G. Brassard, S. Popescu, B. Schumacher, J. A. Smolin, and W. K. Wootters, Phys. Rev. Lett. 76, 722 (1996). 10.1103/PhysRevLett.76.722
-
(1996)
Phys. Rev. Lett.
, vol.76
, pp. 722
-
-
Bennett, C.H.1
Brassard, G.2
Popescu, S.3
Schumacher, B.4
Smolin, J.A.5
Wootters, W.K.6
-
7
-
-
43849112312
-
-
10.1103/RevModPhys.80.517
-
L. Amico, R. Fazio, A. Osterloh, and V. Vedral, Rev. Mod. Phys. 80, 517 (2008). 10.1103/RevModPhys.80.517
-
(2008)
Rev. Mod. Phys.
, vol.80
, pp. 517
-
-
Amico, L.1
Fazio, R.2
Osterloh, A.3
Vedral, V.4
-
8
-
-
0036757880
-
-
10.1103/PhysRevA.66.032110
-
T. J. Osborne and M. A. Nielsen, Phys. Rev. A 66, 032110 (2002). 10.1103/PhysRevA.66.032110
-
(2002)
Phys. Rev. A
, vol.66
, pp. 032110
-
-
Osborne, T.J.1
Nielsen, M.A.2
-
9
-
-
0037061511
-
-
10.1038/416608a
-
A. Osterloh, Nature (London) 416, 608 (2002). 10.1038/416608a
-
(2002)
Nature (London)
, vol.416
, pp. 608
-
-
Osterloh, A.1
-
10
-
-
0038115189
-
-
10.1103/PhysRevLett.90.227902
-
G. Vidal, J. I. Latorre, E. Rico, and A. Kitaev, Phys. Rev. Lett. 90, 227902 (2003). 10.1103/PhysRevLett.90.227902
-
(2003)
Phys. Rev. Lett.
, vol.90
, pp. 227902
-
-
Vidal, G.1
Latorre, J.I.2
Rico, E.3
Kitaev, A.4
-
14
-
-
4243408948
-
-
10.1103/PhysRevB.32.5845
-
G. Müller and R. E. Shrock, Phys. Rev. B 32, 5845 (1985). 10.1103/PhysRevB.32.5845
-
(1985)
Phys. Rev. B
, vol.32
, pp. 5845
-
-
Müller, G.1
Shrock, R.E.2
-
15
-
-
19644400692
-
-
10.1103/PhysRevLett.93.167203;
-
T. Roscilde, P. Verrucchi, A. Fubini, S. Haas, and V. Tognetti, Phys. Rev. Lett. 93, 167203 (2004) 10.1103/PhysRevLett.93.167203
-
(2004)
Phys. Rev. Lett.
, vol.93
, pp. 167203
-
-
Roscilde, T.1
Verrucchi, P.2
Fubini, A.3
Haas, S.4
Tognetti, V.5
-
16
-
-
18144403863
-
-
10.1103/PhysRevLett.94.147208
-
T. Roscilde, P. Verrucchi, A. Fubini, S. Haas, and V. Tognetti, Phys. Rev. Lett. 94, 147208 (2005). 10.1103/PhysRevLett.94.147208
-
(2005)
Phys. Rev. Lett.
, vol.94
, pp. 147208
-
-
Roscilde, T.1
Verrucchi, P.2
Fubini, A.3
Haas, S.4
Tognetti, V.5
-
17
-
-
28344439700
-
-
10.1103/PhysRevB.71.224420
-
S. Dusuel and J. Vidal, Phys. Rev. B 71, 224420 (2005). 10.1103/PhysRevB.71.224420
-
(2005)
Phys. Rev. B
, vol.71
, pp. 224420
-
-
Dusuel, S.1
Vidal, J.2
-
18
-
-
33747781412
-
-
10.1103/PhysRevA.74.022322;
-
L. Amico, F. Baroni, A. Fubini, D. Patane, V. Tognetti, and P. Verrucchi, Phys. Rev. A 74, 022322 (2006) 10.1103/PhysRevA.74.022322
-
(2006)
Phys. Rev. A
, vol.74
, pp. 022322
-
-
Amico, L.1
Baroni, F.2
Fubini, A.3
Patane, D.4
Tognetti, V.5
Verrucchi, P.6
-
19
-
-
34547248371
-
-
10.1088/1751-8113/40/32/010
-
F. Baroni, J. Phys. A 40, 9845 (2007). 10.1088/1751-8113/40/32/010
-
(2007)
J. Phys. A
, vol.40
, pp. 9845
-
-
Baroni, F.1
-
21
-
-
38349188224
-
-
10.1103/PhysRevA.77.012319
-
S. M. Giampaolo, F. Illuminati, P. Verrucchi, and S. De Siena, Phys. Rev. A 77, 012319 (2008). 10.1103/PhysRevA.77.012319
-
(2008)
Phys. Rev. A
, vol.77
, pp. 012319
-
-
Giampaolo, S.M.1
Illuminati, F.2
Verrucchi, P.3
De Siena, S.4
-
26
-
-
62549147786
-
-
10.1103/PhysRevB.79.060405;
-
G. L. Giorgi, Phys. Rev. B 79, 060405 (R) (2009) 10.1103/PhysRevB.79. 060405
-
(2009)
Phys. Rev. B
, vol.79
, pp. 060405
-
-
Giorgi, G.L.1
-
27
-
-
69549095607
-
-
10.1103/PhysRevB.80.019901
-
G. L. Giorgi, Phys. Rev. B 80, 019901 (E) (2009). 10.1103/PhysRevB.80. 019901
-
(2009)
Phys. Rev. B
, vol.80
, pp. 019901
-
-
Giorgi, G.L.1
-
28
-
-
35949030250
-
-
10.1103/PhysRevA.6.2211
-
F. T. Arecchi, E. Courtens, R. Gilmore, H. Thomas, Phys. Rev. A 6, 2211 (1972). 10.1103/PhysRevA.6.2211
-
(1972)
Phys. Rev. A
, vol.6
, pp. 2211
-
-
Arecchi, F.T.1
Courtens, E.2
Gilmore, R.3
Thomas, H.4
-
29
-
-
72049084196
-
-
In terms of Euler angles, e i α s z e i β s y e i γ s z |0□ = c e i θ s y | 0□, with tan θ 2 = e i α tan β 2 and c = e - i s (α+γ) (cosβ/2 cosθ/2) 2s [Eq. d3]. Φ can obviously be restricted to the x,y plane.
-
In terms of Euler angles, eiα sz eiβ sy eiγ sz |0□ =c eiθ sy |0□, with tan θ 2 = eiα tan β 2 and c= e-is (α+γ) (cosβ/2 cosθ/2) 2s [Eq.]. Φ can obviously be restricted to the x,y plane.
-
-
-
-
30
-
-
0037241260
-
-
10.1103/PhysRevA.67.012307
-
P. Rungta and C. M. Caves, Phys. Rev. A 67, 012307 (2003). 10.1103/PhysRevA.67.012307
-
(2003)
Phys. Rev. A
, vol.67
, pp. 012307
-
-
Rungta, P.1
Caves, C.M.2
-
31
-
-
34547411480
-
-
10.1088/1751-8113/40/29/019
-
F. Franchini, J. Phys. A 40, 8467 (2007). 10.1088/1751-8113/40/29/019
-
(2007)
J. Phys. A
, vol.40
, pp. 8467
-
-
Franchini, F.1
-
32
-
-
0036509287
-
-
10.1103/PhysRevA.65.032314
-
G. Vidal and R. F. Werner, Phys. Rev. A 65, 032314 (2002). 10.1103/PhysRevA.65.032314
-
(2002)
Phys. Rev. A
, vol.65
, pp. 032314
-
-
Vidal, G.1
Werner, R.F.2
-
33
-
-
0000727092
-
-
10.1103/PhysRevA.58.883;
-
K. Zyczkowski, P. Horodecki, A. Sanpera, and M. Lewenstein, Phys. Rev. A 58, 883 (1998) 10.1103/PhysRevA.58.883
-
(1998)
Phys. Rev. A
, vol.58
, pp. 883
-
-
Zyczkowski, K.1
Horodecki, P.2
Sanpera, A.3
Lewenstein, M.4
-
34
-
-
0001226716
-
-
10.1103/PhysRevA.60.3496
-
K. Zyczkowski, Phys. Rev. A 60, 3496 (1999). 10.1103/PhysRevA.60.3496
-
(1999)
Phys. Rev. A
, vol.60
, pp. 3496
-
-
Zyczkowski, K.1
-
35
-
-
34547368191
-
-
10.1103/PhysRevA.75.062117
-
A. Datta, S. T. Flammia, A. Shaji, and C. M. Caves, Phys. Rev. A 75, 062117 (2007). 10.1103/PhysRevA.75.062117
-
(2007)
Phys. Rev. A
, vol.75
, pp. 062117
-
-
Datta, A.1
Flammia, S.T.2
Shaji, A.3
Caves, C.M.4
-
37
-
-
4243684526
-
-
10.1103/PhysRevLett.80.2245
-
W. K. Wootters, Phys. Rev. Lett. 80, 2245 (1998). 10.1103/PhysRevLett.80. 2245
-
(1998)
Phys. Rev. Lett.
, vol.80
, pp. 2245
-
-
Wootters, W.K.1
-
38
-
-
0037574296
-
-
10.1103/PhysRevLett.77.1413
-
A. Peres, Phys. Rev. Lett. 77, 1413 (1996). 10.1103/PhysRevLett.77.1413
-
(1996)
Phys. Rev. Lett.
, vol.77
, pp. 1413
-
-
Peres, A.1
-
39
-
-
27144456877
-
-
10.1103/PhysRevA.72.012335;
-
R. Rossignoli and N. Canosa, Phys. Rev. A 72, 012335 (2005) 10.1103/PhysRevA.72.012335
-
(2005)
Phys. Rev. A
, vol.72
, pp. 012335
-
-
Rossignoli, R.1
Canosa, N.2
-
40
-
-
33644513410
-
-
10.1103/PhysRevA.73.022347
-
N. Canosa and R. Rossignoli, Phys. Rev. A 73, 022347 (2006). 10.1103/PhysRevA.73.022347
-
(2006)
Phys. Rev. A
, vol.73
, pp. 022347
-
-
Canosa, N.1
Rossignoli, R.2
-
41
-
-
0039624459
-
-
10.1103/PhysRevA.40.4277
-
R. F. Werner, Phys. Rev. A 40, 4277 (1989). 10.1103/PhysRevA.40.4277
-
(1989)
Phys. Rev. A
, vol.40
, pp. 4277
-
-
Werner, R.F.1
-
44
-
-
72049130763
-
-
For a full isotropic coupling 1 2 ∑i,j vij si □ sj, θ remains arbitrary while Eq. d5 leads to bi =0 if sinθ ≠ 0: At zero field, any global coherent state is here an exact eigenstate.
-
For a full isotropic coupling 1 2 ∑ i,j vij si □ sj, θ remains arbitrary while Eq. leads to bi =0 if sinθ ≠ 0: At zero field, any global coherent state is here an exact eigenstate.
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