-
1
-
-
0000857055
-
-
RMPHAT 0034-6861 10.1103/RevModPhys.70.1039
-
M. Imada, A. Fujimori, and Y. Tokura, Rev. Mod. Phys. 70, 1039 (1998). RMPHAT 0034-6861 10.1103/RevModPhys.70.1039
-
(1998)
Rev. Mod. Phys.
, vol.70
, pp. 1039
-
-
Imada, M.1
Fujimori, A.2
Tokura, Y.3
-
2
-
-
3242875501
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.70.2126
-
Y. Tokura, Phys. Rev. Lett. 70, 2126 (1993). PRLTAO 0031-9007 10.1103/PhysRevLett.70.2126
-
(1993)
Phys. Rev. Lett.
, vol.70
, pp. 2126
-
-
Tokura, Y.1
-
3
-
-
0035811138
-
-
MSBTEK 0921-5107 10.1016/S0921-5107(01)00569-4
-
M. Izumi, Mater. Sci. Eng. B 84, 53 (2001). MSBTEK 0921-5107 10.1016/S0921-5107(01)00569-4
-
(2001)
Mater. Sci. Eng. B
, vol.84
, pp. 53
-
-
Izumi, M.1
-
4
-
-
0037179671
-
-
NATUAS 0028-0836 10.1038/nature00977
-
A. Ohtomo, D.A. Muller, J.L. Grazul, and H.Y. Hwang, Nature (London) NATUAS 0028-0836 419, 378 (2002). 10.1038/nature00977
-
(2002)
Nature (London)
, vol.419
, pp. 378
-
-
Ohtomo, A.1
Muller, D.A.2
Grazul, J.L.3
Hwang, H.Y.4
-
5
-
-
33645769196
-
-
NPAHAX 1745-2481 10.1038/nphys272
-
J. Chakhalian, Nature Phys. 2, 244 (2006). NPAHAX 1745-2481 10.1038/nphys272
-
(2006)
Nature Phys.
, vol.2
, pp. 244
-
-
Chakhalian, J.1
-
6
-
-
0035939262
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.87.047003
-
E. Pavarini, Phys. Rev. Lett. 87, 047003 (2001). PRLTAO 0031-9007 10.1103/PhysRevLett.87.047003
-
(2001)
Phys. Rev. Lett.
, vol.87
, pp. 047003
-
-
Pavarini, E.1
-
7
-
-
0033677485
-
-
ARMSCX 0084-6600 10.1146/annurev.matsci.30.1.451
-
T. Kimura and Y. Tokura, Annu. Rev. Mater. Sci. 30, 451 (2000). ARMSCX 0084-6600 10.1146/annurev.matsci.30.1.451
-
(2000)
Annu. Rev. Mater. Sci.
, vol.30
, pp. 451
-
-
Kimura, T.1
Tokura, Y.2
-
8
-
-
1942421142
-
-
NATUAS 0028-0836 10.1038/nature02450
-
S. Okamoto and A.J. Millis, Nature (London) NATUAS 0028-0836 428, 630 (2004). 10.1038/nature02450
-
(2004)
Nature (London)
, vol.428
, pp. 630
-
-
Okamoto, S.1
Millis, A.J.2
-
9
-
-
0001132637
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.45.8209
-
J.B. Torrance, Phys. Rev. B PRBMDO 0163-1829 45, 8209 (1992). 10.1103/PhysRevB.45.8209
-
(1992)
Phys. Rev. B
, vol.45
, pp. 8209
-
-
Torrance, J.B.1
-
10
-
-
0001088066
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.82.3871
-
J.A. Alonso, Phys. Rev. Lett. 82, 3871 (1999). PRLTAO 0031-9007 10.1103/PhysRevLett.82.3871
-
(1999)
Phys. Rev. Lett.
, vol.82
, pp. 3871
-
-
Alonso, J.A.1
-
11
-
-
42749099658
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.69.153105
-
J.-S. Zhou and J.B. Goodenough, Phys. Rev. B PRBMDO 0163-1829 69, 153105 (2004). 10.1103/PhysRevB.69.153105
-
(2004)
Phys. Rev. B
, vol.69
, pp. 153105
-
-
Zhou, J.-S.1
Goodenough, J.B.2
-
13
-
-
33645369668
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.73.100409
-
V. Scagnoli, Phys. Rev. B PRBMDO 0163-1829 73, 100409(R) (2006). 10.1103/PhysRevB.73.100409
-
(2006)
Phys. Rev. B
, vol.73
-
-
Scagnoli, V.1
-
14
-
-
0037849227
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.66.115107
-
N. Manini, G.E. Santoro, A. Dal Corso, and E. Tosatti, Phys. Rev. B PRBMDO 0163-1829 66, 115107 (2002). 10.1103/PhysRevB.66.115107
-
(2002)
Phys. Rev. B
, vol.66
, pp. 115107
-
-
Manini, N.1
Santoro, G.E.2
Dal Corso, A.3
Tosatti, E.4
-
15
-
-
0000751011
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.54.R11026
-
O. Gunnarsson, E. Koch, and R.M. Martin, Phys. Rev. B PRBMDO 0163-1829 54, R11026 (1996). 10.1103/PhysRevB.54.R11026
-
(1996)
Phys. Rev. B
, vol.54
, pp. 11026
-
-
Gunnarsson, O.1
Koch, E.2
Martin, R.M.3
-
16
-
-
2942617341
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.92.167201
-
M.V. Mostovoy and D.I. Khomskii, Phys. Rev. Lett. 92, 167201 (2004). PRLTAO 0031-9007 10.1103/PhysRevLett.92.167201
-
(2004)
Phys. Rev. Lett.
, vol.92
, pp. 167201
-
-
Mostovoy, M.V.1
Khomskii, D.I.2
-
17
-
-
29744453474
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.72.214431
-
A.M. Oleś, G. Khaliullin, P. Horsch, and L.F. Feiner, Phys. Rev. B PRBMDO 0163-1829 72, 214431 (2005). 10.1103/PhysRevB.72.214431
-
(2005)
Phys. Rev. B
, vol.72
, pp. 214431
-
-
Oleś, A.M.1
Khaliullin, G.2
Horsch, P.3
Feiner, L.F.4
-
19
-
-
33244479203
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.94.206401
-
S. Zhou, Phys. Rev. Lett. 94, 206401 (2005). PRLTAO 0031-9007 10.1103/PhysRevLett.94.206401
-
(2005)
Phys. Rev. Lett.
, vol.94
, pp. 206401
-
-
Zhou, S.1
-
20
-
-
0007690360
-
-
SUSTEF 0953-2048 10.1088/0953-2048/1/1/009
-
F.C. Zhang, C. Gros, T.M. Rice, and H. Shiba, Supercond. Sci. Technol. SUSTEF 0953-2048 1, 36 (1988). 10.1088/0953-2048/1/1/009
-
(1988)
Supercond. Sci. Technol.
, vol.1
, pp. 36
-
-
Zhang, F.C.1
Gros, C.2
Rice, T.M.3
Shiba, H.4
-
21
-
-
0001503164
-
-
At a first glance, La2NiMO6 superlattice might seem as an analog of layered perovskite La2-xSrxNiO4 at x/1 compositions [PRBMDO 0163-1829 10.1103/PhysRevB.43.1229
-
At a first glance, La2NiMO6 superlattice might seem as an analog of layered perovskite La2-xSrxNiO4 at x/1 compositions [R.J. Cava, Phys. Rev. B PRBMDO 0163-1829 43, 1229 (1991)], where an average valence state is Ni3+. However, there are two crucial differences. First, LaSrNiO4 is a solid solution of La and Sr where large local variations of the ratio La/Sr (forming perhaps some patterns) are possible. This should lead to mixed valence states Ni2+,3+,4+ and strong disorder effects. Second, there is no compression of NiO6 octahedra in La2-xSrxNiO4, which are rather elongated at small x and become of a regular shape at x/1. For these reasons, La2NiMO6 superlattice and La2-xSrxNiO4 solid solution should have different properties. 10.1103/PhysRevB.43.1229
-
(1991)
Phys. Rev. B
, vol.43
, pp. 1229
-
-
Cava, R.J.1
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