-
1
-
-
1542265850
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.69.064512
-
H. Eisaki, Phys. Rev. B PRBMDO 0163-1829 69, 064512 (2004). 10.1103/PhysRevB.69.064512
-
(2004)
Phys. Rev. B
, vol.69
, pp. 064512
-
-
Eisaki, H.1
-
2
-
-
0001652117
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.44.7749
-
M.K. Crawford, Phys. Rev. B PRBMDO 0163-1829 44, 7749 (1991). 10.1103/PhysRevB.44.7749
-
(1991)
Phys. Rev. B
, vol.44
, pp. 7749
-
-
Crawford, M.K.1
-
3
-
-
0030734156
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.78.338
-
J.M. Tranquada, Phys. Rev. Lett. 78, 338 (1997). PRLTAO 0031-9007 10.1103/PhysRevLett.78.338
-
(1997)
Phys. Rev. Lett.
, vol.78
, pp. 338
-
-
Tranquada, J.M.1
-
4
-
-
0035127676
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.86.500
-
S. Tajima, T. Noda, H. Eisaki, and S. Uchida, Phys. Rev. Lett. 86, 500 (2001). PRLTAO 0031-9007 10.1103/PhysRevLett.86.500
-
(2001)
Phys. Rev. Lett.
, vol.86
, pp. 500
-
-
Tajima, S.1
Noda, T.2
Eisaki, H.3
Uchida, S.4
-
6
-
-
5544306336
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.76.1348
-
B. Dabrowski, [Phys. Rev. Lett. 76, 1348 (1996)] reported similar results for (La,Nd)1.85(Sr,Ca,Ba)0.15CuO4. PRLTAO 0031-9007 10.1103/PhysRevLett.76.1348
-
(1996)
Phys. Rev. Lett.
, vol.76
, pp. 1348
-
-
Dabrowski, B.1
-
7
-
-
0000943406
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.83.3289
-
J.A. McAllister and J.P. Attfield, Phys. Rev. Lett. 83, 3289 (1999). PRLTAO 0031-9007 10.1103/PhysRevLett.83.3289
-
(1999)
Phys. Rev. Lett.
, vol.83
, pp. 3289
-
-
McAllister, J.A.1
Attfield, J.P.2
-
8
-
-
0037431290
-
-
NATUAS 0028-0836 10.1038/nature01496
-
K. McElroy, Nature (London) NATUAS 0028-0836 422, 592 (2003). 10.1038/nature01496
-
(2003)
Nature (London)
, vol.422
, pp. 592
-
-
McElroy, K.1
-
9
-
-
0038755147
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.67.104512
-
S. Ono and Yoichi Ando, Phys. Rev. B PRBMDO 0163-1829 67, 104512 (2003). 10.1103/PhysRevB.67.104512
-
(2003)
Phys. Rev. B
, vol.67
, pp. 104512
-
-
Ono, S.1
Ando, Y.2
-
10
-
-
0000641948
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.39.7244
-
W. Banhofer, Phys. Rev. B PRBMDO 0163-1829 39, 7244 (1989). 10.1103/PhysRevB.39.7244
-
(1989)
Phys. Rev. B
, vol.39
, pp. 7244
-
-
Banhofer, W.1
-
11
-
-
0028756417
-
-
PHYCE6 0921-4534 10.1016/0921-4534(94)90571-1
-
H. Nameki, M. Kikuchi, and Y. Syono, Physica (Amsterdam) 234C, 255 (1994). PHYCE6 0921-4534 10.1016/0921-4534(94)90571-1
-
(1994)
Physica (Amsterdam)
, vol.234
, pp. 255
-
-
Nameki, H.1
Kikuchi, M.2
Syono, Y.3
-
12
-
-
0033536661
-
-
SCIEAS 0036-8075 10.1126/science.286.5438.265
-
The Hall coefficient measured for y=0.6 Nd-LSCO is also the same as those shown in Fig. 1; T. Noda, H. Eisaki, and S. Uchida, Science SCIEAS 0036-8075 286, 265 (1999). 10.1126/science.286.5438.265
-
(1999)
Science
, vol.286
, pp. 265
-
-
Noda, T.1
Eisaki, H.2
Uchida, S.3
-
13
-
-
84944648082
-
-
ACACBN 0567-7394 10.1107/S0567739476001551
-
R.D. Shannon, Acta Crystallogr. Sect. A ACACBN 0567-7394 32, 751 (1976); 10.1107/S0567739476001551
-
(1976)
Acta Crystallogr. Sect. A
, vol.32
, pp. 751
-
-
Shannon, R.D.1
-
14
-
-
84856125335
-
-
http://abulafia.mt.ic.ac.uk/shannon/ptable.php.
-
-
-
-
15
-
-
50449115322
-
-
GCACAK 0016-7037 10.1016/0016-7037(52)90004-5
-
L.H. Ahrens, Geochim. Cosmochim. Acta GCACAK 0016-7037 2, 155 (1952), the ionic radii of La3+ and Sr2+ are almost identical. If we adopt the data in this reference, the values of Tc0 are close to those for La-Bi2201 and LSCO. 10.1016/0016-7037(52)90004-5
-
(1952)
Geochim. Cosmochim. Acta
, vol.2
, pp. 155
-
-
Ahrens, L.H.1
-
16
-
-
0000779336
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.76.684
-
Y. Fukuzumi, Phys. Rev. Lett. 76, 684 (1996). PRLTAO 0031-9007 10.1103/PhysRevLett.76.684
-
(1996)
Phys. Rev. Lett.
, vol.76
, pp. 684
-
-
Fukuzumi, Y.1
-
17
-
-
6944253061
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.74.3253
-
V.J. Emery and S.A. Kivelson, Phys. Rev. Lett. 74, 3253 (1995). PRLTAO 0031-9007 10.1103/PhysRevLett.74.3253
-
(1995)
Phys. Rev. Lett.
, vol.74
, pp. 3253
-
-
Emery, V.J.1
Kivelson, S.A.2
-
19
-
-
2942687850
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.92.187001
-
X.J. Zhou, Phys. Rev. Lett. 92, 187001 (2004). PRLTAO 0031-9007 10.1103/PhysRevLett.92.187001
-
(2004)
Phys. Rev. Lett.
, vol.92
, pp. 187001
-
-
Zhou, X.J.1
-
20
-
-
0032824555
-
-
SCIEAS 0036-8075 10.1126/science.285.5436.2110
-
T. Valla, Science SCIEAS 0036-8075 285, 2110 (1999). 10.1126/science.285. 5436.2110
-
(1999)
Science
, vol.285
, pp. 2110
-
-
Valla, T.1
-
22
-
-
13744249423
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.70.214503
-
L. Zhu, P.J. Hirshfeld, and D.J. Scalapino, Phys. Rev. B PRBMDO 0163-1829 70, 214503 (2004). 10.1103/PhysRevB.70.214503
-
(2004)
Phys. Rev. B
, vol.70
, pp. 214503
-
-
Zhu, L.1
Hirshfeld, P.J.2
Scalapino, D.J.3
-
23
-
-
0034647481
-
-
SCIEAS 0036-8075 10.1126/science.289.5477.277
-
D.L. Feng, Science SCIEAS 0036-8075 289, 277 (2000). 10.1126/science.289. 5477.277
-
(2000)
Science
, vol.289
, pp. 277
-
-
Feng, D.L.1
-
24
-
-
39249083908
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.87.227001
-
H. Ding, Phys. Rev. Lett. 87, 227001 (2001). PRLTAO 0031-9007 10.1103/PhysRevLett.87.227001
-
(2001)
Phys. Rev. Lett.
, vol.87
, pp. 227001
-
-
Ding, H.1
-
25
-
-
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
-
27
-
-
20844441260
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.70.092503
-
K. Tanaka, Phys. Rev. B PRBMDO 0163-1829 70, 092503 (2004). 10.1103/PhysRevB.70.092503
-
(2004)
Phys. Rev. B
, vol.70
, pp. 092503
-
-
Tanaka, K.1
-
28
-
-
27144448762
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.94.197005
-
K. McElroy, Phys. Rev. Lett. 94, 197005 (2005). PRLTAO 0031-9007 10.1103/PhysRevLett.94.197005
-
(2005)
Phys. Rev. Lett.
, vol.94
, pp. 197005
-
-
McElroy, K.1
-
29
-
-
3342950026
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.62.2317
-
Y.J. Uemura, Phys. Rev. Lett. 62, 2317 (1989). PRLTAO 0031-9007 10.1103/PhysRevLett.62.2317
-
(1989)
Phys. Rev. Lett.
, vol.62
, pp. 2317
-
-
Uemura, Y.J.1
|