-
1
-
-
0000911909
-
-
10.1103/PhysRevLett.59.1041
-
P. A. Montano, G. W. Fernando, B. R. Cooper, E. R. Moog, H. M. Naik, S. D. Bader, Y. C. Lee, Y. N. Darici, H. Min, and J. Marcano, Phys. Rev. Lett. 59, 1041 (1987). 10.1103/PhysRevLett.59.1041
-
(1987)
Phys. Rev. Lett.
, vol.59
, pp. 1041
-
-
Montano, P.A.1
Fernando, G.W.2
Cooper, B.R.3
Moog, E.R.4
Naik, H.M.5
Bader, S.D.6
Lee, Y.C.7
Darici, Y.N.8
Min, H.9
Marcano, J.10
-
2
-
-
3342971059
-
-
10.1103/PhysRevLett.69.3831
-
J. Thomassen, F. May, B. Feldmann, M. Wuttig, and H. Ibach, Phys. Rev. Lett. 69, 3831 (1992). 10.1103/PhysRevLett.69.3831
-
(1992)
Phys. Rev. Lett.
, vol.69
, pp. 3831
-
-
Thomassen, J.1
May, F.2
Feldmann, B.3
Wuttig, M.4
Ibach, H.5
-
3
-
-
3342943166
-
-
10.1103/PhysRevLett.72.3112
-
D. Li, M. Freitag, J. Pearson, Z. Q. Qiu, and S. D. Bader, Phys. Rev. Lett. 72, 3112 (1994). 10.1103/PhysRevLett.72.3112
-
(1994)
Phys. Rev. Lett.
, vol.72
, pp. 3112
-
-
Li, D.1
Freitag, M.2
Pearson, J.3
Qiu, Z.Q.4
Bader, S.D.5
-
4
-
-
0029185168
-
-
10.1016/0039-6028(95)90013-6
-
S. Müller, P. Bayer, A. Kinne, P. Schmailzl, and K. Heinz, Surf. Sci. 322, 21 (1995). 10.1016/0039-6028(95)90013-6
-
(1995)
Surf. Sci.
, vol.322
, pp. 21
-
-
Müller, S.1
Bayer, P.2
Kinne, A.3
Schmailzl, P.4
Heinz, K.5
-
5
-
-
0000848591
-
-
10.1103/PhysRevB.59.1196
-
H. Jenniches, J. Shen, C. V. Mohan, S. S. Manoharan, J. Barthel, P. Ohresser, M. Klaua, and J. Kirschner, Phys. Rev. B 59, 1196 (1999). 10.1103/PhysRevB.59.1196
-
(1999)
Phys. Rev. B
, vol.59
, pp. 1196
-
-
Jenniches, H.1
Shen, J.2
Mohan, C.V.3
Manoharan, S.S.4
Barthel, J.5
Ohresser, P.6
Klaua, M.7
Kirschner, J.8
-
6
-
-
39249085040
-
-
10.1103/PhysRevLett.87.227204
-
D. Qian, X. F. Jin, J. Barthel, M. Klaua, and J. Kirschner, Phys. Rev. Lett. 87, 227204 (2001). 10.1103/PhysRevLett.87.227204
-
(2001)
Phys. Rev. Lett.
, vol.87
, pp. 227204
-
-
Qian, D.1
Jin, X.F.2
Barthel, J.3
Klaua, M.4
Kirschner, J.5
-
7
-
-
0034884206
-
-
10.1103/PhysRevB.63.205413
-
M. Weinelt, S. Schwarz, H. Baier, S. Müller, L. Hammer, K. Heinz, and Th. Fauster, Phys. Rev. B 63, 205413 (2001). 10.1103/PhysRevB.63.205413
-
(2001)
Phys. Rev. B
, vol.63
, pp. 205413
-
-
Weinelt, M.1
Schwarz, S.2
Baier, H.3
Müller, S.4
Hammer, L.5
Heinz, K.6
Fauster, Th.7
-
8
-
-
0037433303
-
-
10.1088/0953-8984/15/5/310
-
K. Amemiya, S. Kitagawa, D. Matsumura, T. Yokoyama, and T. Ohta, J. Phys.: Condens. Matter 15, S561 (2003). 10.1088/0953-8984/15/5/310
-
(2003)
J. Phys.: Condens. Matter
, vol.15
, pp. 561
-
-
Amemiya, K.1
Kitagawa, S.2
Matsumura, D.3
Yokoyama, T.4
Ohta, T.5
-
9
-
-
1542337059
-
-
10.1063/1.1645330
-
K. Amemiya, S. Kitagawa, D. Matsumura, T. H. Abe, T. Ohta, and T. Tokoyama, Appl. Phys. Lett. 84, 936 (2004). 10.1063/1.1645330
-
(2004)
Appl. Phys. Lett.
, vol.84
, pp. 936
-
-
Amemiya, K.1
Kitagawa, S.2
Matsumura, D.3
Abe, T.H.4
Ohta, T.5
Tokoyama, T.6
-
10
-
-
15544378442
-
-
10.1103/PhysRevB.71.035409
-
H. L. Meyerheim, R. Popescu, D. Sander, J. Kirschner, O. Robach, and S. Ferrer, Phys. Rev. B 71, 035409 (2005). 10.1103/PhysRevB.71.035409
-
(2005)
Phys. Rev. B
, vol.71
, pp. 035409
-
-
Meyerheim, H.L.1
Popescu, R.2
Sander, D.3
Kirschner, J.4
Robach, O.5
Ferrer, S.6
-
12
-
-
0001416906
-
-
10.1103/PhysRevB.54.15937
-
R. Lorenz and J. Hafner, Phys. Rev. B 54, 15937 (1996). 10.1103/PhysRevB.54.15937
-
(1996)
Phys. Rev. B
, vol.54
, pp. 15937
-
-
Lorenz, R.1
Hafner, J.2
-
13
-
-
0008878334
-
-
10.1103/PhysRevLett.79.507
-
T. Asada and S. Blügel, Phys. Rev. Lett. 79, 507 (1997). 10.1103/PhysRevLett.79.507
-
(1997)
Phys. Rev. Lett.
, vol.79
, pp. 507
-
-
Asada, T.1
Blügel, S.2
-
15
-
-
0041127188
-
-
10.1103/PhysRevB.56.2646
-
D. Spišák and J. Hafner, Phys. Rev. B 56, 2646 (1997). 10.1103/PhysRevB.56.2646
-
(1997)
Phys. Rev. B
, vol.56
, pp. 2646
-
-
Spišák, D.1
Hafner, J.2
-
16
-
-
0001146683
-
-
10.1103/PhysRevLett.84.4709
-
R. E. Camley and D. Li, Phys. Rev. Lett. 84, 4709 (2000). 10.1103/PhysRevLett.84.4709
-
(2000)
Phys. Rev. Lett.
, vol.84
, pp. 4709
-
-
Camley, R.E.1
Li, D.2
-
17
-
-
0037041092
-
-
10.1103/PhysRevLett.88.147201
-
S. S. A. Razee, J. B. Staunton, L. Szunyogh, and B. L. Gyorffy, Phys. Rev. Lett. 88, 147201 (2002). 10.1103/PhysRevLett.88.147201
-
(2002)
Phys. Rev. Lett.
, vol.88
, pp. 147201
-
-
Razee, S.S.A.1
Staunton, J.B.2
Szunyogh, L.3
Gyorffy, B.L.4
-
18
-
-
18744425898
-
-
10.1103/PhysRevLett.85.5424
-
M. Pajda, J. Kudrnovsky, I. Turek, V. Drchal, and P. Bruno, Phys. Rev. Lett. 85, 5424 (2000). 10.1103/PhysRevLett.85.5424
-
(2000)
Phys. Rev. Lett.
, vol.85
, pp. 5424
-
-
Pajda, M.1
Kudrnovsky, J.2
Turek, I.3
Drchal, V.4
Bruno, P.5
-
19
-
-
0036695317
-
-
10.1103/PhysRevB.66.052417
-
D. Spišák and J. Hafner, Phys. Rev. B 66, 052417 (2002). 10.1103/PhysRevB.66.052417
-
(2002)
Phys. Rev. B
, vol.66
, pp. 052417
-
-
Spišák, D.1
Hafner, J.2
-
22
-
-
0001640352
-
-
10.1103/PhysRevB.3.3887
-
D. L. Mills, Phys. Rev. B 3, 3887 (1971). 10.1103/PhysRevB.3.3887
-
(1971)
Phys. Rev. B
, vol.3
, pp. 3887
-
-
Mills, D.L.1
-
24
-
-
4243656871
-
-
10.1103/PhysRevB.8.4427
-
R. A. Weiner, Phys. Rev. B 8, 4427 (1973). 10.1103/PhysRevB.8.4427
-
(1973)
Phys. Rev. B
, vol.8
, pp. 4427
-
-
Weiner, R.A.1
-
25
-
-
26344476404
-
-
10.1103/PhysRevB.8.4424
-
D. L. Mills, Phys. Rev. B 8, 4424 (1973). 10.1103/PhysRevB.8.4424
-
(1973)
Phys. Rev. B
, vol.8
, pp. 4424
-
-
Mills, D.L.1
-
27
-
-
0037979775
-
-
10.1088/0305-4608/14/12/025
-
L. M. Small and V. Heine, J. Phys. F 14, 3041 (1984). 10.1088/0305-4608/14/12/025
-
(1984)
J. Phys. F
, vol.14
, pp. 3041
-
-
Small, L.M.1
Heine, V.2
-
28
-
-
0023345567
-
-
10.1016/0304-8853(87)90721-9
-
A. I. Liechtenstein, M. I. Katsnelson, V. P. Antropov, and V. A. Gubanov, J. Magn. Magn. Mater. 67, 65 (1987). 10.1016/0304-8853(87)90721-9
-
(1987)
J. Magn. Magn. Mater.
, vol.67
, pp. 65
-
-
Liechtenstein, A.I.1
Katsnelson, M.I.2
Antropov, V.P.3
Gubanov, V.A.4
-
29
-
-
72849138623
-
-
10.1103/PhysRevLett.103.267202
-
H. L. Meyerheim, J.-M. Tonnerre, L. Sandratskii, H. C. N. Tolentino, M. Przybylski, Y. Gabi, F. Yildiz, X. L. Fu, E. Bontempi, S. Grenier, and J. Kirschner, Phys. Rev. Lett. 103, 267202 (2009). 10.1103/PhysRevLett.103.267202
-
(2009)
Phys. Rev. Lett.
, vol.103
, pp. 267202
-
-
Meyerheim, H.L.1
Tonnerre, J.-M.2
Sandratskii, L.3
Tolentino, H.C.N.4
Przybylski, M.5
Gabi, Y.6
Yildiz, F.7
Fu, X.L.8
Bontempi, E.9
Grenier, S.10
Kirschner, J.11
-
31
-
-
77954820802
-
-
note
-
It is worth noting that the inequivalence of the atomic layers in the film leads to the difference of the distances between different pairs of the neighboring layers. This difference was experimentally detected [see, e.g., earlier experiment (Ref.) on the low energy electron diffraction (LEED) or recent experiment (Ref.) on x-ray diffraction]. A typical value of the variation in the interlayer distance in the internal part of the film is about 1%, whereas for the upper most layer it can be substantially larger. For example, for the 8 ML film the distance of the upper most layer to the next one was detected to increase to 1.88 ± 0.015 Å that is by more than 4% with respect to the Cu interlayer distance. Test calculations with varied interlayer distances have shown that all qualitative conclusions formulated in the paper remain valid. In particular the calculations show that the strong ferromagnetic exchange interactions between two upper Fe layers are determined not by the increased interlayer distance but by the reduced coordination of the Fe atoms of the surface layer.
-
-
-
-
35
-
-
77954832575
-
-
A possible reason for the noncollinearity was suggested to be layer dependence of the magnetic anisotropy. Another reason for the noncollinearity might be competing exchange interactions between different blocks. These interactions are rather weak and depend strongly on the concrete defect pattern in the film.
-
A possible reason for the noncollinearity was suggested to be layer dependence of the magnetic anisotropy. Another reason for the noncollinearity might be competing exchange interactions between different blocks. These interactions are rather weak and depend strongly on the concrete defect pattern in the film.
-
-
-
-
36
-
-
29644446205
-
-
10.1103/PhysRevB.72.140406
-
V. Antropov, Phys. Rev. B 72, 140406 (R) (2005). 10.1103/PhysRevB.72. 140406
-
(2005)
Phys. Rev. B
, vol.72
, pp. 140406
-
-
Antropov, V.1
-
37
-
-
33846786573
-
-
10.1103/PhysRevB.75.054402
-
A. V. Ruban, S. Khmelevskyi, P. Mohn, and B. Johansson, Phys. Rev. B 75, 054402 (2007). 10.1103/PhysRevB.75.054402
-
(2007)
Phys. Rev. B
, vol.75
, pp. 054402
-
-
Ruban, A.V.1
Khmelevskyi, S.2
Mohn, P.3
Johansson, B.4
-
38
-
-
77954819943
-
-
The restriction of our statistical-mechanics calculations to the mean-field approximation leaves open the question if the first-order phase transition is an intrinsic property of the model. The application of a more elaborated statistical-mechanics technique should be carried out to verify if the phase transition predicted by the MFA calculations takes place in this form.
-
The restriction of our statistical-mechanics calculations to the mean-field approximation leaves open the question if the first-order phase transition is an intrinsic property of the model. The application of a more elaborated statistical-mechanics technique should be carried out to verify if the phase transition predicted by the MFA calculations takes place in this form.
-
-
-
-
39
-
-
77954829431
-
-
The small values of the moments of the interface layers of the fcc-Fe/Cu(001) films detected in the recent experiment (Ref.) can be explained by strong Fe-Cu intermixing.
-
The small values of the moments of the interface layers of the fcc-Fe/Cu(001) films detected in the recent experiment (Ref.) can be explained by strong Fe-Cu intermixing.
-
-
-
|