-
1
-
-
0035900398
-
-
0036-8075
-
S. A. Wolf, D. D. Awschalom, R. A. Buhrman, J. M. Daughton, S. von Molnar, M. L. Roukes, A. Y. Chtchelkanova, and D. M. Treger, Science 0036-8075 294, 1488 (2001).
-
(2001)
Science
, vol.294
, pp. 1488
-
-
Wolf, S.A.1
Awschalom, D.D.2
Buhrman, R.A.3
Daughton, J.M.4
Von Molnar, S.5
Roukes, M.L.6
Chtchelkanova, A.Y.7
Treger, D.M.8
-
2
-
-
10044225881
-
-
1476-1122 10.1038/nmat1256
-
S. S. Parkin, C. Kaiser, A. Panchula, P. Rice, B. Hughes, M. Sammat, and S.-H. Yang, Nat. Mater. 1476-1122 10.1038/nmat1256 3, 862 (2004).
-
(2004)
Nat. Mater.
, vol.3
, pp. 862
-
-
Parkin, S.S.1
Kaiser, C.2
Panchula, A.3
Rice, P.4
Hughes, B.5
Sammat, M.6
Yang, S.-H.7
-
3
-
-
34547626151
-
-
0031-9007 10.1103/PhysRevLett.50.2024
-
R. de Groot, F. Mueller, P. van Engen, and K. Buschow, Phys. Rev. Lett. 0031-9007 10.1103/PhysRevLett.50.2024 50, 2024 (1983).
-
(1983)
Phys. Rev. Lett.
, vol.50
, pp. 2024
-
-
De Groot, R.1
Mueller, F.2
Van Engen, P.3
Buschow, K.4
-
4
-
-
0032472150
-
-
0921-4526 10.1016/S0921-4526(97)00495-X
-
S. Ishida, T. Masaki, S. Fujii, and S. Asano, Physica B: Condensed Matter 0921-4526 10.1016/S0921-4526(97)00495-X 245, 1 (1998).
-
(1998)
Physica B
, vol.245
, pp. 1
-
-
Ishida, S.1
Masaki, T.2
Fujii, S.3
Asano, S.4
-
5
-
-
2142824428
-
-
0021-8979 10.1063/1.1556249
-
S. Kämmerer, S. Heitmann, D. Meyners, D. Sudfeld, A. Thomas, A. Hütten, and G. Reiss, J. Appl. Phys. 0021-8979 10.1063/1.1556249 93, 7945 (2003).
-
(2003)
J. Appl. Phys.
, vol.93
, pp. 7945
-
-
Kämmerer, S.1
Heitmann, S.2
Meyners, D.3
Sudfeld, D.4
Thomas, A.5
Hütten, A.6
Reiss, G.7
-
6
-
-
37649030879
-
-
0163-1829 10.1103/PhysRevB.70.024426
-
J. Schmalhorst, S. Kämmerer, M. Sacher, G. Reiss, A. Hütten, and A. Scholl, Phys. Rev. B 0163-1829 10.1103/PhysRevB.70.024426 70, 024426 (2004).
-
(2004)
Phys. Rev. B
, vol.70
, pp. 024426
-
-
Schmalhorst, J.1
Kämmerer, S.2
Sacher, M.3
Reiss, G.4
Hütten, A.5
Scholl, A.6
-
7
-
-
18644374382
-
-
0003-6951 10.1063/1.1853526
-
J. Schmalhorst, S. Kämmerer, G. Reiss, and A. Hütten, Appl. Phys. Lett. 0003-6951 10.1063/1.1853526 86, 052501 (2005).
-
(2005)
Appl. Phys. Lett.
, vol.86
, pp. 052501
-
-
Schmalhorst, J.1
Kämmerer, S.2
Reiss, G.3
Hütten, A.4
-
8
-
-
28744435193
-
-
0163-1829 10.1103/PhysRevB.71.144416
-
W. H. Wang, Phys. Rev. B 0163-1829 10.1103/PhysRevB.71.144416 71, 144416 (2005).
-
(2005)
Phys. Rev. B
, vol.71
, pp. 144416
-
-
Wang, W.H.1
-
9
-
-
3242679924
-
-
0003-6951 10.1063/1.1769082
-
S. Kämmerer, A. Thomas, A. Hütten, and G. Reiss, Appl. Phys. Lett. 0003-6951 10.1063/1.1769082 85, 79 (2004).
-
(2004)
Appl. Phys. Lett.
, vol.85
, pp. 79
-
-
Kämmerer, S.1
Thomas, A.2
Hütten, A.3
Reiss, G.4
-
11
-
-
0000511944
-
-
0168-9002 10.1016/0168-9002(94)91869-4
-
Y. U. Idzerda, C. T. Chen, H. -J. Lin, G. Meigs, G. H. Ho, and C. -C. Kao, Nucl. Instrum. Methods Phys. Res. A 0168-9002 10.1016/0168-9002(94)91869-4 347, 134 (1994).
-
(1994)
Nucl. Instrum. Methods Phys. Res. A
, vol.347
, pp. 134
-
-
Idzerda, Y.U.1
Chen, C.T.2
Lin, H.-J.3
Meigs, G.4
Ho, G.H.5
Kao, C.-C.6
-
12
-
-
33845783732
-
-
The comparison of FY and TEY data of 4 and 100 nm thick Co2 MnSi films and transmission data of 20 nm thick films (unpublished results) showed that the probability for the fluorescence decay is larger for holes in the 2 p12 shell than for holes in the 2 p32 shell. The higher FY signal at the Mn L2 edge compared with the Mn L3 edge results from the stronger saturation effect at the L3 edge and the larger fluorescence probability at the L2 edge.
-
The comparison of FY and TEY data of 4 and 100 nm thick Co2 MnSi films and transmission data of 20 nm thick films (unpublished results) showed that the probability for the fluorescence decay is larger for holes in the 2 p12 shell than for holes in the 2 p32 shell. The higher FY signal at the Mn L2 edge compared with the Mn L3 edge results from the stronger saturation effect at the L3 edge and the larger fluorescence probability at the L2 edge.
-
-
-
-
13
-
-
33845799580
-
-
edited by H.Ebert
-
The Munich SPR-KKR package, version 2.1.3, edited by, H. Ebert, http://olymp.cup.uni-muenchen.de/ak/ebert/SPRKKR; H. Ebert, in Electronic Structure and Physical Properties of Solids, Lecture Notes in Physics, Vol. 535, edited by, H. Dreysse, (Springer, Berlin, 2000), p. 191.
-
-
-
-
14
-
-
0000561702
-
-
Lecture Notes in Physics, Vol. edited by H.Dreysse (Springer, Berlin
-
The Munich SPR-KKR package, version 2.1.3, edited by, H. Ebert, http://olymp.cup.uni-muenchen.de/ak/ebert/SPRKKR; H. Ebert, in Electronic Structure and Physical Properties of Solids, Lecture Notes in Physics, Vol. 535, edited by, H. Dreysse, (Springer, Berlin, 2000), p. 191.
-
(2000)
Electronic Structure and Physical Properties of Solids
, vol.535
, pp. 191
-
-
Ebert, H.1
-
15
-
-
3342975547
-
-
0031-9007 10.1103/PhysRevLett.75.152
-
C. T. Chen, Y. U. Idzerda, H.-J. Lin, N. V. Smith, G. Meigs, E. Chaban, G. H. Ho, E. Pellegrin, and F. Sette, Phys. Rev. Lett. 0031-9007 10.1103/PhysRevLett.75.152 75, 152 (1995).
-
(1995)
Phys. Rev. Lett.
, vol.75
, pp. 152
-
-
Chen, C.T.1
Idzerda, Y.U.2
Lin, H.-J.3
Smith, N.V.4
Meigs, G.5
Chaban, E.6
Ho, G.H.7
Pellegrin, E.8
Sette, F.9
-
16
-
-
33845727474
-
-
To correct the jj mixing for Mn18 its spin moment ms had be multiplied by the factor . The value of is not precisely known, but lies in the range from 1.0 (Ref. 19) to 1.5 (Ref. 18). This resulted in the large uncertainty for mMn mCo.
-
To correct the jj mixing for Mn18 its spin moment ms had be multiplied by the factor. The value of is not precisely known, but lies in the range from 1.0 (Ref.) to 1.5 (Ref.). This resulted in the large uncertainty for mMn mCo.
-
-
-
-
18
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-
33845744768
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XAS in transmission (unpublished results) showed, that the x-ray attenuation lengths at the intensity maxima of the Co and Mn L2 edges are nearly the same, because the higher number of Mn 3d holes compared with the number of Co 3d holes is compensated by the larger Co concentration in the Co2 MnSi film.
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XAS in transmission (unpublished results) showed, that the x-ray attenuation lengths at the intensity maxima of the Co and Mn L2 edges are nearly the same, because the higher number of Mn 3d holes compared with the number of Co 3d holes is compensated by the larger Co concentration in the Co2 MnSi film.
-
-
-
-
19
-
-
0001402740
-
-
0163-1829 10.1103/PhysRevB.63.214406
-
Y. Yonamoto, T. Yokoyama, K. Amemiya, D. Matsumura, and T. Ohta, Phys. Rev. B 0163-1829 10.1103/PhysRevB.63.214406 63, 214406 (2001).
-
(2001)
Phys. Rev. B
, vol.63
, pp. 214406
-
-
Yonamoto, Y.1
Yokoyama, T.2
Amemiya, K.3
Matsumura, D.4
Ohta, T.5
-
20
-
-
33845728467
-
-
E. Göring (private communication).
-
-
-
Göring, E.1
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