-
1
-
-
0026188590
-
-
431 (1991).
-
D. H. Kim, K. E. Gray, R. T. Kampwirth, J. C. Smith, D. S. Richeson, T. J. Marks, J. H. Kang, J. Talvacchio and M. Eddy, Physica C177, 431 (1991).
-
K. E. Gray, R. T. Kampwirth, J. C. Smith, D. S. Richeson, T. J. Marks, J. H. Kang, J. Talvacchio and M. Eddy, Physica C177
-
-
Kim, D.H.1
-
3
-
-
0041595201
-
-
7737 (1991).
-
C. Duran, J. Yazyi, F. de la Cruz, D. J. Bishop, D. B. Mitzi and A. Kapitulnik, Phys. Rev. B44, 7737 (1991).
-
J. Yazyi, F. De La Cruz, D. J. Bishop, D. B. Mitzi and A. Kapitulnik, Phys. Rev. B44
-
-
Duran, C.1
-
4
-
-
0004770917
-
-
67, 648 (1991).
-
L. Civale, A. D. Marwick, T. K. Worthington, M. A. Kirk, J. R. Thompson, L. Krusin-Elbaum, Y. Sun, J. R. Clem and F. H. Holtzberg, Phys. Rev. Lett. 67, 648 (1991).
-
A. D. Marwick, T. K. Worthington, M. A. Kirk, J. R. Thompson, L. Krusin-Elbaum, Y. Sun, J. R. Clem and F. H. Holtzberg, Phys. Rev. Lett.
-
-
Civale, L.1
-
5
-
-
36449007811
-
-
60, 2306 (1992); W. Gerhäuser, G. Ries, H. W. Neumüller, W. Schmidt, O. Eibl, G. Saemann-Ischenko and S. Klaumünzer, Phys. Rev. Lett. 68, 879 (1992).
-
J. R. Thompson, Y. R. Sun, H. R. Kerchner, D. K. Christen, B. C. Sales, B. C. Chakoumakos, A. D. Marwick, L. Civale and J. O. Thomson, Appl. Phys. Lett. 60, 2306 (1992); W. Gerhäuser, G. Ries, H. W. Neumüller, W. Schmidt, O. Eibl, G. Saemann-Ischenko and S. Klaumünzer, Phys. Rev. Lett. 68, 879 (1992).
-
Y. R. Sun, H. R. Kerchner, D. K. Christen, B. C. Sales, B. C. Chakoumakos, A. D. Marwick, L. Civale and J. O. Thomson, Appl. Phys. Lett.
-
-
Thompson, J.R.1
-
6
-
-
33646662069
-
-
3523 (1993); and Physica A200, 413 (1993).
-
L. Klein, E. R. Yacoby, Y. Yeshurun, M. Konczykowski and K. Kishio, Phys. Rev. B48, 3523 (1993); and Physica A200, 413 (1993).
-
E. R. Yacoby, Y. Yeshurun, M. Konczykowski and K. Kishio, Phys. Rev. B48
-
-
Klein, L.1
-
10
-
-
33747765410
-
-
This Suggestion stems from the reasonable expectation of significant film strain caused by the deposited heavy ions expanding the substrate.
-
This Suggestion stems from the reasonable expectation of significant film strain caused by the deposited heavy ions expanding the substrate.
-
-
-
-
12
-
-
33747792921
-
-
0000 (August 1, 1996).
-
K. E. Gray, J. D. Hettinger, D. J. Miller, B. R. Washburn C. Moreau, C. Lee, B. G. Glagola and M. M. Eddy, Phys. Rev. B54, 0000 (August 1, 1996).
-
-
-
-
13
-
-
34547566407
-
-
36, 39 (1964).
-
The force is perhaps more correctly thought of as the magnetic pressure due to the flux gradient caused by the transport current density, see P. W. Anderson and Y. B. Kim, Rev. Mod. Phys. 36, 39 (1964).
-
Rev. Mod. Phys.
-
-
Anderson, P.W.1
Kim, Y.B.2
-
14
-
-
0345495344
-
-
72, 1750 (1994)
-
S. Behler, S. H. Pan, P. Jess, A. Baratoff, H. J. Güntherodt, F. Levy, G. Wirth and J. Wiesner, Phys. Rev. Lett. 72, 1750 (1994)
-
S. H. Pan, P. Jess, A. Baratoff, H. J. Güntherodt, F. Levy, G. Wirth and J. Wiesner, Phys. Rev. Lett.
-
-
Behler, S.1
|