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Civale, L.1
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Krusin-Elbaum, L.6
Sun, Y.7
Clem, J.8
Holtzberg, F.9
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M. Konczykowski, F. Rullier-Albenque, E.R. Jacoby, A. Shaulov, Y. Yeshurun and P. Lejay, Phys. Rev. B 44, 7167 (1991).
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Lejay, P.6
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12044251389
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For a review, see, G. Blatter, M.V. Feigel'man, V.B. Geshkenbein, A.I. Larkin and V.M. Vinokur, Rev. Mod. Phys. 66, 1125 (1994).
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Blatter, G.1
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Geshkenbein, V.3
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Vinokur, V.5
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L. Krusin-Elbaum, L. Civale, G. Blatter, A.D. Marwick, F. Holtzberg and C. Feild, Phys. Rev. Lett. 72, 1914 (1994).
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Blatter, G.3
Marwick, A.4
Holtzberg, F.5
Feild, C.6
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0000763617
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our case, for (Formula presented)(5 K)∼7×(Formula presented) A/(Formula presented) and t∼20fμm, the characteristic field for a thin sample is (Formula presented)=(Formula presented)t/2≃0.7 T. Thus, with the maximum H=5.5 T, the deviations from the conventional Bean model are insignificant
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J.R. Clem and A. Sanchez, Phys. Rev. B 50, 9355 (1994); in our case, for (Formula presented)(5 K)∼7×(Formula presented) A/(Formula presented) and t∼20fμm, the characteristic field for a thin sample is (Formula presented)=(Formula presented)t/2≃0.7 T. Thus, with the maximum H=5.5 T, the deviations from the conventional Bean model are insignificant.
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Phys. Rev. B
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, pp. 9355
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Clem, J.1
Sanchez, A.2
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0000983340
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L. Civale, L. Krusin-Elbaum, J.R. Thompson and F. Holtzberg, Phys. Rev. B 50, 7188 (1994).
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Phys. Rev. B
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Krusin-Elbaum, L.2
Thompson, J.3
Holtzberg, F.4
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25944460472
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L. Civale, L. Krusin-Elbaum, J.R. Thompson, R. Wheeler, A.D. Marwick, M.A. Kirk, Y. Sun, F. Holtzberg and C. Feild, Phys. Rev. B 50, 4102 (1994);J.R. Thompson, L. Krusin-Elbaum, and L. Civale (unpublished).
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Civale, L.1
Krusin-Elbaum, L.2
Thompson, J.3
Wheeler, R.4
Marwick, A.5
Kirk, M.6
Sun, Y.7
Holtzberg, F.8
Feild, C.9
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16
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85037904640
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L. Civale, G. Pasquini, P. Levy, G. Nieva, D. Casa, and H. Lanza, Physica C (to be published).
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Civale, L.1
Pasquini, G.2
Levy, P.3
Nieva, G.4
Casa, D.5
Lanza, H.6
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