Quantum-well or bulklike behaviour of Cu layers on Co

Journal of Physics Condensed Matter

Volumn 9, Issue 32, 1997, Pages

  Hansen, E D ^a   Miller, T ^a   Chiang, T C ^a  

^a NONE

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0342266050     PISSN: 09538984     EISSN: None     Source Type: Journal    
DOI: 10.1088/0953-8984/9/32/001     Document Type: Article

References (29)

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12. The observed magnetic oscillation in Cu-Co(111) is weak, if nonzero. It is controversial whether or not the sometimes observed effect is caused by sample imperfection (inclusion of crystallites of other orientations). See, for example. Pollard R J, Wilson M J and Grundy P J 1995 J. Magn. Magn. Mater. 151 139 Ives A J R et al 1994 J. Appl. Phys. 75 6458 Schreyer A et al 1993 Phys. Rev. B 47 15334 Egelhoff W F Jr and Kief M T 1992 Phys. Rev. B 45 7795
13. The observed magnetic oscillation in Cu-Co(111) is weak, if nonzero. It is controversial whether or not the sometimes observed effect is caused by sample imperfection (inclusion of crystallites of other orientations). See, for example. Pollard R J, Wilson M J and Grundy P J 1995 J. Magn. Magn. Mater. 151 139 Ives A J R et al 1994 J. Appl. Phys. 75 6458 Schreyer A et al 1993 Phys. Rev. B 47 15334 Egelhoff W F Jr and Kief M T 1992 Phys. Rev. B 45 7795
14. The observed magnetic oscillation in Cu-Co(111) is weak, if nonzero. It is controversial whether or not the sometimes observed effect is caused by sample imperfection (inclusion of crystallites of other orientations). See, for example. Pollard R J, Wilson M J and Grundy P J 1995 J. Magn. Magn. Mater. 151 139 Ives A J R et al 1994 J. Appl. Phys. 75 6458 Schreyer A et al 1993 Phys. Rev. B 47 15334 Egelhoff W F Jr and Kief M T 1992 Phys. Rev. B 45 7795
15. The observed magnetic oscillation in Cu-Co(111) is weak, if nonzero. It is controversial whether or not the sometimes observed effect is caused by sample imperfection (inclusion of crystallites of other orientations). See, for example. Pollard R J, Wilson M J and Grundy P J 1995 J. Magn. Magn. Mater. 151 139 Ives A J R et al 1994 J. Appl. Phys. 75 6458 Schreyer A et al 1993 Phys. Rev. B 47 15334 Egelhoff W F Jr and Kief M T 1992 Phys. Rev. B 45 7795
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19. It is well known that thin Co films grow as fee crystals on Cu(100) and Cu(110). The growth on Cu(111) is mixed fcc and hep. The fee notation is used here for simplicity.
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22. The band structures of hcp Co(0001) and fee Co(111) are the same along the surface normal. See Himpsel F J and Eastman D E 1980 Phys. Rev. B 21 3207 Jarlborg T and Peter M 1984 J. Magn. Magn. Mater. 42 89 Papaconstantopolous D A 1986 Handbook of the Band Structure of Elemental Solids (New York: Plenum)
23. The band structures of hcp Co(0001) and fee Co(111) are the same along the surface normal. See Himpsel F J and Eastman D E 1980 Phys. Rev. B 21 3207 Jarlborg T and Peter M 1984 J. Magn. Magn. Mater. 42 89 Papaconstantopolous D A 1986 Handbook of the Band Structure of Elemental Solids (New York: Plenum)
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