Home Browse Search Subscriptions Help
Volume: Page/Article:

Article Collection: View Collection  Help (Click on the Check Box to add an article.)

Phys. Rev. Lett. 78, 1154–1157 (1997)

[Issue 6 – 10 February 1997 ]

Previous article | Next article | Issue 6 contents ]

Add to article collection View PDF (136 kB)


k-Space Origin of the Long-Period Oscillation in Fe/Cr Multilayers: A Photoemission Study of Epitaxial Cr Grown on an Fe(100) Whisker

Dongqi Li, J. Pearson, and S. D. Bader
Materials Science Division, Argonne National Laboratory, Argonne, Illinois 60439
E. Vescovo1, D.-J. Huang2, and P. D. Johnson2
1National Synchrotron Light Source, Brookhaven National Laboratory, Upton, New York 11973
2Physics Department, Brookhaven National Laboratory, Upton, New York 11973
B. Heinrich
Physics Department, Simon Fraser University, Burnaby, British Columbia V5A 1S6, Canada
Received 22 February 1996

The k-space origin of the long-period (18 Å) oscillation in the interlayer magnetic coupling of Fe/Cr(100) multilayers is investigated by means of angle-resolved photoemission by probing quantum well (QW) states at the Fermi energy for epitaxial Cr grown on an Fe(100) whisker at 300 °C. The periodicity of the intensity oscillations of the Cr QW states in the vicinity of the d-derived "lens" feature of the Fermi surface is 17±2 Å. Thus the lens is identified as a prime candidate for the origin of the long period.

©1997 The American Physical Society

URL: http://link.aps.org/abstract/PRL/v78/p1154
DOI: 10.1103/PhysRevLett.78.1154
PACS: 75.70.Cn, 73.20.Dx, 79.60.Bm


Add to article collection View PDF (136 kB)

Previous article | Next article | Issue 6 contents ]


References

(Reference links marked with dot may require a separate subscription.)
  1. J. E. Ortega and F. J. Himpsel, Phys. Rev. Lett. 69, 844 (1992).
  2. P. Bruno, J. Magn. Magn. Mater. 121, 248 (1993).[dot INSPEC]
  3. D. M. Edwards et al., Phys. Rev. Lett. 67, 493 (1991).
  4. J. E. Ortega et al., Phys. Rev. B 47, 1540 (1993).
  5. N. B. Brookes, Y. Chang, and P. D. Johnson, Phys. Rev. Lett. 67, 354 (1991).
  6. K. Garrison, Y. Chang, and P. D. Johnson, Phys. Rev. Lett. 71, 2801 (1993).
  7. C. Carbone et al., Phys. Rev. Lett. 71, 2805 (1993).
  8. N. V. Smith et al., Phys. Rev. B 49, 332 (1994).
  9. P. Bruno, Phys. Rev. B 52, 411 (1995).
  10. M. D. Stiles, Phys. Rev. B 48, 7238–7258 (1993).
  11. M. van Schilfgaarde and W. A. Harrison, Phys. Rev. Lett. 71, 3870 (1993).
  12. S. Mirbt et al., Phys. Rev. B 54, 6382 (1996).
  13. M. Stiles, Phys. Rev. B (to be published).
  14. P. D. Johnson et al., Phys. Rev. B 50, 8954 (1994).
  15. D. D. Koelling, Phys. Rev. B 50, 273 (1994).
  16. J. Unguris, R. J. Celotta, and D. T. Pierce, Phys. Rev. Lett. 67, 140 (1991).
  17. B. Heinrich et al., J. Appl. Phys. 79, 4518 (1996).[dot SPIN][dot INSPEC]
  18. L. E. Klebanoff et al., Phys. Rev. B 32, 1997 (1985).
  19. D. G. Laurent et al., Phys. Rev. B 23, 4977 (1981).
  20. S. S. P. Parkin, N. More, and K. P. Roche, Phys. Rev. Lett. 64, 2304 (1990).
  21. J. Unguris, R. J. Celotta, and D. T. Pierce, Phys. Rev. Lett. 69, 1125 (1992).
  22. E. E. Fullerton et al., Phys. Rev. B 48, 15 755 (1993).


Add to article collection View PDF (136 kB)

[Show Articles Citing This One] Requires Subscription

Previous article | Next article | Issue 6 contents ]

Home  | Browse  | Search  | Subscriptions  | Help  ]

E-mail: prola@aps.org