V. Smelyansky, A. Perlov, V. Antonov
Nov 26, 1990
Journal of Physics: Condensed Matter
On the basis of fully relativistic self-consistent band structure calculations a model of the Fermi surface of Os is suggested. The angular dependence of the extremal cross-section areas has been determined and found to be in good agreement with experimental data. Two additional groups of DHVA oscillations in the region of 200 MG associated with the large orbits on a hole 'monster' are predicted.