Abstract
By using the de Haas-van Alphen (dHvA) effect, g factors have been determined in antimony for most carrier branches in the trigonal-bisectrix and binary-bisectrix planes. The use of magnetic fields to 11.8 T, low-level field modulation, and annealed samples allowed accurate determination of the relative spin splitting by direct observation of the dHvA wave shape. Infinite-field phase extrapolations show that g factors are much lower than previously reported. This is shown to be in agreement with theoretical expectations for these g factors.

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