Hole Fermi surface in Bi2Se3 probed by quantum oscillations

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Abstract

Transport and torque magnetometry measurements are performed at high magnetic fields and low temperatures in a series of p-type (Ca-doped) Bi2Se3 crystals. The angular dependence of the Shubnikov-de Haas and de Haas-van Alphen quantum oscillations enables us to determine the Fermi surface of the bulk valence band states as a function of the carrier density. At low density, the angular dependence exhibits a downturn in the oscillations frequency between 0 and 90, reflecting a bag-shaped hole Fermi surface. The detection of a single frequency for all tilt angles rules out the existence of a Fermi surface with different extremal cross sections down to 24 meV. There is therefore no signature of a camelback in the valence band of our bulk samples, in accordance with the direct band gap predicted by GW calculations.

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Piot, B. A., Desrat, W., Maude, D. K., Orlita, M., Potemski, M., Martinez, G., & Hor, Y. S. (2016). Hole Fermi surface in Bi2Se3 probed by quantum oscillations. Physical Review B, 93(15). https://doi.org/10.1103/PhysRevB.93.155206

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