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Scanning Tunneling Microscopy and Spectroscopy (STM/S) Reveals Small Energy Gap of CrBr<sub>3</sub>

ORAL

Abstract

CrBr3 is a 2D van der Waals magnetic material. Despite the great attention on the magnetic properties, the electronic properties of the CrBr3 are relatively unexplored. The energy gap of CrBr3 is believed to be in the range of 1.68-2.1 eV, based on the optical measurements. Density fluctuation theory (DFT) calculations show even higher deviation in the energy gap. These controversies have indicated that the energy gap of CrBr3 is not well studied. Here, we present results from scanning tunneling microscopy and spectroscopy (STM/S) on a defect free surface that is confirmed by atomic resolution topography, having much smaller energy gap (0.57 ± 0.04eV) in thick flake. The multi-peak dI/dV spectrum measured at 77K represents the energies of high density of states (DOS). The energy difference between the conduction band-valance band peak pairs in multi-peak spectrum agrees well with the reported optical transitions further confirming that the measured peaks are intrinsic to CrBr3. DFT calculations with U = 5 eV and J = 3 eV reproduce this energy gap. Finally, the mono- and bi-layer flake shows edge degradation due to ~15 minutes of air exposure during sample transfer. These observations of energy states provide important information towards the fundamental understanding of CrBr3.

Presenters

  • Dinesh Baral

    University of Wyoming

Authors

  • Dinesh Baral

    University of Wyoming

  • Zhuangen Fu

    University of Wyoming

  • Andrei S. Zadorozhnyi

    University of Wyoming

  • Rabindra Dulal

    Physics and Astronomy, University of Wyoming, University of Wyoming

  • Aaron Wang

    University of Wyoming

  • Narendra Shrestha

    University of Wyoming

  • Uppalaiah Erugu

    University of Wyoming

  • Jinke Tang

    University of Wyoming

  • Yuri Dahnovsky

    University of Wyoming

  • Jifa Tian

    Physics and Astronomy, University of Wyoming, University of Wyoming

  • Te-Yu Chien

    Physics and Astronomy, University of Wyoming, University of Wyoming