Orbital- and k<sub>z</sub>-selective hybridisation of Se 4p and Ti 3d states at the CDW transition of TiSe<sub>2</sub>

ORAL

Abstract

We revisit the enduring problem of the 2×2×2 charge density wave (CDW) order in TiSe2, utilising photon energy-dependent angle-resolved photoemission spectroscopy (ARPES) to probe the full three-dimensional high- and low-temperature electronic structure. Our measurements demonstrate how a mismatch of dimensionality between the 3D conduction bands and the quasi-2D valence bands in this system leads to a hybridisation that is strongly kz-dependent. This 3D momentum-selective coupling shifts the strongly hybridized states well away from the Fermi level, providing the energy gain required to form the CDW. However, we show how additional ``passenger'' states remain, and dominate the low energy physics in the ordered state. In particular we find that a branch of the conduction band with 3dz2 character remains essentially unhybridised in the ordered phase, forming a coherent and ungapped electron-like Fermi surface. We conclude by making a comparison to the 2x2 CDW of monolayer TiSe2, where kz-selective effects are absent, but orbital-selective hybridisation persists. [1] Watson et al., arXiv:1808.07141 (2018).

*We gratefully acknowledge support from The Leverhulme Trust (Grant Nos. RL-2016-006 and PLP-2015-144) and The Royal Society.

Presenters

  • Matthew Watson

    • University of St Andrews
    • School of Physics and Astronomy, University of St. Andrews
    • Diamond Light Source
    • School of Physics and Astronomy, University of St Andrews, St. Andrews KY16 9SS, United Kingdom

Authors

  • Matthew Watson

    • University of St Andrews
    • School of Physics and Astronomy, University of St. Andrews
    • Diamond Light Source
    • School of Physics and Astronomy, University of St Andrews, St. Andrews KY16 9SS, United Kingdom
  • Oliver J Clark

    • University of St Andrews
    • School of Physics and Astronomy, University of St Andrews, St. Andrews KY16 9SS, United Kingdom
  • Federico Mazzola

    • University of St Andrews
    • School of Physics and Astronomy, University of St Andrews, St. Andrews KY16 9SS, United Kingdom
  • Igor Marković

    • University of St Andrews
    • School of Physics and Astronomy, University of St Andrews, UK
    • School of Physics and Astronomy, University of St Andrews, St. Andrews KY16 9SS, United Kingdom
  • Veronika Sunko

    • Max Planck Institute for Chemical Physics of Solids
    • School of Physics and Astronomy, University of St Andrews, St. Andrews KY16 9SS, United Kingdom
  • Timur Kim

    • Diamond Light Source
    • Diamond Light Source, Harwell Campus, Didcot, OX11 0DE, United Kingdom
  • Kai Rossnagel

    • Kiel University
    • Institute of Experimental and Applied Physics, Kiel University
    • Institut für Experimentelle und Angewandte Physik, Christian-Albrechts-Universität zu Kiel, 24098 Kiel, Germany
  • Philip King

    • University of St Andrews
    • School of Physics and Astronomy, University of St Andrews, St. Andrews KY16 9SS, United Kingdom