paper

Orbital transmutation and the electronic spectrum of FeSe in the nematic phase

arXiv:1908.04889 · doi:10.1103/PhysRevResearch.2.013015

Abstract

We consider the electronic spectrum near in the nematic phase of FeSe () and make a detailed comparison with recent ARPES and STM experiments. Our main focus is the unexpected temperature dependence of the excitations at the point. These have been identified as having and orbital character well below , but remain split at , in apparent contradiction to the fact that in the tetragonal phase the and orbitals are degenerate. Here we present two scenarios which can describe the data. In both scenarios, hybridization terms present in the tetragonal phase leads to an orbital transmutation, a change in the dominant orbital character of some of the bands, between and . The first scenario relies on the spin-orbit coupling at the point. We show that a finite spin-orbit coupling gives rise to orbital transmutation, in which one of the modes, identified as ( at , becomes predominantly at and hence does not merge with the predominantly () mode. The second scenario, complementary to the first, takes into consideration the fact that both ARPES and STM are surface probes. In the bulk, a direct hybridization between the and orbitals is not allowed at the point, however, it is permitted on the surface. In the presence of a direct hybridization, the orbital character of the modes changes from pure and pure at to at , i.e., the two modes again have mono-orbital character at low , but do not merge at . We discuss how these scenarios can be distinguished in polarized ARPES experiments.

12 + epsilon pages, 13 figures

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