Bulletin of the American Physical Society
APS March Meeting 2022
Volume 67, Number 3
Monday–Friday, March 14–18, 2022; Chicago
Session A70: Ruthenates and 4D Systems
8:00 AM–10:36 AM,
Monday, March 14, 2022
Room: Hyatt Regency Hotel -Jackson Park B
Sponsoring
Units:
DMP DCMP
Chair: Jennifer Fowlie, Stanford University
Abstract: A70.00001 : Low-energy orbital texture of Ca2RuO4 and Ca3Ru2O7
8:00 AM–8:36 AM
Presenter:
Karin von Arx
(University of Zurich, Chalmers University of Technology)
Authors:
Karin von Arx
(University of Zurich, Chalmers University of Technology)
Filomena Forte
(CNR-SPIN)
Mario Cuoco
(CNR-SPIN)
Masafumi Horio
(University of Tokyo)
Veronica Granata
(University of Salerno)
Qisi Wang
(University of Zurich)
Lakshmi Das
(University of Zurich)
Yasmine Sassa
(Chalmers University of Technology)
Rosalba Fittipaldi
(CNR-SPIN)
Claudia G Fatuzzo
(Ecole Polytechnique Fedérale de Lausanne)
Oleh Ivashko
(Deutsches Elektronen-Synchrotron DESY)
Antonio Vecchione
(CNR-SPIN)
Thorsten Schmitt
(Paul Scherrer Institut)
Johan Chang
(University of Zurich)
On this background, a wide scientific interest has been put towards the Ruddlesden-Popper type ruthenates (Sr, Ca)n+1RunO3n+1, which show a very rich variety of exotic ground states including superconductivity and Mott physics [1-3]. This talk presents combined oxygen K-edge x-ray absorption and resonant inelastic x-ray scattering studies of the single layer Ca2RuO4 and the bilayered Ca3Ru2O7 [4-5]. Excitations of ruthenium d orbitals were accessed indirectly through their hybridization with oxygen p orbitals. With this method, it is possible to investigate the low-lying electronic structure site and orbital specific for these closely related compounds. Whereas Ca2RuO4 is an antiferromagnetic band-Mott insulator at low temperature, the ground state of Ca3Ru2O7 exhibits in-plane ferromagnetic order and a metallic behaviour. This direct comparison of the low-lying spin-orbital excitations demonstrates remarkable differences. Furthermore, the experimentally observed dispersion of excitations allows their interpretation as spin-orbital quasiparticle branches.
[1] Fatuzzo et al., PRB 91, 155104 (2015)
[2] Das, L. et al., PRX 8, 011048 (2018)
[3] Gretarsson et al., PRB 100, 045123 (2019)
[4] von Arx et al., PRB 102, 235194 (2020)
[5] von Arx et al., in preparation
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