Local model Hamiltonian calculation of RIXS amplitudes of Sr3NiIrO6

Show full item record



Permalink

http://urn.fi/URN:NBN:fi:hulib-201911073872
Title: Local model Hamiltonian calculation of RIXS amplitudes of Sr3NiIrO6
Author: Keller, Levi
Contributor: University of Helsinki, Faculty of Science
Publisher: Helsingin yliopisto
Date: 2019
Language: eng
URI: http://urn.fi/URN:NBN:fi:hulib-201911073872
http://hdl.handle.net/10138/307311
Thesis level: master's thesis
Degree program: Materiaalitutkimuksen maisteriohjelma
Master's Programme in Materials Research
Magisterprogrammet i materialforskning
Specialisation: Fysiikka
Physics
Fysik
Discipline: none
Abstract: The spin-orbit-coupled insulator Sr 3 NiIrO 6 is a strongly correlated transition metal compound, where an interplay of geometric frustration and spin anisotropy gives rise to novel magnetic phases. Resonant inelastic x-ray scattering (RIXS) is a powerful probe of the low-lying quasi-particle excitations that underpin these emergent properties. In this work, we partition the active space into approximately non-interacting parts in order to introduce a tight-binding single-particle model Hamiltonian describing the distorted IrO6 octahedra in Sr3NiIrO6. We then use this model to calculate its RIXS spectrum at the Ir L3-edge in the sub-electronvolt range. The results of this calculation are compared with experiments performed at the European Synchrotron Radiation Facility, and with a multiplet crystal field model calculation. We find that this one electron model largely agrees with the full-multiplet model and describes the d-d excitations observed in experiment. The addition of an exchange field term explains the low-lying temperature-dependent magnetic feature, disambiguating the sign of the crystal-field term, and suggesting that the feature is well localized at low temperatures, and is best described as an orbitally- entangled local spin-flip excitation. However, the correspondence at room temperature diminishes, suggesting that dispersive description is necessary to model this regime. The drastic reduction in active space entailed by this model facilitates the creation of extended non-collinear Heisenberg-like models, which can be calculated at a lower computational cost than full multiplet extended models.
Subject: Synchotron
Spectroscopy
Resonant Inelastic X-ray Scattering
model Hamiltonian
Spin-orbit coupling
Crystal Field


Files in this item

Total number of downloads: Loading...

Files Size Format View
main.pdf 2.100Mb PDF View/Open

This item appears in the following Collection(s)

Show full item record