Strain control of a bandwidth-driven spin reorientation in Ca3Ru2O7
Overview & Synopsis
Abstract The layered-ruthenate family of materials possess an intricate interplay of structural, electronic and magnetic degrees of freedom that yields a plethora of delicately balanced ground states. This is exemplified by Ca 3 Ru 2 O 7 , which hosts a coupled transition in which the lattice parameters jump, the Fermi surface partially gaps and the spins undergo a 90 ∘ in-plane reorientation. Here, we show how the transition is driven by a lattice strain that tunes the electronic bandwidth. We apply uniaxial stress to single crystals of Ca 3 Ru 2 O 7 , using neutron and resonant x-ray scattering to simultaneously probe the structural and magnetic responses. These measurements demonstrate that the transition can be driven by externally induced strain, stimulating the development of a theoretical model in which an internal strain is generated self-consistently to lower the electronic energy. We understand the strain to act by modifying tilts and rotations of the RuO 6 octahedra, which directly influences the nearest-neighbour hopping. Our results offer a blueprint for uncovering the driving force behind coupled phase transitions, as well as a route to controlling them.
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Document Information
| Document Title | Strain control of a bandwidth-driven spin reorientation in Ca3Ru2O7 |
|---|---|
| Author / Organization | C D Dashwood, A H Walker, M P Kwasigroch, L S I Veiga, Q. Faure, J G Vale, D G Porter, P. Manuel, D D Khalyavin, F. Orlandi, C V Colin, O. Fabelo, F. Krüger, R S Perry, R D Johnson, A G Green, D F Mcmorrow |
| Subject & Discipline | Multidisciplinary Academic Open Research |
| Categories | Science & Mathematics |
| Publication Year | 2023 |
| License / Rights | Open Access / Creative Commons |
| Resource Verification | Listed PDF (Verification Pending) |
| Original Host Website |
HAL Open Science
(hal.science)
|
| File Format | application/pdf (Portable Document Format) |
| Language | EN |
| Catalog ID | DOC-222576 |
| Original Source Link | Visit Source Page on hal.science » |