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Structure and magnetic properties of epitaxial CaFe2O4 thin films
Silvia Damerio, Pavan Nukala, Jean Juraszek, Pim Reith, Hans Hilgenkamp, Beatriz Noheda

Structure and magnetic properties of epitaxial CaFe2O4 thin films

Science & Mathematics Published 2020 Verification Pending

Overview & Synopsis

CaFe 2 O 4 is a highly anisotropic antiferromagnet reported to display two spin arrangements with up-up-down-down (phase A) and up-down-up-down (phase B) configurations. The relative stability of these phases is ruled by the competing ferromagnetic and antiferromagnetic interactions between Fe 3+ spins arranged in two different environments, but a complete understanding of the magnetic structure of this material does not exist yet. In this study, we investigate epitaxial CaFe 2 O 4 thin films grown on TiO 2 (110) substrates by means of pulsed laser deposition (PLD). Structural characterization reveals the coexistence of two out-of-plane crystal orientations and the formation of three in-plane oriented domains. The magnetic properties of the films, investigated macroscopically as well as locally, including highly sensitive Mössbauer spectroscopy, reveal the presence of just one order parameter showing long-range ordering below T = 185 K and the critical nature of the transition. In addition, a non-zero in-plane magnetization is found, consistent with the presence of uncompensated spins at phase or domain boundaries, as proposed for bulk samples.

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Document Information

Document Title Structure and magnetic properties of epitaxial CaFe2O4 thin films
Author / Organization Silvia Damerio, Pavan Nukala, Jean Juraszek, Pim Reith, Hans Hilgenkamp, Beatriz Noheda
Subject & Discipline Multidisciplinary Academic Open Research
Categories Science & Mathematics
Publication Year 2020
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-179000
Original Source Link Visit Source Page on hal.science »