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Spiral magnetism, spin flop, and pressure-induced ferromagnetism in the negative charge-transfer-gap insulator Sr2FeO4

Authors :
Adler, Peter
Reehuis, Manfred
Stüßer, Norbert
Medvedev, Sergey A.
Nicklas, Michael
Peets, Darren C.
Bertinshaw, Joel
Christensen, Christian Kolle
Etter, Martin
Hoser, Andreas
Schröder, Liane
Merz, Patrick
Schnelle, Walter
Schulz, Armin
Mu, Qingge
Bessas, Dimitrios
Chumakov, Aleksandr
Jansen, Martin
Felser, Claudia
Source :
'Physical Review B ', vol: 105, pages: 054417-1-054417-10 (2022), Physical review / B 105(5), 054417 (2022). doi:10.1103/PhysRevB.105.054417
Publication Year :
2022

Abstract

Physical review / B 105(5), 054417 (2022). doi:10.1103/PhysRevB.105.054417<br />Iron(IV) oxides are strongly correlated materials with negative charge-transfer energy (negative $Δ$), and exhibit peculiar electronic and magnetic properties such as topological helical spin structures in the metallic cubic perovskite SrFeO$_3$. Here, the spin structure of the layered negative-$Δ$ insulator Sr$_2$FeO$_4$ was studied by powder neutron diffraction in zero field and magnetic fields up to 6.5 T. Below $T_N$=56K, Sr$_2$FeO$_4$ adopts an elliptical cycloidal spin structure with modulated magnetic moments between 1.9 and 3.5 $μ_B$ and a propagation vector k=($τ,τ$,0) with $τ$=0.137. With increasing magnetic field the spin structure undergoes a spin-flop transition near 5 T. Synchrotron $^{57}$Fe-Mössbauer spectroscopy reveals that the spin spiral transforms to a ferromagnetic structure at pressures between 5 and 8 GPa, just in the pressure range where a Raman-active phonon nonintrinsic to the K$_2$NiF$_4$-type crystal structure vanishes. These results indicate an insulating ground state which is stabilized by a hidden structural distortion and differs from the charge disproportionation in other Fe(IV) oxides.<br />Published by Inst., Woodbury, NY

Details

Language :
English
ISSN :
24699950
Volume :
105
Database :
OpenAIRE
Journal :
Physical Review B
Accession number :
edsair.doi.dedup.....90dd0b731287b39263266bcb7d9e4780
Full Text :
https://doi.org/10.1103/PhysRevB.105.054417