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Zigzag spin structure in layered honeycomb Li3Ni2SbO6: A combined diffraction and antiferromagnetic resonance study.

Authors :
Kurbakov, A. I.
Korshunov, A. N.
Podchezertsev, S. Yu.
Malyshev, A. L.
Evstigneeva, M. A.
Damay, F.
Park, J.
Koo, C.
Klingeler, R.
Zvereva, E. A.
Nalbandyan, V. B.
Source :
Physical Review B. 7/8/2017, Vol. 96 Issue 2, p1-1. 1p.
Publication Year :
2017

Abstract

The magnetic structure of Li3Ni2SbO6 has been determined by low-temperature neutron diffraction, and the crystal structure has been refined by a combination of synchrotron and neutron powder diffraction. The monoclinic (C2/m) symmetry, assigned previously to this pseudohexagonal layered structure, has been unambiguously proven by peak splitting in the synchrotron diffraction pattern. The structure is based on essentially hexagonal honeycomb-ordered Ni2SbO6 layers alternating with Li3 layers, all cations and anions being in an octahedral environment. The compound orders antiferromagnetically below TN = 15 K, with the magnetic supercell being a 2a × 2b multiple of the crystal cell. The magnetic structure within the honeycomb layer consists of zigzag ferromagnetic spin chains coupled antiferromagnetically. The ordered magnetic moment amounts to 1.62 (2) µ B/Ni, which is slightly lower than the full theoretical value. Upon cooling below TN, the spins tilt from the c axis, with a maximum tilting angle of 15.6° at T = 1.5 K. Our data imply non-negligible ferromagnetic interactions between the honeycomb layers. The observed antiferromagnetic resonance modes are in agreement with the two-sublattice model derived from the neutron data. Orthorhombic anisotropy shows up in zero-field splitting of Δ = 198 ± 4 and 218 ± 4 GHz. Above TN, the electron spin resonance data imply short-range antiferromagnetic order up to about 80 K. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
24699950
Volume :
96
Issue :
2
Database :
Academic Search Index
Journal :
Physical Review B
Publication Type :
Academic Journal
Accession number :
124521764
Full Text :
https://doi.org/10.1103/PhysRevB.96.024417