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Pseudo-Goldstone Magnons in the Frustrated S=3/2 Heisenberg Helimagnet ZnCr_{2}Se_{4} with a Pyrochlore Magnetic Sublattice

Authors :
Y. V. Tymoshenko
Y. A. Onykiienko
T. Müller
R. Thomale
S. Rachel
A. S. Cameron
P. Y. Portnichenko
D. V. Efremov
V. Tsurkan
D. L. Abernathy
J. Ollivier
A. Schneidewind
A. Piovano
V. Felea
A. Loidl
D. S. Inosov
Source :
Physical Review X, Vol 7, Iss 4, p 041049 (2017)
Publication Year :
2017
Publisher :
American Physical Society, 2017.

Abstract

Low-energy spin excitations in any long-range ordered magnetic system in the absence of magnetocrystalline anisotropy are gapless Goldstone modes emanating from the ordering wave vectors. In helimagnets, these modes hybridize into the so-called helimagnon excitations. Here we employ neutron spectroscopy supported by theoretical calculations to investigate the magnetic excitation spectrum of the isotropic Heisenberg helimagnet ZnCr_{2}Se_{4} with a cubic spinel structure, in which spin-3/2 magnetic Cr^{3+} ions are arranged in a geometrically frustrated pyrochlore sublattice. Apart from the conventional Goldstone mode emanating from the (0 0 q_{h}) ordering vector, low-energy magnetic excitations in the single-domain proper-screw spiral phase show soft helimagnon modes with a small energy gap of ∼0.17 meV, emerging from two orthogonal wave vectors (q_{h} 0 0) and (0 q_{h} 0) where no magnetic Bragg peaks are present. We term them pseudo-Goldstone magnons, as they appear gapless within linear spin-wave theory and only acquire a finite gap due to higher-order quantum-fluctuation corrections. Our results are likely universal for a broad class of symmetric helimagnets, opening up a new way of studying weak magnon-magnon interactions with accessible spectroscopic methods.

Subjects

Subjects :
Physics
QC1-999

Details

Language :
English
ISSN :
21603308
Volume :
7
Issue :
4
Database :
Directory of Open Access Journals
Journal :
Physical Review X
Publication Type :
Academic Journal
Accession number :
edsdoj.545641831dd4f59be2539bb13b54d22
Document Type :
article
Full Text :
https://doi.org/10.1103/PhysRevX.7.041049