Abstract
In this paper, we present a comprehensive study of the low-energy optical magnetic response of the skyrmionic Mott insulator Cu 2 OSeO 3 via high resolution time-domain THz spectroscopy. In zero field, a new magnetic excitation (f 0 = 2.03 THz) which has not been predicted by spin-wave theory is observed and shown, with accompanying time-of-flight neutron scattering experiments, to be a zone folded magnon from the R to Γ points of the Brillouin zone. Highly sensitive polarimetry experiments performed in weak magnetic fields, μ 0 H < 200 mT, observe Faraday and Kerr rotations which are proportional to the sample magnetization, allowing for optical detection of the skyrmion phase and construction of a magnetic phase diagram. From these measurements, we extract a critical exponent of β = 0.35 ± 0.04, in good agreement with the expected value for the 3D Heisenberg universality class of β = 0.367. In large magnetic fields, μ 0 H > 5 T, we observe the magnetically active uniform mode of the ferrimagnetic field polarized phase whose dynamics as a function of field and temperature are studied. In addition to extracting a g eff = 2.08 ± 0.03, we observe the uniform mode to decay through a non-Gilbert damping mechanism and to possess a finite spontaneous decay rate, Γ 0 ≈ 25 GHz, in the zero temperature limit. Our observations are attributed to Dzyaloshinkii-Moriya interactions, which have been proposed to be exceptionally strong in Cu 2 OSeO 3 and are expected to impact the low-energy magnetic response of such chiral magnets.
Original language | English |
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Article number | 235155 |
Journal | Physical Review B |
Volume | 95 |
Issue number | 23 |
DOIs | |
State | Published - Jun 2017 |
Funding
This research was funded by the US Department of Energy, Office of Basic Energy Sciences, Division of Materials Sciences and Engineering through Grant No. DE-FG02-08ER46544. A portion of this research used resources at the Spallation Neutron Source, a DOE Office of Science User Facility operated by the Oak Ridge National Laboratory. N.J.L. acknowledges additional support through the ARCS Foundation Dillon Fellowship. G.G.M. acknowledges generous support from the NSF-GRFP, Grant No. DGE-1232825. We would like to thank L. Balents, S. Chernyshev, W. Fuhrman, F. Mahmood, K. Plumb, M. Valentine, and C. Varma for helpful conversations.