Temperature evolution of the phonon dynamics in the Kitaev spin liquid

Kexin Feng, Mengxing Ye, Natalia B. Perkins

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17 Scopus citations

Abstract

Here we present a study of the phonon dynamics in the honeycomb Kitaev spin model at finite temperatures. We show that the fractionalized spin excitations of the Kitaev spin liquid, the itinerant Majorana fermions, and static Z2 fluxes have distinct effects on the phonon dynamics, which makes the phonon dynamics a promising tool for exploring the Kitaev spin liquid candidate materials. In particular, we focus on the signature of the fractionalized excitations in the thermodynamic behavior of the sound attenuation and the phonon Hall viscosity: the former describes the phonon decay into the fractionalized excitations, and the latter is the leading order time-reversal symmetry breaking effect on the acoustic phonon. We find that the angular dependence of the attenuation coefficient and its magnitude is modified by the thermal excitation of the Z2 fluxes. The strength of this effect strongly depends on the relative magnitude of the sound velocity and the Fermi velocity characterizing the low-energy Majorana fermions. We also show that the Hall viscosity is strongly suppressed by the increase of the density of the Z2 fluxes at finite temperatures. All these observations reflect the effects of the emergent disorder on the Majorana fermions introduced by the Z2 fluxes. Our analysis is based on the complementary analytical calculations in the low-temperature zero-flux sector, and numerical calculations in the inhomogeneous flux sectors at intermediate and high temperatures with stratified Monte Carlo (strMC) method.

Original languageEnglish (US)
Article number214416
JournalPhysical Review B
Volume103
Issue number21
DOIs
StatePublished - Jun 1 2021

Bibliographical note

Funding Information:
M.Y. and N.B.P. thank Fiona Burnell, Rafael Fernandes and Wen-Han Kao for valuable discussions. K.F. and N.B.P. were supported by the U.S. Department of Energy, Office of Basic Energy Sciences under Award No. DE-SC0018056. N.B.P. acknowledges the hospitality of Kavli Institute for Theoretical Physics and the National Science Foundation under Grant No. NSF PHY-1748958. M.Y. was supported in part by the Gordon and Betty Moore Foundation through Grant GBMF8690 to UCSB and by the National Science Foundation under Grant No. NSF PHY-1748958. The authors thank the Minnesota Supercomputing Institute for providing computing resources, with which the numerical calculations in this paper were performed.

Publisher Copyright:
© 2021 American Physical Society.

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