Unusual Phonon Heat Transport in α-RuCl3: Strong Spin-Phonon Scattering and Field-Induced Spin Gap

被引:171
作者
Hentrich, Richard [1 ]
Wolter, Anja U. B. [1 ]
Zotos, Xenophon [1 ,2 ,3 ]
Brenig, Wolfram [4 ]
Nowak, Domenic [5 ]
Isaeva, Anna [5 ]
Doert, Thomas [5 ]
Banerjee, Arnab [6 ]
Lampen-Kelley, Paula [7 ,8 ]
Mandrus, David G. [7 ,8 ]
Nagler, Stephen E. [6 ]
Sears, Jennifer [9 ,10 ]
Kim, Young-June [9 ,10 ]
Buechner, Bernd [1 ,11 ,12 ]
Hess, Christian [1 ,12 ]
机构
[1] Leibniz Inst Solid State & Mat Res, D-01069 Dresden, Germany
[2] Univ Crete, ITCP, Iraklion 71003, Greece
[3] Univ Crete, Dept Phys, CCQCN, Iraklion 71003, Greece
[4] TU Braunschweig, Inst Theoret Phys, D-38106 Braunschweig, Germany
[5] Tech Univ Dresden, Dept Chem & Food Chem, D-01062 Dresden, Germany
[6] Oak Ridge Natl Lab, Quantum Condensed Matter Div, Oak Ridge, TN USA
[7] Oak Ridge Natl Lab, Mat Sci & Technol Div, Oak Ridge, TN USA
[8] Univ Tennessee, Dept Mat Sci & Engn, Knoxville, TN 37996 USA
[9] Univ Toronto, Dept Phys, 60 St George St, Toronto, ON M5S 1A7, Canada
[10] Univ Toronto, Ctr Quantum Mat, 60 St George St, Toronto, ON M5S 1A7, Canada
[11] Tech Univ Dresden, Inst Solid State Phys, D-01069 Dresden, Germany
[12] Tech Univ Dresden, Ctr Transport & Devices, D-01069 Dresden, Germany
基金
加拿大自然科学与工程研究理事会;
关键词
LATTICE THERMAL CONDUCTIVITY; LIQUID; MAGNET; MODEL;
D O I
10.1103/PhysRevLett.120.117204
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The honeycomb Kitaev-Heisenberg model is a source of a quantum spin liquid with Majorana fermions and gauge flux excitations as fractional quasiparticles. Here we unveil the highly unusual low-temperature heat conductivity kappa of alpha-RuCl (3), a prime candidate for realizing such physics: beyond a magnetic field of B-c approximate to 7.5 T, kappa increases by about one order of magnitude, both for in-plane as well as out-of-plane transport. This clarifies the unusual magnetic field dependence unambiguously to be the result of severe scattering of phonons off putative Kitaev-Heisenberg excitations in combination with a drastic field-induced change of the magnetic excitation spectrum. In particular, an unexpected, large energy gap arises, which increases linearly with the magnetic field, reaching remarkable (h) over bar omega(0) /k(B) approximate to 50 K at 18 T.
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收藏
页数:6
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