A magnetic excitation linking quasi-1D Chevrel-type selenide and arsenide superconductors
arXiv:2110.10226 · doi:10.1103/PhysRevMaterials.6.124804
Abstract
The quasi-one-dimensional Chevrel phases, AMoSe (A = Tl, In, K, Rb, Cs), are of interest due to their atypical electronic properties. The Tl and In analogues undergo a superconducting transition whereas the alkali metal analogues show charge gapping of another, not well understood type. We report the results of inelastic neutron scattering on polycrystalline InMoSe (K) and RbMoSe (non-superconducting) samples, which reveal a column of intensity with linear dispersion from [0 0 1/2] to [0 0 1] in both compounds. The observed temperature and || independence together suggest the presence of unconventional carriers with a spin contribution to the excitation. This is contrary to the prevailing model for these materials, which is that they are non-magnetic. The excitation has similar dispersion and behavior as one observed in the structurally related superconducting compounds ACrAs and AMoAs (A = K, Rb, Cs), which has been interpreted as magnetic in origin and related to Fermi surface nesting. The connection is unexpected because the calculated Fermi surface of the arsenides differs substantially from the AMoSe compounds, and many consider them distinct classes of materials. The new observation suggests a hidden link in the physics between both classes of superconductors, perhaps originating from their quasi-low-dimensional character.
Replaced with accepted article: 12 pages, 3 figures. Appendix: 4 pages, 1 figure
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