Topological surface states in Kondo insulator SmB$_{6}$ via planar tunneling spectroscopy$^{\ast }$
ORAL
Abstract
Samarium hexaboride (SmB$_{6})$ belongs to a class of materials called Kondo insulators in which the hybridization between itinerant electrons and local moments leads to an emergent state of matter. With inherently large spin-orbit coupling along with strong correlation, SmB$_{6}$ has been recently predicted to be topological meaning that topologically robust conducting states should exist at its surfaces. Although extensive investigations have provided growing evidence for the existence of such states, corroborative spectroscopic evidences are still lacking unlike in the weakly correlated counterparts. We adopt planar tunneling spectroscopy to unveil their detailed nature and behavior utilizing its inherently high energy resolution. Measurements of tunneling conductance on two different crystal surfaces (001) and (011) reveal the expected linear density of states for two and one Dirac cones, respectively. Moreover, it is found that these topological states cease to be protected well before they merge into the bulk states at the gap edges. Microscopic modeling of the tunneling processes accounting for the interaction with spin excitons as predicted by a recent theory [1] provide consistent explanations for all the observed features, corroborating the proposed picture on the incompletely protected surface states in SmB$_{6}$. [1] Kapilevich \textit{et al}., Phys. Rev. B \textbf{92}, 085133 (2015). $^{\ast }$The work at UIUC is supported by the NSF DMR 12-06766.
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Authors
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Wan Kyu Park
University of Illinois at Urbana-Champaign, University of Illinois Urbana-Champaign
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Lunan Sun
University of Illinois at Urbana-Champaign
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Alex Noddings
University of Illinois at Urbana-Champaign
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Laura Greene
Florida State University, NHMFL, National High Magnetic Field Laboratory and Florida State University
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Dae-Jeong Kim
University of California, Irvine, Dept. of Physics and Astronomy, University of California, Irvine, University of California at Irvine, Department of Physics and Astronomy
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Zachary Fisk
University of California, Irvine, University of California at Irvine, Department of Physics and Astronomy