22–27 Jul 2012
Embassy Suites Napa Valley
US/Pacific timezone

Optical conductivity of Bismuth-based topological insulators

23 Jul 2012, 17:15
25m
Chardonnay Ballroom (Embassy Suites Napa Valley)

Chardonnay Ballroom

Embassy Suites Napa Valley

1075 California Boulevard, Napa, California, United States 94559
Invited Topological Insulators Topological Insulators I

Speaker

Stefano Lupi (Department of Physics, University of Rome La Sapienza)

Description

Stefano Lupi Department of Physics University of Rome La Sapienza Topological Insulators (TI) are new quantum materials with an insulating-gap in the bulk of spin-orbit origin and metallic states at the surface. These states are chiral and show dissipation-less transport properties protected from disorder by the time-reversal symmetry. In addition to their fundamental properties, TI have potential applications in quantum computing, photonics, and spintronic devices. Materials belonging to the V2VI3 (V= Bi, Sb, S; VI = Se, Te, S) family recently emerged, due to their large bulk insulating gap (~300 meV), as the first candidates for the study of topological surface states. However the as-grown crystals usually display, due to impurities/unstoichiometry related to the growing process, an extrinsic degenerate semiconducting behavior. Those impurities affect the low energy transport properties, rendering difficult the separation between the intrinsic 2D metallic behavior due to topological surface states and the 3D metallic conduction induced by extrinsic charges. In this talk I will discuss the optical conductivity σ1(ω) and the optical spectral weight SW of four topological insulators with an increasing chemical compensation (Bi2Se3, Bi2-xCaxSe3 x=0.005, Bi2Se2Te, Bi2Te2Se). The effect of compensation is clearly visible in the infrared spectra, through the suppression of the extrinsic Drude term and the appearance of strong peaks in the terahertz range assigned to electronic transition among impurity states. The SW of the most compensated sample (Bi2Te2Se) is still nearly two orders of magnitude higher than that expected from the surface states.

Primary author

Stefano Lupi (Department of Physics, University of Rome La Sapienza)

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