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Strong Long-Wave Infrared Optical Response in a Topological Semiconductor with a Mexican Hat Band Structure

Optics 2025-02-06 v1 Materials Science

Abstract

Light sources and photodetectors operating in the far- to mid-infrared (FIR/MIR) band (88-12 μm12~\rm \mu m, 0.10.1-0.15 eV0.15~\rm eV) remain relatively poorly developed compared to their counterparts operating in the visible and near-infrared ranges, despite extensive application potential for thermal imaging, standoff sensing, and other technologies. This is attributable in part to the lack of narrow-gap materials (<0.1 eV<0.1~\rm eV) with high optical gain and absorption. In this work, a narrow-gap semiconductor, Pb0.7Sn0.3Se\rm Pb_{0.7}Sn_{0.3}Se, is demonstrated to exhibit an optical response >10×>10\times larger than that of HgxCd1xTe\rm Hg_{x}Cd_{1-x}Te (MCT), the dominant material for FIR/MIR photodetectors. A previous theoretical investigation indicated that chalcogen pp and metal dd band inversion in this material creates a Mexican hat band structure (MHBS), which results in a dramatic increase in the joint density of states at the optical transition edge compared to typical semiconductors. This prediction is experimentally validated here using single-crystal specimens of Pb0.7Sn0.3Se\rm Pb_{0.7}Sn_{0.3}Se measured using temperature-dependent spectroscopic ellipsometry over a wavelength range of 1.71.7-20 μm20~\rm \mu m (0.730.73-0.062 eV0.062~\rm eV). These measurements demonstrate a large enhancement in extinction coefficient and refractive index characteristic of a MHBS in the vicinity of the absorption edge, in agreement with theoretical predictions. The realization of topological semiconductors with a MHBS is expected to lead to high-efficiency detectors operating in the FIR/MID range.

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Cite

@article{arxiv.2502.02791,
  title  = {Strong Long-Wave Infrared Optical Response in a Topological Semiconductor with a Mexican Hat Band Structure},
  author = {Mark J. Polking and Haowei Xu and Raman Sankar and Kevin Grossklaus and Ju Li},
  journal= {arXiv preprint arXiv:2502.02791},
  year   = {2025}
}

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