Abstract

In this work we study the electronic structure of and , two chiral insulators whose gap can be tuned through small changes in the lattice parameter by applying hydrostatic pressure or choosing different growth protocols. Based on first principles calculations we compute their band structure for different values of the lattice parameters and show that while retains its direct narrow gap at the Γ point, can turn into a metal. Focusing on we derive a low energy model around Γ using group theory, which we use to calculate the optical conductivity for different values of the lattice constant. We discuss our results in the context of detection of light dark matter particles, which have masses of the order of a keV, and conclude that satisfies three important requirements for a suitable detector: small Fermi velocities, meV band gap, and low photon screening. Our work motivates the growth of high-quality and large samples of to be used as target materials in dark matter detectors.

Highlights

  • BergaraDonostia International Physics Center, 20018 Donostia-San Sebastian, Spain IKERBASQUE, Basque Foundation for Science, Maria Diaz de Haro 3, 48013 Bilbao, Spain

  • Narrow gap semiconductors belong to a particular branch of the semiconductor family, those with a narrow forbidden energy window, the gap, between valence and conduction bands

  • In this work we study the electronic structure of Ag3AuSe2 and Ag3AuTe2, two chiral insulators whose gap can be tuned through small changes in the lattice parameter by applying hydrostatic pressure or choosing different growth protocols

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Summary

Bergara

Donostia International Physics Center, 20018 Donostia-San Sebastian, Spain IKERBASQUE, Basque Foundation for Science, Maria Diaz de Haro 3, 48013 Bilbao, Spain

Introduction
Analysis based on Density Functional Theory
Effective model
How to build effective models
Effective Hamiltonian for conduction bands
Coupling Hamiltonian
Low energy Hamiltonian and parameters
Optical conductivity
Optical conductivity and relevant transitions for a given lattice parameter
Optical conductivity for different lattice parameters
Feasibility for light dark matter detection
Findings
Conclusion
Full Text
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