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  • Letter

Analytical WKB theory for high-harmonic generation and its application to massive Dirac electrons

Hidetoshi Taya1,2,*, Masaru Hongo3,1,†, and Tatsuhiko N. Ikeda4,‡

  • 1RIKEN iTHEMS, RIKEN, Wako 351-0198, Japan
  • 2Research and Education Center for Natural Sciences, Keio University 4-1-1 Hiyoshi, Kohoku-ku, Yokohama, Kanagawa 223-8521, Japan
  • 3Department of Physics, University of Illinois, Chicago, Illinois 60607, USA
  • 4Institute for Solid State Physics, University of Tokyo, Kashiwa, Chiba 277-8581, Japan

  • *hidetoshi.taya@riken.jp
  • †masaru.hongo@riken.jp
  • ‡tikeda@issp.u-tokyo.ac.jp

Phys. Rev. B 104, L140305 – Published 21 October, 2021

DOI: https://doi.org/10.1103/PhysRevB.104.L140305

Abstract

We propose an analytical approach to high-harmonic generation (HHG) for nonperturbative low-frequency and high-intensity fields based on the (Jeffreys-)Wentzel-Kramers-Brillouin (WKB) approximation. By properly taking into account Stokes phenomena of WKB solutions, we obtain wave functions that systematically include the repetitive dynamics of production and acceleration of electron-hole pairs and quantum interference due to phase accumulation between different pair production times (Stückelberg phase). Using the obtained wave functions without relying on any phenomenological assumptions, we explicitly compute electric current (including intra- and interband contributions) as the source of HHG for a massive Dirac system in (1+1) dimensions under an ac electric field. We demonstrate that the WKB approximation agrees well with numerical results obtained by solving the time-dependent Schrödinger equation and point out that the quantum interference is important in HHG. We also predict in the deep nonperturbative regime that (1) harmonic intensities oscillate with respect to electric-field amplitude E0 and frequency Ω, with a period determined by the Stückelberg phase, (2) the cutoff order of HHG is determined by 2eE0/ℏΩ2, with e being the electron charge, and that (3) noninteger harmonics, controlled by the Stückelberg phase, appear as a transient effect. Our WKB theory is particularly suited for a parameter regime, where the Keldysh parameter γ=(Δ/2)Ω/eE0, with Δ being the gap size, is small. This parameter regime corresponds to intense lasers in the terahertz regime for realistic massive Dirac materials. Our analysis implies that the so-called HHG plateau can be observed at the terahertz frequency within the current technology.

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