Extreme nonlinear optics in a long pulse regime: High harmonic generation of picosecond mid-IR pulses in polycrystalline zinc selenide

Author:

Marble Christopher B.1ORCID,Sanderson Carl R.2ORCID,Ballmann Charles W.2,Yakovlev Vladislav V.134ORCID

Affiliation:

1. Department of Physics and Astronomy, Texas A&M University 1 , College Station, Texas 77843, USA

2. Systems Management and Production Center, The University of Alabama in Huntsville 2 , Huntsville, Alabama 34899, USA

3. Department of Bioengineering, Texas A&M University 3 , College Station, Texas 77843, USA

4. Department of Electrical Engineering, Texas A&M University 4 , College Station, Texas 77843, USA

Abstract

High harmonic generation (HHG) in semiconductors has been extensively studied recently in the high-intensity limit using middle infrared (mid-IR) femtosecond laser pulses resulting in emission spectra of self-phase modulated harmonics resting on top of a broadband continuum. In this report, a different approach to HHG in polycrystalline zinc selenide (poly-ZnSe) was explored utilizing a relatively low power regime (1–40 GW/cm2) and much longer (30 ps) mid-IR laser pulses. Through a combination of low power, picosecond excitation, and narrowband (<10 nm full width at half maximum) mid-IR excitation, the nonlinear optical effects in poly-ZnSe could be isolated and studied independently. From the clearly distinguishable HHG peaks, harmonic conversion efficiencies of 10−4–10−12 for second to ninth harmonic in poly-ZnSe were measured, and the relationship between the Nth harmonic intensity and excitation intensity (I0) was found to follow a power law, I0x with x ≤ N/2, as a result of the random quasi-phase matching process.

Funder

National Institutes of Health

Directorate for Engineering

Air Force Office of Scientific Research

U.S. Army Medical Research Acquisition Activity

Cancer Prevention and Research Institute of Texas

U.S. Army Veterinary Corps

Human Exploration and Operations Mission Directorate

Publisher

AIP Publishing

Subject

Physics and Astronomy (miscellaneous)

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