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    Influence of Kerr anisotropy in parametric amplification

    Nathan G. Drouillard1, Fadi Farook2, Meerna Albert1, Rachel Durling1, Jordan Saad1, Jeffrey G. Rau1, and TJ Hammond1,*

    • *Contact author: tj.hammond@uwindsor.ca

    Phys. Rev. A 113, 043513 – Published 14 April, 2026

    DOI: https://doi.org/10.1103/hqqh-q2c9

    Abstract

    Four-wave parametric amplification can be extended to the TW/cm2 regime using femtosecond pump pulses to amplify nearly octave spanning pulses achieving gain greater than 20 mm−1, which we call Kerr instability amplification. Cross-polarized wave generation exploits Kerr anisotropy to induce a transient intensity-dependent polarization evolution. In this work we combine Kerr instability amplification with cross-polarized wave generation to simultaneously amplify and rotate the output polarization of a signal beam, and we explore laser and crystal parameters to control the resulting polarization. In 1 mm MgO(100), we amplify linearly polarized light by 2000× orthogonal to the pump and seed polarization. The parametric amplification and polarization rotation offers excellent pulse contrast enhancement for future high-power laser systems. Furthermore, the polarization provides an additional observable to study the nonlinear dynamics occurring in this extreme ultrafast light-matter interaction.

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