Magnetic field generation in plasma waves driven by co-propagating intense twisted lasers

ORAL

Abstract

We present a new magnetic field generation mechanism in underdense plasmas driven by the beating of two, co-propagating, Laguerre-Gaussian (LG) orbital angular momentum (OAM) laser pulses with different frequencies and also different twist indices. Results of 3D particle-in-cell simulations show that the twisted ponderomotive force drives up an electron plasma wave with a helical rotating structure. For the case of 300 fs duration, 3.8×1017 W/cm2 peak laser intensity we observe magnetic field of up to 0.4 MG. We will also outline a theoretical model, based on cold electron fluid equations, that reproduces that pertinent features of the PIC simulations – including the axial magnetic field – in the appropriate limits and elucidates the mechanism and highlights its scaling with key parameters.To second order, there is a nonlinear rotating current leading to the onset of an intense, static axial magnetic field, which persists over a long time in the plasma (ps scale) after the laser pulses have passed by. Applications of this new method of magnetic field creation will be discussed.

Presenters

  • Yin Shi

    UC San Diego , Imperial College London

Authors

  • Yin Shi

    UC San Diego , Imperial College London

  • Jorge M Vieira

    ISCTE - Inst Universitario Lisboa, Instituto Superior Técnico, Lisbon, Portugal, GoLP/Instituto Superior Tecnico, Inst Superior Tecnico (IST), GoLP/IPFN Instituto Superior Técnico, Universidade de Lisboa, Lisboa, Portugal, Instituto de Plasmas e Fusão Nuclear-Laboratório Associado, Inst Superior Tecnico (IST), Inst Superior Tecnico (IST)

  • Raoul M Trines

    Rutherford Appleton Lab

  • Robert Bingham

    Rutherford Appleton Lab, Rutherford Appleton Lab, University of Strathclyde, Rutherford Appleton Lab, Univeristy of Stratchclyde

  • Baifei Shen

    Shanghai Inst of Opt & Fine Mechanics

  • Robert J Kingham

    Imperial College London