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.
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Presenters
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Yin Shi
UC San Diego , Imperial College London
Authors
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Yin Shi
UC San Diego , Imperial College London
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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)
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Raoul M Trines
Rutherford Appleton Lab
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Robert Bingham
Rutherford Appleton Lab, Rutherford Appleton Lab, University of Strathclyde, Rutherford Appleton Lab, Univeristy of Stratchclyde
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Baifei Shen
Shanghai Inst of Opt & Fine Mechanics
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Robert J Kingham
Imperial College London