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Ultra-energetic electron bunches from SPW excitation in the ultra-high intensity regime

ORAL

Abstract

Recent experiments [1] have demonstrated that the resonant excitation of surface plasma waves (SPW) by ultra-high intensity fs lasers impinging on a solid-density target strongly enhances the laser-plasma coupling and provides a new path for generating relativistic, high charge electron bunches emitting radiation with interesting characteristics. In this work, we show that laser wavefront rotation (WFR) [2] acts to both shorten the duration (down to very few optical cycles) and increase the intensity of SPW [3], thus favoring the production of ultra-short, energetic electron bunches. Optimal laser parameters were identified analytically and verified by means of Particle-In-Cell (PIC) simulations with the open-source code SMILEI [4]. The laser pulse with WFR was combined with a smart grating target design. In the laser-plasma relativistic regime of interaction (i.e. Iλ2 = 3.4 × 1019 W/cm2 μm2), we show that this set-up may produce SPW with ~3.6 cycles duration which accelerate high-charge (few 10’s of pC), high-energy (up to 70 MeV) electron bunches of few fs duration [5]. Extending this set up, or more in general exploiting the possibility of SPW excitation by forthcoming multi-petawatt laser facilities ( Iλ2 > 1021) implies an in depth understanding of the SPW excitation conditions and lifetime in that regime. Through extensive parametric studies we identify the optimum SPW excitation angle in the ultra-relativistic regime, that coincides with the optimal angle to optimize the electron acceleration along the plasma surface [6]. The dependence on the plasma density and grating shape is also discussed. As a conclusion, we show that excitation of SPW by a grating can hold at the highest laser intensities available, opening the doors to new experiments on forthcoming multi-petawatt laser systems.

Publication: [1] L. Fedeli et al., Phys. Rev. Lett. 116, 015001 (2016); G. Cantono et al., Phys. Rev. Lett. 120, 264803 (2018). <br>[2] H. Vincenti and F. Quéré, Phys. Rev. Lett. 108, 113904 (2012) . <br>[3] F. Pisani, L. Fedeli and A. Macchi, ACS Photonics 5, 1068 (2018).<br>[4] J. Derouillat et al., Comput. Phys. Commun. 222, 351 (2018). <br>[5] S. Marini et al., Phys. Rev. E. 103, L021201 (2021) <br>[6] S.Marini et al., Phys. of Plasma. 28, xx (2021) <br>

Presenters

  • Michèle RAYNAUD

    LSI, CEA, CNRS, Ecole polytechnique, Institut Polytechnique de Paris

Authors

  • Michèle RAYNAUD

    LSI, CEA, CNRS, Ecole polytechnique, Institut Polytechnique de Paris

  • Paula Kleij

    LSI, CEA, CNRS, Ecole polytechnique, Institut Polytechnique de Paris

  • Samuel Marini

    LSI/LULI, CEA, CNRS, École Polytechnique, Institut Polytechnique de Paris

  • François Amiranoff

    LULI, CNRS, CEA, Sorbonne Université, École Polytechnique,Institut Polytechnique de Paris

  • Mickael Grech

    LULI, CNRS, CEA, Sorbonne Université, École Polytechnique,Institut Polytechnique de Paris,

  • Andrea Macchi

    Enrico Fermi Department of Physics, University of Pisa,

  • Caterina Riconda

    Sorbonne University, LULI, CNRS, CEA, Sorbonne Université, École Polytechnique,Institut Polytechnique de Paris,