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.
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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,