Transverse instability in the "light sail" ion acceleration - Archive ouverte HAL
Pré-Publication, Document De Travail Année : 2019

Transverse instability in the "light sail" ion acceleration

Y. Wan
  • Fonction : Auteur
I.A. Andriyash
W. Lu
  • Fonction : Auteur
W.B. Mori
  • Fonction : Auteur

Résumé

Acceleration of ultrathin plasma foils by laser radiation pressure promises compact alternatives to the conventional ion accelerators. It was shown, that a major showstopper for such schemes is a strong transverse instability, which develops the surface ripples, and is often attributed to the Rayleigh-Taylor (RT) type. However, simulations indicate, that these perturbations develop the features, that cannot be consistently explained by the RT mechanism. Here we develop a three-dimensional (3D) theory of this instability, which shows that its linear stage is mainly driven by strong electron-ion coupling, while the RT contribution is actually weak. Our model provides the instability spectral structure and its growth rate, that agrees with the large scale 3D particle-in-cell simulations. Numerical modeling shows, that target destruction results from a rapid plasma heating induced by the instability field. Possible paths to instability mitigation are discussed.

Dates et versions

hal-02165528 , version 1 (26-06-2019)

Identifiants

Citer

Y. Wan, I.A. Andriyash, W. Lu, W.B. Mori, V. Malka. Transverse instability in the "light sail" ion acceleration. 2019. ⟨hal-02165528⟩
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