# Transverse instability in the "light sail" ion acceleration

**Authors:** Y. Wan, I. A. Andriyash, W. Lu, W. B. Mori, V. Malka

arXiv: 1903.11354 · 2019-04-04

## TL;DR

This paper develops a 3D theoretical model of transverse instability in laser-driven ion acceleration, revealing electron-ion coupling as the main driver, and aligns with simulation results, offering insights for instability mitigation.

## Contribution

A novel 3D theory of transverse instability in light sail ion acceleration, emphasizing electron-ion coupling over Rayleigh-Taylor effects, supported by simulation validation.

## Key findings

- Electron-ion coupling drives the instability's linear stage.
- The spectral structure and growth rate match 3D PIC simulations.
- Target destruction is caused by rapid plasma heating from the instability.

## Abstract

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.

## Full text

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## Figures

6 figures with captions in the complete paper: https://tomesphere.com/paper/1903.11354/full.md

## References

36 references — full list in the complete paper: https://tomesphere.com/paper/1903.11354/full.md

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Source: https://tomesphere.com/paper/1903.11354