Instability of a Thin Conducting Foil Accelerated by a Finite Wavelength Intense Laser
arXiv:1408.1558 · doi:10.1088/1367-2630/17/3/033026
Abstract
We derive a theoretical model for the Rayleigh-Taylor (RT)-like instability for a thin foil accelerated by an intense laser, taking into account finite wavelength effects in the laser wave field. The latter leads to the diffraction of the electromagnetic wave off the periodic structures arising from the instability of the foil, which significantly modifies the growth rate of the RT-like instability when the perturbations on the foil have wavenumbers comparable to or larger than the laser wavenumber. In particular, the growth rate has a local maximum at a perturbation wavenumber approximately equal to the laser wavenumber. The standard RT instability, arising from a pressure difference between the two sides of a foil, is approximately recovered for perturbation wavenumbers smaller than the laser wavenumber. Differences in the results for circular and linear polarization of the laser light are pointed out. The model has significance to radiation pressure acceleration of thin foils and to laser-driven inertial confinement fusion schemes, where RT-like instabilities are significant obstacles.
5 pages, 1 figure
References in corpus (3)
- Radiation Pressure Acceleration of Thin Foils with Circularly Polarized Laser Pulses
- Laser-Driven Rayleigh-Taylor Instability: Plasmonics Effects and Three-Dimensional Structures
- Suppression of transverse ablative Rayleigh-Taylor-like instability in the hole-boring radiation pressure acceleration by using elliptically polarized laser pulses
Cited by in corpus (4)
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- Radiation pressure acceleration of protons from structured thin-foil targets