The effect of shape in the three-dimensional ablative Rayleigh-Taylor instability. I: Single-mode perturbations

The nonlinear saturation amplitudes attained by Rayleigh–Taylor perturbations growing on ablatively stabilized laser fusion targets are crucial in determining the survival time of those targets. For a given set of baseline simulation parameters, the peak amplitude is found to be a progressive function of cross‐sectional perturbation shape as well as of wave number, with three‐dimensional (3‐D) square modes and two‐dimensional (2‐D) axisymmetric bubbles saturating later, and at higher amplitudes than two‐dimensional planar modes. In late nonlinear times hydrodynamic evolution diverges; the 3‐D square mode bubble continues to widen, while the 2‐D axisymmetric bubble fills in.

[1]  D. Sharp An overview of Rayleigh-Taylor instability☆ , 1984 .

[2]  Mikaelian LASNEX simulations of the classical and laser-driven Rayleigh-Taylor instability. , 1990, Physical review. A, Atomic, molecular, and optical physics.

[3]  Stephen E. Bodner,et al.  Rayleigh-Taylor Instability and Laser-Pellet Fusion , 1974 .

[4]  E. Ott,et al.  Three‐dimensional, nonlinear evolution of the Rayleigh–Taylor instability of a thin layer , 1984 .

[5]  John Lindl,et al.  Hydrodynamic stability and the direct drive approach to laser fusion , 1990 .

[6]  G. Taylor The instability of liquid surfaces when accelerated in a direction perpendicular to their planes. I , 1950, Proceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences.

[7]  Ivan Catton,et al.  Three-dimensional Rayleigh-Taylor instability Part 2. Experiment , 1988, Journal of Fluid Mechanics.

[8]  Nishihara,et al.  Three-dimensional Rayleigh-Taylor instability of spherical systems. , 1990, Physical review letters.

[9]  S. Haan,et al.  Weakly nonlinear hydrodynamic instabilities in inertial fusion , 1991 .

[10]  Yabe,et al.  Two- and three-dimensional behavior of Rayleigh-Taylor and Kelvin-Helmholtz instabilities. , 1991, Physical review. A, Atomic, molecular, and optical physics.

[11]  J. Dahlburg,et al.  Numerical simulation of ablative Rayleigh–Taylor instability , 1991 .

[12]  J. Dahlburg,et al.  Simulation of the Rayleigh–Taylor instability in colliding, ablatively driven laser foils , 1991 .

[13]  Gardner,et al.  Ablative Rayleigh-Taylor instability in three dimensions. , 1990, Physical review. A, Atomic, molecular, and optical physics.

[14]  W. Manheimer,et al.  Steady‐state planar ablative flow , 1981 .

[15]  D. Layzer,et al.  On the Instability of Superposed Fluids in a Gravitational Field. , 1955 .

[16]  D. Youngs,et al.  Three-dimensional numerical simulation of turbulent mixing by Rayleigh-Taylor instability , 1991 .

[17]  Town,et al.  Three-dimensional simulations of the implosion of inertial confinement fusion targets. , 1991, Physical review letters.

[18]  Kunioki Mima,et al.  Self‐consistent growth rate of the Rayleigh–Taylor instability in an ablatively accelerating plasma , 1985 .

[19]  Anthony T. Patera,et al.  Secondary instability of wall-bounded shear flows , 1983, Journal of Fluid Mechanics.

[20]  I. Catton,et al.  Three-dimensional Rayleigh-Taylor instability Part 1. Weakly nonlinear theory , 1988, Journal of Fluid Mechanics.

[21]  S. Obenschain,et al.  Laser interaction in long-scale-length plasmas , 1985 .

[22]  Nonlinear aspects of hydrodynamic instabilities in laser ablation , 1982 .

[23]  Gretar Tryggvason,et al.  Computations of three‐dimensional Rayleigh–Taylor instability , 1990 .