2010
DOI: 10.1016/j.hedp.2009.12.005
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High-mode Rayleigh-Taylor growth in NIF ignition capsules

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Cited by 162 publications
(79 citation statements)
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“…It gives equation of state and selfdiffusion coefficients with an accuracy comparable to ab-initio simulations but is computationally much more efficient. The challenge of accurately modeling dense plasmas over a wide range of conditions represents an unsolved problem lying at the heart of many important phenomena such as inertial confinement fusion [1], exoplanets and white dwarfs [2,3]. The production of large scale and accurate tabulations of data such as equation of state and transport coefficients as a function of density and temperature is a formidable task, requiring a consistent quantum mechanical treatment of the many-electron problem together with a classical treatment of the nuclear motion.…”
mentioning
confidence: 99%
“…It gives equation of state and selfdiffusion coefficients with an accuracy comparable to ab-initio simulations but is computationally much more efficient. The challenge of accurately modeling dense plasmas over a wide range of conditions represents an unsolved problem lying at the heart of many important phenomena such as inertial confinement fusion [1], exoplanets and white dwarfs [2,3]. The production of large scale and accurate tabulations of data such as equation of state and transport coefficients as a function of density and temperature is a formidable task, requiring a consistent quantum mechanical treatment of the many-electron problem together with a classical treatment of the nuclear motion.…”
mentioning
confidence: 99%
“…To model these extremely fine-scale features, specialized high-resolution 2D simulations must be run [22]. To include the important effects of the tent and the fill tube in nominal resolution simulations, surrogate perturbations are then derived from these high-resolution simulations, and their longer-wavelength features can then be initialized in the lower resolution cases.…”
Section: Discussionmentioning
confidence: 99%
“…As shown in figure 1, the linear stability of these implosions is quantified by comparing their ablation front growth factors. These growth factors are defined as the ratio of the perturbation amplitude at the time of peak implosion velocity relative to the initial perturbation amplitude for an individual Legendre mode [21][22][23]. For all cases, the simulations were run using a 2D wedge initialized with a small Gaussian bump (15 μm wide by 1 nm in height) on the ablator surface at the axis of symmetry.…”
Section: Linear Stability Simulationsmentioning
confidence: 99%
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