2018
DOI: 10.1073/pnas.1717236115
|View full text |Cite|
|
Sign up to set email alerts
|

Rayleigh–Taylor instabilities in high-energy density settings on the National Ignition Facility

Abstract: The Rayleigh-Taylor (RT) instability occurs at an interface between two fluids of differing density during an acceleration. These instabilities can occur in very diverse settings, from inertial confinement fusion (ICF) implosions over spatial scales of [Formula: see text] cm (10-1,000 μm) to supernova explosions at spatial scales of [Formula: see text] cm and larger. We describe experiments and techniques for reducing ("stabilizing") RT growth in high-energy density (HED) settings on the National Ignition Faci… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1

Citation Types

2
102
0

Year Published

2019
2019
2024
2024

Publication Types

Select...
6
1

Relationship

0
7

Authors

Journals

citations
Cited by 81 publications
(104 citation statements)
references
References 71 publications
2
102
0
Order By: Relevance
“…Non-equilibrium transport, interfaces and mixing are omnipresent in nature and technology at astrophysical and at molecular scales, and in high and low energy density regimes [1]. Fluid instabilities and interfacial mixing in supernovae and in inertial confinement fusion, particle-field interactions in magnetic fusion and in imploding Z-pinches, downdrafts in stellar interior and in planetary magnetoconvection, coronal mass ejections in the Solar flares and plasma instabilities in the Earth ionosphere, plasma thrusters and nano-fabrication -are examples of processes governed by non-equilibrium interfacial dynamics [2][3][4][5][6][7][8][9][10][11][12][13][14][15][16][17][18][19]. The realistic environments are often characterized by sharply and rapidly changing flow fields and by small effects of dissipation and diffusion resulting in the formation of discontinuities (referred to as fronts or as interfaces) between the flow non-uniformities (phases) at macroscopic (continuous) scales [11].…”
Section: Section 1 -Introductionmentioning
confidence: 99%
“…Non-equilibrium transport, interfaces and mixing are omnipresent in nature and technology at astrophysical and at molecular scales, and in high and low energy density regimes [1]. Fluid instabilities and interfacial mixing in supernovae and in inertial confinement fusion, particle-field interactions in magnetic fusion and in imploding Z-pinches, downdrafts in stellar interior and in planetary magnetoconvection, coronal mass ejections in the Solar flares and plasma instabilities in the Earth ionosphere, plasma thrusters and nano-fabrication -are examples of processes governed by non-equilibrium interfacial dynamics [2][3][4][5][6][7][8][9][10][11][12][13][14][15][16][17][18][19]. The realistic environments are often characterized by sharply and rapidly changing flow fields and by small effects of dissipation and diffusion resulting in the formation of discontinuities (referred to as fronts or as interfaces) between the flow non-uniformities (phases) at macroscopic (continuous) scales [11].…”
Section: Section 1 -Introductionmentioning
confidence: 99%
“…This issue reports significant successes that have been achieved recently in understanding interfaces, mixing, and nonequilibrium dynamics based on theoretical analysis, large-scale numerical simulations, laboratory experiments, and technology development (20)(21)(22)(23)(24)(25)(26)(27)(28)(29)(30)(31)(32)(33)(34). These include theoretical approaches for handling complex multiscale, nonlocal, and statistically unsteady dynamics and boundary value problems; developments of efficient Eulerian and Lagrangian methods of large-scale numerical modeling; advancements in laboratory experiments in low-and high-energy density regimes; and possibilities for dramatic improvements in precision, accuracy, dynamic range, reproducibility, and data acquisition rate with the use of modern technologies (20)(21)(22)(23)(24)(25)(26)(27)(28)(29)(30)(31)(32)(33)(34).…”
mentioning
confidence: 99%
“…These works represent frontier research in interaction of molecules and chemical reactions, interfacial dynamics and nonequilibrium processes, fluid turbulence and turbulent mixing, supernovas and nuclear synthesis, formation of fluid phases at molecular scales, first-principlesbased reaction kinetics, ion transport of nanoscales, electric and magnetic fields structures, dynamics of high-energy density plasmas, subdiffusive and superdiffusive transport, formation of vortices in geophysical flows, diffusiophoresis of charged particles, and electron transport in macromolecules. They motivate the discussions of rigorous mathematical problems, theoretical approaches, and state-of-the-art numerical simulations along with advanced experimental methods and technological applications (20)(21)(22)(23)(24)(25)(26)(27)(28)(29)(30)(31)(32).…”
mentioning
confidence: 99%
See 2 more Smart Citations