Late stages of the Rayleigh-Taylor instability - A numerical study in the context of accreting neutron stars

1985 ◽  
Vol 299 ◽  
pp. 85 ◽  
Author(s):  
Y.-M. Wang ◽  
J. A. Robertson
Keyword(s):  
Neutron Stars ◽  
Numerical Study ◽  
Taylor Instability ◽  
Rayleigh Taylor Instability ◽  
Late Stages

A numerical study of bubble interactions in Rayleigh–Taylor instability for compressible fluids

1990 ◽  
Vol 2 (11) ◽  
pp. 2046-2054 ◽  
Author(s):  
J. Glimm ◽  
X. L. Li ◽  
R. Menikoff ◽  
D. H. Sharp ◽  
Q. Zhang
Keyword(s):  
Numerical Study ◽  
Taylor Instability ◽  
Compressible Fluids ◽  
Bubble Interactions ◽  
Rayleigh Taylor Instability

Density Ratio and Entrainment Effects on Asymptotic Rayleigh–Taylor Instability

2017 ◽  
Vol 140 (5) ◽  
Author(s):  
Assaf Shimony ◽  
Guy Malamud ◽  
Dov Shvarts
Keyword(s):  
Numerical Study ◽  
Density Ratio ◽  
Three Dimensional ◽  
Growth Parameter ◽  
Taylor Instability ◽  
Mixing Zone ◽  
Mixing Process ◽  
Mixing Parameters ◽  
Rayleigh Taylor Instability ◽  
Self Similar

A comprehensive numerical study was performed in order to examine the effect of density ratio on the mixing process inside the mixing zone formed by Rayleigh–Taylor instability (RTI). This effect exhibits itself in the mixing parameters and increase of the density of the bubbles. The motivation of this work is to relate the density of the bubbles to the growth parameter for the self-similar evolution, α, we suggest an effective Atwood formulation, found to be approximately half of the original Atwood number. We also examine the sensitivity of the parameters above to the dimensionality (two-dimensional (2D)/three-dimensional (3D)) and to numerical miscibility.

A Numerical Study of Rayleigh-Taylor Instability in Magnetic Fluids

1995 ◽  
Vol 453 ◽  
pp. 332 ◽  
Author(s):  
Byung-Il Jun ◽  
Michael L. Norman ◽  
James M. Stone
Keyword(s):  
Numerical Study ◽  
Magnetic Fluids ◽  
Taylor Instability ◽  
Rayleigh Taylor Instability
Sign in / Sign up

Export Citation Format

Share Document