Relative role of convective and diffusive mixing in the miscible Rayleigh-Taylor instability in porous media

2017 ◽  
Vol 2 (1) ◽  
Author(s):  
S. S. Gopalakrishnan ◽  
J. Carballido-Landeira ◽  
A. De Wit ◽  
B. Knaepen
Keyword(s):  
Porous Media ◽  
Taylor Instability ◽  
Relative Role ◽  
Rayleigh Taylor Instability ◽  
Diffusive Mixing

scholarly journals Supernova Explosions - The Role of a Rayleigh-Taylor Instability

1980 ◽  
Vol 58 ◽  
pp. 571-577
Author(s):  
J. Robert Buchler ◽  
Mario Livio ◽  
Stirling A. Colgate
Keyword(s):  
Large Scale ◽  
Supernova Explosion ◽  
Taylor Instability ◽  
Core Collapse ◽  
Two Dimensional ◽  
Supernova Explosions ◽  
Hydrodynamic Study ◽  
Rayleigh Taylor Instability ◽  
Energy And Momentum

AbstractA two dimensional hydrodynamic study indicates that convectively unstable gradients which develop during core collapse and bounce give rise to large scale core overturn. It is also shown that the concomitant release of neutrini can deposit large amounts of energy and momentum in the infalling envelope and give rise to a powerful supernova explosion.

Rayleigh Taylor instability of rotating compressible fluid through porous media

Meccanica ◽  
2010 ◽  
Vol 46 (6) ◽  
pp. 1331-1340 ◽  
Author(s):  
Aiyub Khan ◽  
S. S. Tak ◽  
Neha Sharma
Keyword(s):  
Porous Media ◽  
Compressible Fluid ◽  
Taylor Instability ◽  
Rayleigh Taylor Instability
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