Elastic-plastic Rayleigh-Taylor instability at a cylindrical interface

2021 ◽  
Vol 104 (3) ◽  
Author(s):  
A. R. Piriz ◽  
S. A. Piriz ◽  
N. A. Tahir
2009 ◽  
Vol 105 (11) ◽  
pp. 116101 ◽  
Author(s):  
A. R. Piriz ◽  
J. J. López Cela ◽  
N. A. Tahir

2010 ◽  
Vol 244 (2) ◽  
pp. 022007
Author(s):  
A R Piriz ◽  
J J López Cela ◽  
N A Tahir

1998 ◽  
Vol 80 (6) ◽  
pp. 1212-1215 ◽  
Author(s):  
Guy Dimonte ◽  
Robert Gore ◽  
Marilyn Schneider

2014 ◽  
Vol 136 (6) ◽  
Author(s):  
Subramanian Annamalai ◽  
Manoj K. Parmar ◽  
Yue Ling ◽  
S. Balachandar

The nonlinear growth of instabilities of an outward propagating, but decelerating, cylindrical interface separated by fluids of different densities is investigated. Single mode perturbations are introduced around the contact-surface, and their evolution is studied by conducting inviscid 2D and 3D numerical simulations. In the past, a significant amount of work has been carried out to model the development of the perturbations in a planar context where the contact surface is stationary or in a spherical context where a point-source blast wave is initiated at the origin. However, for the finite-source cylindrical blast-wave problem under consideration, there is a need for a framework which includes additional complexities such as compressibility, transition from linear to nonlinear stages of instability, finite thickness of the contact interface (CI), and time-dependent deceleration of the contact surface. Several theoretical potential flow models are presented. The model which is able to capture the above mentioned effects (causing deviation from the classical Rayleigh–Taylor Instability (RTI)) is identified as it compares reasonably well with the DNS results. Only for higher wavenumbers, the early development of secondary instabilities (Kelvin–Helmholtz) complicates the model prediction, especially in the estimation of the high-density fluid moving into low-density ambient.


2021 ◽  
Vol 103 (2) ◽  
Author(s):  
S. A. Piriz ◽  
A. R. Piriz ◽  
N. A. Tahir ◽  
S. Richter ◽  
M. Bestehorn

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