In the turbulent Rayleigh–Taylor instability, the light fluid penetrates the heavy fluid as
bubbles with a diameter D b and amplitude hb that grow self-similarly D b∝ hb∼ α b A gt 2 …

The turbulent Rayleigh–Taylor instability is investigated in the limit of strong mode-coupling
using a variety of high-resolution, multimode, three dimensional numerical simulations (NS) …

The dependency of the self-similar Rayleigh-Taylor bubble acceleration constant α b
(≡[(amplitude)∕ 2]×(displacement)×(Atwood number)) on the initial perturbation amplitude …

In this research, the temporal evolution of the bubble tip velocity in Rayleigh-Taylor
instability (RTI) at arbitrary Atwood numbers and different initial perturbation velocities with a …

Implicit large eddy simulations of two-dimensional Rayleigh-Taylor instability at different
density ratios (ie, Atwood number A= 0.05, 0.5, and 0.9) are conducted to investigate the late …

In order to study the effect of compressibility on Rayleigh-Taylor (RT) instability, we
numerically simulated the late-time evolution of two-dimensional single-mode RT instability …

Growth of the single-fluid single-mode Rayleigh–Taylor instability (RTI) is revisited in 2D and
3D using fully compressible high-resolution simulations. We conduct a systematic analysis …

The growth of the two-dimensional single-mode Rayleigh-Taylor instability (RTI) at low
Atwood number (A= 0.04) is investigated using Direct Numerical Simulations. The main …

In some researches on the bubble problem in the Rayleigh–Taylor instability, the bubble
radius is identified with one-half spatial period. We show that these quantities are distinct …

From nonlinear models and direct numerical simulations we report on several findings of
relevance to the single-mode Rayleigh-Taylor (RT) instability driven by time-varying …