Abstract
Within the framework of modified Layzer-type potential flow theory [V. N. Goncharov, “Analytical model of nonlinear, single-mode, classical Rayleigh-Taylor instability at arbitrary Atwood numbers,” Phys. Rev. Lett. 88, 134502 (2002)], we study bubble growth in compressible Rayleigh–Taylor (RT) and Richtmyer–Meshkov (RM) instabilities. It is known from adiabatic equations that the density ρ and adiabatic index γ are compressibility-related factors for a given static pressure p. Here, we introduce a dynamically varying stagnation point pressure P̃=p±12ρ̃η̇02, which relates time-varying quantities, such as fluid density ρ̃, pressure P̃, and bubble tip velocity η̇0, and then, we analytically derive the governing equations for time evolution of bubbles in the RT and RM instabilities of compressible fluids. For the RT instability, the upper fluid adiabatic index γu and density ρu increase the bubble amplitude and velocity, but they decrease the bubble curvature radius at the early stage, while the lower fluid adiabatic index γl and density ρl have opposite effects on those of γu and ρu, which is consistent with recent results. For the RM instability, γu and ρu decrease the bubble amplitude and velocity, but they increase the bubble curvature radius at the early stage; however, γl and ρl have opposite effects on those of γu and ρu. Moreover, we find a good agreement between our three-dimensional results of the RM bubble amplitude and recent numerical simulations.
Highlights
Lett. 88, 134502 (2002)], we study bubble growth in compressible
When a low-density fluid supports or pushes a high-density fluid, fingering instability will happen at the interface between the two fluids
We study the bubble growth in compressible RT and RM instabilities through changing the density and adiabatic index, respectively
Summary
When a low-density fluid supports or pushes a high-density fluid, fingering instability will happen at the interface between the two fluids. We set the static density and the adiabatic index of the upper (lower) fluid at the interface to be ρu0 (ρl0) and γu (γl), respectively. We obtain the governing equation set as follows: These expressions can be extended to the three-dimensional (3D) case by 3D velocity potentials φu = a1(t)J0(kr)e−kz and φl = b1(t)J0(kr)ekz + b2(t)z, where the normal direction of bubble motion is the positive direction of the z axis, r is the polar coordinate, and J0(x) is the zero-order Bessel function.
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