Dynamic evolution of Rayleigh-Taylor bubbles from sinusoidal, W-shaped, and random perturbations

Zhi-Rui Zhou, You-Sheng Zhang, and Bao-Lin Tian
Phys. Rev. E 97, 033108 – Published 22 March 2018

Abstract

Implicit large eddy simulations of two-dimensional Rayleigh-Taylor instability at different density ratios (i.e., Atwood number A=0.05, 0.5, and 0.9) are conducted to investigate the late-time dynamics of bubbles. To produce a flow field full of bounded, semibounded, and chaotic bubbles, three problems with distinct perturbations are simulated: (I) periodic sinusoidal perturbation, (II) isolated W-shaped perturbation, and (III) random short-wave perturbations. The evolution of height h, velocity v, and diameter D of the (dominant) bubble with time t are formulated and analyzed. In problem I, during the quasisteady stage, the simulations confirm Goncharov's prediction of the terminal speed v=FrAgλ/(1+A), where Fr=1/3π. Moreover, the diameter D at this stage is found to be proportional to the initial perturbation wavelength λ as Dλ. This differed from Daly's simulation result of D=λ(1+A)/2. In problem II, a W-shaped perturbation is designed to produce a bubble environment similar to that of chaotic bubbles in problem III. We obtain a similar terminal speed relationship as above, but Fr is replaced by Frw0.63. In problem III, the simulations show that h grows quadratically with the bubble acceleration constant αh/(Agt2)0.05, and D expands self-similarly with a steady aspect ratio βD/h(1+A)/2, which differs from existing theories. Therefore, following the mechanism of self-similar growth, we derive a relationship of β=4α(1+A)/Frw2 to relate the evolution of chaotic bubbles in problem III to that of semibounded bubbles in problem II. The validity of this relationship highlights the fact that the dynamics of chaotic bubbles in problem III are similar to the semibounded isolated bubbles in problem II, but not to that of bounded periodic bubbles in problem I.

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  • Received 29 November 2017
  • Revised 8 February 2018

DOI:https://doi.org/10.1103/PhysRevE.97.033108

©2018 American Physical Society

Physics Subject Headings (PhySH)

Fluid Dynamics

Authors & Affiliations

Zhi-Rui Zhou1, You-Sheng Zhang1,2,*, and Bao-Lin Tian1,2,†

  • 1Institute of Applied Physics and Computational Mathematics, Beijing 100094, China
  • 2Center for Applied Physics and Technology, Peking University, Beijing 100871, China

  • *zhang_yousheng@iapcm.ac.cn
  • tian_baolin@iapcm.ac.cn

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Issue

Vol. 97, Iss. 3 — March 2018

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