Hostname: page-component-cd9895bd7-jn8rn Total loading time: 0 Render date: 2024-12-12T12:31:16.198Z Has data issue: false hasContentIssue false

Analytical model of nonlinear evolution of single-mode Rayleigh–Taylor instability in cylindrical geometry

Published online by Cambridge University Press:  06 August 2020

Zhiye Zhao
Affiliation:
Department of Modern Mechanics, University of Science and Technology of China, Hefei, Anhui230026, PR China Institute of Applied Physics and Computational Mathematics, Beijing10094, PR China
Pei Wang
Affiliation:
Institute of Applied Physics and Computational Mathematics, Beijing10094, PR China
Nansheng Liu
Affiliation:
Department of Modern Mechanics, University of Science and Technology of China, Hefei, Anhui230026, PR China
Xiyun Lu*
Affiliation:
Department of Modern Mechanics, University of Science and Technology of China, Hefei, Anhui230026, PR China State Key Laboratory of Fire Science, University of Science and Technology of China, Hefei, Anhui230026, PR China
*
Email address for correspondence: xlu@ustc.edu.cn

Abstract

We present an analytical model of nonlinear evolution of two-dimensional single-mode Rayleigh–Taylor instability (RTI) in cylindrical geometry at arbitrary Atwood number for the first time. Our model covers a full scenario of bubble evolution from the earlier exponential growth to the nonlinear regime with the bubbles growing in time as $\frac {1}{2}a_{b}t^2$ for cylindrical RTI, other than as $V_{b}t$ for planar RTI, where $a_{b}$ and $V_{b}$ are the bubble acceleration and velocity, respectively. It is found that from this model the saturating acceleration $a_{b}$ is formulated as a simplified function of the external acceleration, Atwood number and number of perturbation waves. This model's predictions are in good agreement with data from direct numerical simulations.

Type
JFM Papers
Copyright
© The Author(s), 2020. Published by Cambridge University Press

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

REFERENCES

Annamalai, S., Parmar, M. K., Ling, Y. & Balachandar, S. 2014 Nonlinear Rayleigh–Taylor instability of a cylindrical interface in explosion flows. Trans. ASME: J. Fluids Engng 136 (6), 060910.Google Scholar
Besnard, D. 2007 The megajoule laser program-ignition at hand. Eur. Phys. J. D 44, 207213.CrossRefGoogle Scholar
Bian, X., Aluie, H., Zhao, D.-X., Zhang, H.-S. & Livescu, D. 2020 Revisiting the late-time growth of single-mode Rayleigh–Taylor instability and the role of vorticity. Physica D 403, 132250.CrossRefGoogle Scholar
Bodner, S. E., Colombant, D. G., Gardner, J. H., Lehmberg, R. H., Obenschain, S. P., Phillips, L., Schmitt, A. J., Sethian, J. D., McCrory, R. L., Seka, W. & others 1998 Direct-drive laser fusion: status and prospects. Phys. Plasmas 5, 19011918.CrossRefGoogle Scholar
Boffetta, G. & Mazzino, A. 2017 Incompressible Rayleigh–Taylor turbulence. Annu. Rev. Fluid Mech. 49, 119143.CrossRefGoogle Scholar
Caproni, A., Lanfranchi, G. A., da Silva, A. L. & Falceta-Gonçalves, D. 2015 Three-dimensional hydrodynamical simulations of the supernovae-driven gas loss in the dwarf spheroidal galaxy URSA minor. Astrophys. J. 805, 109120.CrossRefGoogle Scholar
Chambers, K. & Forbes, L. K. 2012 The cylindrical magnetic Rayleigh–Taylor instability for viscous fluids. Phys. Plasmas 19 (10), 102111.CrossRefGoogle Scholar
Chertkov, M. 2003 Phenomenology of Rayleigh–Taylor turbulence. Phys. Rev. Lett. 91 (11), 115001.CrossRefGoogle ScholarPubMed
Epstein, R. 2004 On the Bell–Plesset effects: the effects of uniform compression and geometrical convergence on the classical Rayleigh–Taylor instability. Phys. Plasmas 11 (11), 51145124.CrossRefGoogle Scholar
Forbes, L. K. 2011 A cylindrical Rayleigh–Taylor instability: radial outflow from pipes or stars. J. Engng Maths 70 (1-3), 205224.CrossRefGoogle Scholar
Gamezo, V. N., Khokhlov, A. M., Oran, E. S., Chtchelkanova, A. Y. & Rosenberg, R. O. 2003 Thermonuclear supernovae: simulations of the deflagration stage and their implications. Science 299 (5603), 7781.CrossRefGoogle ScholarPubMed
Glimm, J., Grove, J. & Zhang, Y.-M. 1999 Numerical calculation of Rayleigh–Taylor and Richtmyer–Meshkov instabilities for three dimensional axi-symmetric flows in cylindrical and spherical geometries. Preprint, SUNY at Stony Brook.Google Scholar
Goncharov, V. N. 2002 Analytical model of nonlinear, single-mode, classical Rayleigh–Taylor instability at arbitrary Atwood numbers. Phys. Rev. Lett. 88 (13), 134502.CrossRefGoogle ScholarPubMed
Guo, H.-Y., Wang, L.-F., Ye, W.-H., Wu, J.-F. & Zhang, W.-Y. 2018 Weakly nonlinear Rayleigh–Taylor instability in cylindrically convergent geometry. Chin. Phys. Lett. 35 (5), 055201.CrossRefGoogle Scholar
Hsing, W. W., Barnes, C. W., Beck, J. B., Hoffman, N. M., Galmiche, D., Richard, A., Edwards, J., Graham, P., Rothman, S. & Thomas, B. 1997 Rayleigh–Taylor instability evolution in ablatively driven cylindrical implosions. Phys. Plasmas 4 (5), 18321840.CrossRefGoogle Scholar
Hu, Z.-X., Zhang, Y.-S., Tian, B.-L., He, Z.-W. & Li, L. 2019 Effect of viscosity on two-dimensional single-mode Rayleigh–Taylor instability during and after the reacceleration stage. Phys. Fluids 31 (10), 104108.Google Scholar
Jiang, G.-S. & Shu, C.-W. 1996 Efficient implementation of weighted ENO schemes. J. Comput. Phys. 126, 202228.CrossRefGoogle Scholar
Joggerst, C. C., Nelson, A., Woodward, P., Lovekin, C., Masser, T., Fryer, C. L., Ramaprabhu, P., Francois, M. & Rockefeller, G. 2014 Cross-code comparisons of mixing during the implosion of dense cylindrical and spherical shells. J. Comput. Phys. 275, 154173.CrossRefGoogle Scholar
Kord, A. & Capecelatro, J. 2019 Optimal perturbations for controlling the growth of a Rayleigh–Taylor instability. J. Fluid Mech. 876, 150185.CrossRefGoogle Scholar
Layzer, D. 1955 On the instability of superposed fluids in a gravitational field. Astrophys. J. 122, 112.CrossRefGoogle Scholar
Li, H.-F., He, Z.-W., Zhang, Y.-S. & Tian, B.-L. 2019 On the role of rarefaction/compression waves in Richtmyer–Meshkov instability with reshock. Phys. Fluids 31 (5), 054102.Google Scholar
Lombardini, M., Pullin, D. I. & Meiron, D. I. 2014 Turbulent mixing driven by spherical implosions. Part 1. Flow description and mixing-layer growth. J. Fluid Mech. 748, 85112.CrossRefGoogle Scholar
Luo, T.-F., Wang, J.-C., Xie, C.-Y., Wan, M.-P. & Chen, S.-Y. 2020 Effects of compressibility and Atwood number on the single-mode Rayleigh–Taylor instability. Phys. Fluids 32 (1), 012110.Google Scholar
Mikaelian, K. O. 1998 Analytic approach to nonlinear Rayleigh–Taylor and Richtmyer–Meshkov instabilities. Phys. Rev. Lett. 80 (3), 508511.CrossRefGoogle Scholar
Mikaelian, K. O. 2003 Explicit expressions for the evolution of single-mode Rayleigh–Taylor and Richtmyer–Meshkov instabilities at arbitrary Atwood numbers. Phys. Rev. E 67 (2), 026319.CrossRefGoogle ScholarPubMed
Mikaelian, K. O. 2005 Rayleigh–Taylor and Richtmyer–Meshkov instabilities and mixing in stratified cylindrical shells. Phys. Fluids 17 (9), 094105.CrossRefGoogle Scholar
Morgan, B. E. & Greenough, J. A. 2016 Large-eddy and unsteady RANS simulations of a shock-accelerated heavy gas cylinder. Shock Waves 26 (4), 355383.CrossRefGoogle Scholar
Nuckolls, J., Wood, L., Thiessen, A. & Zimmerman, G. 1972 Laser compression of matter to super-high densities: thermonuclear (CTR) applications. Nature 239 (5368), 139142.CrossRefGoogle Scholar
Rayleigh, Lord 1900 Investigation of the character of the equilibrium of an incompressible heavy fluid of variable density. Scientific Papers 200207, vol. II. Cambridge University Press.Google Scholar
Sohn, S.-I. 2003 Simple potential-flow model of Rayleigh–Taylor and Richtmyer–Meshkov instabilities for all density ratios. Phys. Rev. E 67 (2), 026301.CrossRefGoogle ScholarPubMed
Taylor, G. I. 1950 The instability of liquid surfaces when accelerated in a direction perpendicular to their planes. I. Proc. R. Soc. Lond. A 201 (1065), 192196.Google Scholar
Wang, L.-F., Wu, J.-F., Ye, W.-H., Zhang, W.-Y. & He, X.-T. 2013 Weakly nonlinear incompressible Rayleigh–Taylor instability growth at cylindrically convergent interfaces. Phys. Plasmas 20 (4), 042708.Google Scholar
Weir, S. T., Chandler, E. A. & Goodwin, B. T. 1998 Rayleigh–Taylor instability experiments examining feedthrough growth in an incompressible, convergent geometry. Phys. Rev. Lett. 80 (17), 37633766.CrossRefGoogle Scholar
Wieland, S. A., Hamlington, P. E., Reckinger, S. J. & Livescu, D. 2019 Effects of isothermal stratification strength on vorticity dynamics for single-mode compressible Rayleigh–Taylor instability. Phys. Rev. Fluids 4 (9), 093905.CrossRefGoogle Scholar
Xie, C.-Y., Tao, J.-J., Sun, Z.-L. & Li, J. 2017 Retarding viscous Rayleigh–Taylor mixing by an optimized additional mode. Phys. Rev. E 95 (2), 023109.CrossRefGoogle ScholarPubMed
Yu, H.-D. & Livescu, D. 2008 Rayleigh–Taylor instability in cylindrical geometry with compressible fluids. Phys. Fluids 20 (10), 104103.CrossRefGoogle Scholar
Zhang, Q. 1998 Analytical solutions of layzer-type approach to unstable interfacial fluid mixing. Phys. Rev. Lett. 81 (16), 33913394.CrossRefGoogle Scholar
Zhang, Q. & Graham, M. J. 1998 A numerical study of Richtmyer–Meshkov instability driven by cylindrical shocks. Phys. Fluids 10 (4), 974992.CrossRefGoogle Scholar
Zhang, Q. & Guo, W.-X. 2016 Universality of finger growth in two-dimensional Rayleigh–Taylor and Richtmyer–Meshkov instabilities with all density ratios. J. Fluid Mech. 786, 4761.CrossRefGoogle Scholar
Zhao, K.-G., Xue, C., Wang, L.-F., Ye, W.-H., Wu, J.-F., Ding, Y.-K., Zhang, W.-Y. & He, X.-T. 2018 Thin shell model for the nonlinear fluid instability of cylindrical shells. Phys. Plasmas 25 (9), 092703.Google Scholar
Zhou, Y. 2017 a Rayleigh–Taylor and Richtmyer–Meshkov instability induced flow, turbulence, and mixing. I. Phys. Rep. 720, 1136.Google Scholar
Zhou, Y. 2017 b Rayleigh–Taylor and Richtmyer–Meshkov instability induced flow, turbulence, and mixing. II. Phys. Rep. 723, 1160.Google Scholar