Rayleigh-Taylor instability at spherical interfaces between viscous fluids: Fluid/vacuum interface
Abstract
For a spherical interface of radius R separating two different homogeneous regions of incompressible viscous fluids under the action of a radially directed acceleration, we perform a linear stability analysis in terms of spherical surface harmonics Y n to derive the dispersion relation. The instability behavior is investigated by computing the growth rates and the most-unstable modes as a function of the spherical harmonic degree n. This general methodology is applicable to the entire parameter space spanned by the Atwood number, the viscosity ratio, and the dimensionless number B = (αRΡ²2/μ²²)¹/³ R (where αR, Ρ2 and μ2 are the local radial acceleration at the interface, and the density and viscosity of the denser overlying fluid, respectively). While the mathematical formulation here is general, this paper focuses on instability that arises at a spherical viscous fluid/vacuum interface as there is a great deal to be learned from the effects of one-fluid viscosity and sphericity alone. To quantify and understand the effect that curvature and radial accelerationhave on the Rayleigh-Taylor instability, a comparison of the growth rates, under homologous driving conditions, between the planar and spherical interfaces is performed. The derived dispersion relation for the planar interface accounts for an underlying finitemore »
- Authors:
-
- Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
- Publication Date:
- Research Org.:
- Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC). Basic Energy Sciences (BES); USDOE National Nuclear Security Administration (NNSA)
- OSTI Identifier:
- 1735910
- Alternate Identifier(s):
- OSTI ID: 1238594
- Report Number(s):
- LA-UR-20-24207; LA-UR-13-20570
Journal ID: ISSN 1070-6631; TRN: US2205267
- Grant/Contract Number:
- 89233218CNA000001; AC52-06NA25396
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physics of Fluids
- Additional Journal Information:
- Journal Volume: 27; Journal Issue: 5; Journal ID: ISSN 1070-6631
- Publisher:
- American Institute of Physics (AIP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; viscosity; perturbation theory; real analysis; flow instabilities; dispersion function; covariance and correlation; fluid mechanics; viscous liquid; Newtonian fluids; linear stability analysis
Citation Formats
Terrones, Guillermo, and Carrara, Mark D. Rayleigh-Taylor instability at spherical interfaces between viscous fluids: Fluid/vacuum interface. United States: N. p., 2015.
Web. doi:10.1063/1.4921648.
Terrones, Guillermo, & Carrara, Mark D. Rayleigh-Taylor instability at spherical interfaces between viscous fluids: Fluid/vacuum interface. United States. https://doi.org/10.1063/1.4921648
Terrones, Guillermo, and Carrara, Mark D. Fri .
"Rayleigh-Taylor instability at spherical interfaces between viscous fluids: Fluid/vacuum interface". United States. https://doi.org/10.1063/1.4921648. https://www.osti.gov/servlets/purl/1735910.
@article{osti_1735910,
title = {Rayleigh-Taylor instability at spherical interfaces between viscous fluids: Fluid/vacuum interface},
author = {Terrones, Guillermo and Carrara, Mark D.},
abstractNote = {For a spherical interface of radius R separating two different homogeneous regions of incompressible viscous fluids under the action of a radially directed acceleration, we perform a linear stability analysis in terms of spherical surface harmonics Y n to derive the dispersion relation. The instability behavior is investigated by computing the growth rates and the most-unstable modes as a function of the spherical harmonic degree n. This general methodology is applicable to the entire parameter space spanned by the Atwood number, the viscosity ratio, and the dimensionless number B = (αRΡ²2/μ²²)¹/³ R (where αR, Ρ2 and μ2 are the local radial acceleration at the interface, and the density and viscosity of the denser overlying fluid, respectively). While the mathematical formulation here is general, this paper focuses on instability that arises at a spherical viscous fluid/vacuum interface as there is a great deal to be learned from the effects of one-fluid viscosity and sphericity alone. To quantify and understand the effect that curvature and radial accelerationhave on the Rayleigh-Taylor instability, a comparison of the growth rates, under homologous driving conditions, between the planar and spherical interfaces is performed. The derived dispersion relation for the planar interface accounts for an underlying finite fluid region of thickness L and normal acceleration αR. Under certain conditions, the development of the most-unstable modes at a spherical interface can take place via the superposition of two adjacent spherical harmonics Yn and Yn+1. This bimodality in the evolution of disturbances in the linear regime does not have a counterpart in the planar configuration where the most-unstable modes are associated with a unique wave number.},
doi = {10.1063/1.4921648},
journal = {Physics of Fluids},
number = 5,
volume = 27,
place = {United States},
year = {Fri May 01 00:00:00 EDT 2015},
month = {Fri May 01 00:00:00 EDT 2015}
}
Web of Science
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Works referencing / citing this record:
Linear analysis on the interfacial instability of a spherical liquid droplet subject to a radial vibration
journal, October 2018
- Li, Yikai; Zhang, Peng; Kang, Ning
- Physics of Fluids, Vol. 30, Issue 10