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The effect of the magnetic field on the Rayleigh-Taylor instability in a couple-stress fluid

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Języki publikacji
EN
Abstrakty
EN
In this study we examine the effect of the magnetic field parameter on the growth rate of the Rayleigh-Taylor instability (RTI) in a couple stress fluids. A simple theory based on fully developed flow approximations is used to derive the dispersion relation for the growth rate of the RTI. The general dispersion relation obtained using perturbation equations with appropriate boundary conditions will be reduced for the special cases of propagation and the condition of instability and stability will be obtained. In solving the problem of the R-T instability the appropriate boundary conditions will be applied. The couple-stress parameter is found to be stabilizing and the influence of the various parameters involved in the problem on the interface stability is thoroughly analyzed. The new results will be obtained by plotting the curves between the dimensionless growth rate and the dimensionless wave number for various physical parameters involved in the problem (viz. the magnetic field, couple-stress, porosity, etc.) in the problem. It is found that the magnetic field and couple-stress have a stabilization effect whereas the buoyancy force (surface tension) has a destabilization effect on the RT instability in the presence of porous media.
Rocznik
Strony
611--622
Opis fizyczny
Bibliogr. 17 poz., wykr.
Twórcy
  • Department of Mathematics, S.S. Government First Grade College Nargund, INDIA
autor
  • Department of Mathematics, Rani Channamma University Belgaum, INDIA
  • Department of Mathematics, Government College Gulbarga - 585105, Karnataka, INDIA
autor
  • K.L.E’s Dr. M. S. Sheshagiri College of Engineering and Technology Belgaum, INDIA
Bibliografia
  • [1] Shilling O., Steinkamp M. and Baer M. (2006): Turbulent Mixing and Hydrodnamics. – Predictive Science Academic Alliances Program Technical White Paper.
  • [2] Sharp D.H. (1984): An overview of Rayleigh-Taylor instability. – Physica D 12, pp.3-18.
  • [3] Rayleigh L. (1883): On the stability or instability of certain fluid motion. – Proc. Lond. Math., Soc., vol.11, No.57.
  • [4] Taylor G.I. (1950): The instability of liquid surfaces when accelerated in a direction perpendicular to their planes I. – Proc. Roy. Soc. London, Ser. A201, pp.192-196.
  • [5] Chandrasekhar S. (1961): Hydrodynamic and Hydromagnetic Stability. – New York: Dover Publications.
  • [6] Bhatia P.K. (1974): Rayleigh-Taylor instability of two viscous superposed conducting fluids. – Nuovo Cim. 19B, pp.161-168.
  • [7] Sharma R.C. and Sharma K.C. (1978): Rayleigh-Taylor instability of two superposed conducting fluids in the presence of suspended particles. – Acta. Physica Hungarica 45, pp.213-220.
  • [8] Stokes V.K. (1966): Couple stresses in Fluids. – Phys. Fluids, vol.9, pp.1709-1715.
  • [9] Sinha P., Singh P.C. and Prasad K.R. (1981): Couple stresses in journal bearings lubricants and the effect of cavitation. – Wear, vol.67, No.1, pp.15-24.
  • [10] Bujurke N.M. and Jayaraman G. (1982): The influence of couple stresses in squeeze films. – Int. J. Mech. Sci., vol.24, pp.369-376.
  • [11] Walicki E. and Walicka A. (1999): Inertia effect in the squeeze film of a couple-stress fluid in biological bearings. – Appl. Mech. Engg., vol.4, No.2, pp.363-373.
  • [12] Sunil, Sharma R.C. and Chandel R.S. (2002): On superposed fluids in porous medium in hydrodynamics. – Z. Naturforsch, 57a, pp.955-960.
  • [13] Chavaraddi K.B., Awati V.B. and Gouder P.M. (2013): Effect Boundary Roughness on Rayleigh-Taylor Instability of a Couple-Stress Fluid. – Gen. Math. Notes, vol.17, No.2, pp.66-75.
  • [14] Srinivasan B., Dimonte G. and Tang X.-Z. (2012): Magnetic field generation in Rayleigh-Taylor unstable inertial confinement fusion plasmas. – Phys. Rev. Lett. 108, 165002.
  • [15] Srinivasan B. and Tang X.-Z. (2012): Mechanism for magnetic field generation and growth in Rayleigh-Taylor unstable inertial confinement fusion plasmas. – Phys. Plasmas 19, 082703.
  • [16] Modica F., Plewa T. and Zhiglo A. (2013): The Braginskii model of the Rayleigh--Taylor instability. I. Effects of self-generated magnetic fields and thermal conduction in two dimensions. – High Energy Density Phys., vol.9, pp.767-780.
  • [17] Alves E.P., Grismayer T., Martins S.F., Fiza F., Fonseca R.A. and Silva L.O. (2012): Large-scale magnetic field generation via the kinetic Kelvin-Helmholtz instability in unmagnetized scenarios. – Astrophys. J. Lett. 746:L14.
Uwagi
PL
Opracowanie rekordu w ramach umowy 509/P-DUN/2018 ze środków MNiSW przeznaczonych na działalność upowszechniającą naukę (2019)
Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-de2eccf7-8b84-4af4-8876-d7e7cfbd9cff
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