Abstract Views :526 |
PDF Views:4
Authors
Affiliations
1 Department of Mathematics, Gauhati University, Guwahati-781014, IN
Source
International Journal of Fluids Engineering, Vol 5, No 1 (2013), Pagination: 39-55
Abstract
The effects of Hall current and radiation on unsteady MHD free convective visco-elastic flow past an infinite vertical porous plate in presence of heat and mass transfer subjected to wall slip condition have been analyzed analytically. The highly non-linear equations are solved analytically by using multi parameter perturbation technique. The expressions for velocity field, temperature field, shearing stress and rate of heat transfer as well as mass transfer have been obtained. To study the visco-elastic effects with the combination of other flow parameters, the velocity and shearing stress have been illustrated graphically with physical interpretation.
Keywords
Free Convection, Radiation, Perturbation Scheme, Walters Liquid (model B’).
References
- Sato H., J. Phys. Soc. Japan, Vol.16, pp1427, 1961.
- Sherman A. and Sutton G.W., Engineering magnetohydrodynamic, New York, McGraw-Hill, 1965.
- Beard D.W. & Walters K, Pro Cambridge Philo Soc. Math Phys Sci, Vol.60, pp 667, 1964.
- Katagiri M.J., Phys Soc Japan, Vol.27, pp 1051, 1969.
- Pop I., J. Math. Phys. Sci., Vol.5, pp 375, 1971
- Raptis A., Ram P.C., Astrophys. Space Sci., Vol.106, pp 257, 1984
- Attia H.A., Canadian J. Phys, Vol.76 (9), pp 739, 1998.
- Biswal S., Sahoo P.K., Proc. Natl. Acad. Sci India, Vol. 69 A (1), 45-57, 1999
- Takhar H.S., Chamkha A.J., Nath G., Int. J. Eng. Sci. Vol. 40,pp 1511, 2002.
- Attia H.A., Canadian J. Phys, Vol. 82(2), pp 127. 2004.
- Kumar R., Chand K., Int. J. Eng. Sc. Tech., Vol.3(4), pp 3124,2011.
- Singh K.D., Kumar R., Int. J. Appl. Maths. Mech., Vol. 6 (13), pp 28,2010.
- Raju M.C., Reddy N.A., Verma S.V.K., thermal science, Vol. 15(2),pp 527, 2011.
- Ahmed N., Kalita D., J. Energy Heat mass transfer, Vol.33, pp 271-29, 2011.
- Choudhury R., Das S.K., IOSR Journal of Mathematics, Vol. 5(1), pp 20, 2013.
