Similarity solution for a cylindrical shock wave in a rotational axisymmetric dusty gas with heat conduction and radiation heat flux

被引:30
作者
Vishwakarma, J. P. [1 ]
Nath, G. [2 ]
机构
[1] DDU Gorakhpur Univ, Dept Math & Stat, Gorakhpur 273009, Uttar Pradesh, India
[2] Natl Inst Technol Raipur, Dept Math, Raipur 492010, Madhya Pradesh, India
关键词
Self-similar solution; Rotating dusty gas; Conduction and radiation heat flux; Mechanics of fluids; SELF-SIMILAR SOLUTION; BLAST WAVES; PROPAGATION; FLOW; REFLECTION; MIXTURE;
D O I
10.1016/j.cnsns.2011.04.021
中图分类号
O29 [应用数学];
学科分类号
070104 ;
摘要
The propagation of shock waves in a rotational axisymmetric dusty gas with heat conduction and radiation heat flux, which has a variable azimuthally fluid velocity together with a variable axial fluid velocity, is investigated. The dusty gas is assumed to be a mixture of non-ideal (or perfect) gas and small solid particles, in which solid particles are continuously distributed. It is assumed that the equilibrium flow-condition is maintained and variable energy input is continuously supplied by the piston (or inner expanding surface). The fluid velocities in the ambient medium are assume to be vary and obey power laws. The density of the ambient medium is assumed to be constant, the heat conduction is express in terms of Fourier's law and the radiation is considered to be of the diffusion type for an optically thick grey gas model. The thermal conductivity K and the absorption coefficient x, ? are assumed to vary with temperature and density. In order to obtain the similarity solutions the angular velocity of the ambient medium is assume to be decreasing as the distance from the axis increases. The effects of the variation of the heat transfer parameter and non-idealness of the gas in the mixture are investigated. The effects of an increase in (i) the mass concentration of solid particles in the mixture and (ii) the ratio of the density of solid particles to the initial density of the gas on the flow variables are also investigated. (C) 2011 Elsevier B.V. All rights reserved.
引用
收藏
页码:154 / 169
页数:16
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