@article {
author = {Bajargaan, R. and Patel, A.},
title = {Similarity Solution for a Cylindrical Shock Wave in a Self-gravitating, Rotating Axisymmetric Dusty Gas with Heat Conduction and Radiation Heat Flux},
journal = {Journal of Applied Fluid Mechanics},
volume = {10},
number = {1},
pages = {329-341},
year = {2017},
publisher = {},
issn = {1735-3572},
eissn = {1735-3645},
doi = {10.18869/acadpub.jafm.73.238.25679},
abstract = {Similarity solutions are obtained for unsteady adiabatic propagation of a cylindrical shock wave in a self gravitating, rotating, axisymmetric dusty gas with heat conduction and radiation heat flux in which variable energy input is continuously supplied by the piston. The dusty gas is taken to be a mixture of non-ideal gas and small solid particles. Azimuthal fluid velocity and axial fluid velocity in the ambient medium are taken to be variable. The equilibrium flow conditions are assumed to be maintained. The initial density is assumed to be constant. The heat conduction is expressed in terms of Fourierâ€™s law and the radiation is taken to be of the diffusion type for an optically thick grey gas model. The thermal conductivity and the absorption coefficient are assumed to vary with temperature and density. The effects of the variation of the gravitational parameter and the heat transfer parameters on the shock strength and the flow variables such as radial velocity, azimuthal velocity, axial velocity, density, pressure, total heat flux, mass behind the shock front, azimuthal vorticity vector, axial vorticity vector, isothermal speed of sound and adiabatic compressibility are studied. It is found that the presence of gravitation effect in the medium modify the radiation and conduction effect on the flow variables.},
keywords = {Self similar solution,Shock wave,Dusty gas,Self gravitation,Conduction and radiation heat flux},
url = {https://www.jafmonline.net/article_432.html},
eprint = {https://www.jafmonline.net/article_432_89292fb92b7264edc3ad7fea6b0d9ec5.pdf}
}