Similarity solutions for unsteady flow behind an exponential shock in an axisymmetric rotating non-ideal gas

DOI10.1007/s11012-015-0115-2zbMath1325.76112OpenAlexW2021110640MaRDI QIDQ890429

G. Nath

Publication date: 10 November 2015

Published in: Meccanica (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s11012-015-0115-2

zbMATH Keywords

shock wavesimilarity solutionsrotating mediumnon-ideal gasmechanics of fluidinterstellar mediumisothermal and adiabatic flows

Mathematics Subject Classification ID

Shock waves and blast waves in fluid mechanics (76L05) General theory of rotating fluids (76U05)

Related Items (10)

Propagation of an exponential shock wave in a rotational axisymmetric isothermal or adiabatic flow of a self-gravitating non-ideal gas under the influence of axial or azimuthal magnetic field ⋮ On the blast wave propagation and structure in a rotational axisymmetric perfect gas ⋮ Analytical solution for unsteady adiabatic flow behind the blast wave in a non-ideal gas and small inert solid particles mixture ⋮ Shock wave driven out by a piston in a mixture of a non-ideal gas and small solid particles under the influence of the gravitation field with monochromatic radiation ⋮ Self-similar solution for the flow behind an exponential shock wave in a rotational axisymmetric non-ideal gas with magnetic field ⋮ Exact similarity solution for the propagation of spherical shock wave in a Van der Waals gas with azimuthal magnetic field, radiation heat flux, radiation pressure and radiation energy under gravitational field ⋮ Magnetogasdynamic shock waves in non-ideal gas under gravitational field-isothermal flow ⋮ Flow behind an exponential shock wave in a rotational axisymmetric non-ideal gas with conduction and radiation heat flux ⋮ Similarity solutions for magnetogasdynamic shock waves in a rotating ideal gas using the Lie group-theoretic method ⋮ Similarity solutions for magnetogasdynamic cylindrical shock wave in rotating non-ideal gas using Lie group theoretic method

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