Shock Waves
https://doi.org/10.1007/s00193-020-00972-x
ORIGINAL ARTICLE
Shock wave structure in non-ideal dilute gases under variable
Prandtl number
D. Khapra
1
· A. Patel
1
Received: 27 April 2020 / Revised: 4 September 2020 / Accepted: 13 September 2020
© Springer-Verlag GmbH Germany, part of Springer Nature 2020
Abstract
This paper investigates the structure of normal shock waves for a planar steady flow of non-ideal dilute gases under variable
viscosity and thermal conductivity using the Navier–Stokes–Fourier approach to the continuum model. The gas is assumed
to follow the simplified van der Waals equation of state along with the power-law temperature-dependent coefficients of
shear viscosity, bulk viscosity, and thermal conductivity. A closed system of nonlinear differential equations having a variable
Prandtl number (Pr) is formulated. Exact analytical solutions of the shock wave structure in non-ideal gases are derived
for Pr →∞ and Pr → 0 limits, and the corresponding profiles for velocity and temperature are obtained. For Pr → 0,
an isothermal shock is encountered for high Mach numbers. It appears sooner in non-ideal gases. The solution profiles for
Pr = 2/3 are obtained numerically and compared with the corresponding profiles for Pr → 0, 3/4, and ∞ under the same
initial conditions. Qualitative agreement is obtained with the theoretical and experimental results for the shock wave structure.
The inverse shock thickness is computed for different values of Pr, and it is found that the inverse shock thickness increases
with an increase in the Prandtl number. The bulk viscosity, the non-idealness parameter, the specific heat ratio, the power-law
index, and the pre-shock Mach number have a significant effect on the shock wave structure.
Keywords Shock wave · Navier–Stokes–Fourier model · Non-ideal gas · Prandtl number
1 Introduction
A shock wave is a transition zone across which the flow
variables such as velocity, density, pressure, temperature,
and entropy of the medium undergo a rapid change when
a pressure front moves at supersonic speed. When there are
no dissipative effects in the medium, such as viscosity and
heat conduction, this transition layer is very thin and is con-
sidered as a discontinuity surface. But in the presence of
viscosity and heat conduction, the thickness of the transi-
tion layer or shock wave is considerable and that requires
the mathematicians to investigate the internal structure of
shock waves. The internal structure of shock waves depends
on the inherent dynamics between momentum diffusion and
thermal diffusion. The ratio of momentum diffusion to ther-
mal diffusion during a thermo-physical process is defined
Communicated by D. Zeitoun.
B A. Patel
arvindpatelmath09@gmail.com
1
Department of Mathematics, University of Delhi, Delhi, India
as Prandtl number (Pr) [1]. It is a dimensionless number
depending only upon the characteristic of the fluid and was
introduced by Ludwig Prandtl around 1910. For air, at room
temperature, Pr = 0.71 and most common gases have similar
values. Small values of the Prandtl number (Pr ≪ 1) mean
that thermal diffusivity dominates, whereas large values
(Pr ≫ 1) imply that momentum diffusivity dominates the
behavior. Thus, Pr ≈ 0.02 for mercury means that in mer-
cury heat conduction is more pronounced than viscous effects
while oils generally have a large Prandtl number (≈ 10,000),
making convection the predominant means of transferring
energy as compared to pure conduction. Thus, taking Pr as a
variable, the shock wave structure for all fluids can be deter-
mined for a given equation of state.
Owing to the wide application of shock wave structure
in many physical problems such as molecular dissociation,
vibrational excitation, and high-temperature gas dynamics,
there has been a lot of experimental as well as theoretical
work done by mathematicians to study the internal structure
of shock waves. Riemann first introduced the fundamen-
tal concept of shock waves in the mid-nineteenth century.
Becker [2] provided an exact analytical solution for the pla-
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