Shock wave kinematics in interstellar gas clouds with dust particles
- Swati Chauhan,
- Antim Chauhan,
- Rajan Arora
Swati Chauhan
Indian Institute of Technology Roorkee
Corresponding Author:sswati2325iitr@gmail.com
Author ProfileAbstract
In this article, a system of partial differential equations governing
the one-dimensional motion of an inviscid gas with solid dust particles
is considered. The evolutionary behavior of cylindrical and spherical
shock waves in dusty gas is determined. To accomplish this, we used a
technique that is based on the kinematics of the one-dimensional motion
of shock waves. This allowed us to derive an infinite hierarchy of
transport equations that describe the strength of shock waves and the
induced discontinuity behind them. These equations are used to determine
both the decay and growth behaviors of shock waves in dusty gas.
Considering the first two truncation approximations, the results so
obtained are compared with the results obtained by Guderley's exact
solution and CCW approximation.