Kinematics of spherical shock waves in an interstellar ideal gas clouds with dust particles

Author(s):  
Antim Chauhan ◽  
Rajan Arora
2021 ◽  
Vol 0 (0) ◽  
Author(s):  
Swati Chauhan ◽  
Antim Chauhan ◽  
Rajan Arora

Abstract In this work, we consider the system of partial differential equations describing one-dimensional (1D) radially symmetric (i.e., cylindrical or spherical) flow of a nonideal gas with small solid dust particles. We analyze the implosion of cylindrical and spherical symmetric strong shock waves in a mixture of a nonideal gas with small solid dust particles. An evolution equation for the strong cylindrical and spherical shock waves is derived by using the Maslov technique based on the kinematics of 1D motion. The approximate value of the similarity exponent describing the behavior of strong shocks is calculated by applying a first-order truncation approximation. The obtained approximate values of similarity exponent are compared with the values of the similarity exponent obtained from Whitham’s rule and Guderley’s method. All the above computations are performed for the different values of mass fraction of dust particles, relative specific heat, and the ratio of the density of dust particle to the density of the mixture and van der Waals excluded volume.


AIAA Journal ◽  
2001 ◽  
Vol 39 (5) ◽  
pp. 969-971 ◽  
Author(s):  
F. Aizik ◽  
G. Ben-Dor ◽  
T. Elperin ◽  
O. Igra

2010 ◽  
Vol 22 (11) ◽  
pp. 116102 ◽  
Author(s):  
Malte Kjellander ◽  
Nils Tillmark ◽  
Nicholas Apazidis

Sign in / Sign up

Export Citation Format

Share Document