Shock propagation in a driven hard sphere gas: molecular dynamics simulations and hydrodynamics

Fuente: arXiv
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Main Authors: Kumar, Amit, Rajesh, R.
Format: Preprint
Published: 2024
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author Kumar, Amit
Rajesh, R.
author_facet Kumar, Amit
Rajesh, R.
contents The continuous injection of energy in a stationary gas creates a shock wave that propagates radially outwards. We study the hydrodynamics of this disturbance using event driven molecular dynamics of a hard sphere gas in two and three dimensions, the numerical solution of the Euler equation with a virial equation of state for the gas, and the numerical solution of the Navier-Stokes equation, for the cases when the driving is localised in space and when it is uniform throughout the shock. We show that the results from the Euler equation do not agree with the data from hard sphere simulations when the driving is uniform and has singularities when the driving is localised. Including dissipative terms through the Navier-Stokes equation results in reasonably good description of the data, when the coefficients of dissipation are chose parametrically.
format Preprint
id arxiv_https___arxiv_org_abs_2409_12086
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Shock propagation in a driven hard sphere gas: molecular dynamics simulations and hydrodynamics
Kumar, Amit
Rajesh, R.
Statistical Mechanics
Soft Condensed Matter
The continuous injection of energy in a stationary gas creates a shock wave that propagates radially outwards. We study the hydrodynamics of this disturbance using event driven molecular dynamics of a hard sphere gas in two and three dimensions, the numerical solution of the Euler equation with a virial equation of state for the gas, and the numerical solution of the Navier-Stokes equation, for the cases when the driving is localised in space and when it is uniform throughout the shock. We show that the results from the Euler equation do not agree with the data from hard sphere simulations when the driving is uniform and has singularities when the driving is localised. Including dissipative terms through the Navier-Stokes equation results in reasonably good description of the data, when the coefficients of dissipation are chose parametrically.
title Shock propagation in a driven hard sphere gas: molecular dynamics simulations and hydrodynamics
topic Statistical Mechanics
Soft Condensed Matter
url https://arxiv.org/abs/2409.12086