A three-dimensional multidimensional gas-kinetic scheme for the Navier-Stokes equations under gravitational fields

TL;DR

This paper develops a multidimensional gas-kinetic scheme for the Navier-Stokes equations under gravitational fields, addressing key issues for well-balanced accuracy and validating it through numerical examples.

Contribution

It introduces a novel multidimensional gas-kinetic scheme incorporating gravitational source terms with second-order accuracy for the Navier-Stokes equations.

Findings

The scheme accurately models gas dynamics under gravity.

It maintains well-balanced properties and avoids artificial heating.

Numerical results agree with established methods.

Abstract

This paper extends the gas-kinetic scheme for one-dimensional inviscid shallow water equations (J. Comput. Phys. 178 (2002), pp. 533-562) to multidimensional gas dynamic equations under gravitational fields. Four important issues in the construction of a well-balanced scheme for gas dynamic equations are addressed. First, the inclusion of the gravitational source term into the flux function is necessary. Second, to achieve second-order accuracy of a well-balanced scheme, the Chapman-Enskog expansion of the Boltzmann equation with the inclusion of the external force term is used. Third, to avoid artificial heating in an isolated system under a gravitational field, the source term treatment inside each cell has to be evaluated consistently with the flux evaluation at the cell interface. Fourth, the multidimensional approach with the inclusion of tangential gradients in two-dimensional and three-dimensional cases becomes important in order to maintain the accuracy of the scheme. Many numerical examples are used to validate the above issues, which include the comparison between the solutions from the current scheme and the Strang splitting method. The methodology developed in this paper can also be applied to other systems, such as semi-conductor device simulations under electric fields.