In continuum mechanics, a branch of mathematics, the Burnett equations are a set of higher-order continuum equations for non-equilibrium flows and the transition regimes where the Navier–Stokes equations do not perform well.
[1][2][3] They were derived by the English mathematician D.
[4] The series expansion technique used to derive the Burnett equations involves expanding the distribution function
in the Boltzmann equation as a power series in the Knudsen number
represents the Maxwell-Boltzmann equilibrium distribution function, dependent on the number density
, macroscopic velocity
etc., are higher-order corrections that account for non-equilibrium effects, with each subsequent term incorporating higher powers of the Knudsen number
The first-order term
in the expansion gives the Navier-Stokes equations, which include terms for viscosity and thermal conductivity.
To obtain the Burnett equations, one must retain terms up to second order, corresponding to
The Burnett equations include additional second-order derivatives of velocity, temperature, and density, representing more subtle effects of non-equilibrium gas dynamics.
The Burnett equations can be expressed as:
higher-order terms
{\displaystyle \mathbf {u} _{t}+(\mathbf {u} \cdot \nabla )\mathbf {u} +\nabla p=\nabla \cdot (\nu \nabla \mathbf {u} )+{\text{higher-order terms}}}
Here, the "higher-order terms" involve second-order gradients of velocity and temperature, which are absent in the Navier-Stokes equations.
These terms become significant in situations with high Knudsen numbers, where the assumptions of the Navier-Stokes framework break down.
The Onsager-Burnett Equations, commonly referred to as OBurnett, which form a superset of the Navier-Stokes equations and are second-order accurate for Knudsen number.
τ
τ
τ
τ
d τ
τ (
d τ
( τ −
τ
τ
[6] Starting with the Boltzmann equation
This mathematics-related article is a stub.
You can help Wikipedia by expanding it.