Burnett equations

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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. Burnett.[4]

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Series expansion

Series expansion approach

The series expansion technique used to derive the Burnett equations involves expanding the distribution function f in the Boltzmann equation as a power series in the Knudsen number Kn:

f(r,c,t)=f(0)(c|n,u,T)[1+Knϕ(1)(c|n,u,T)+Kn2ϕ(2)(c|n,u,T)+]

Here, f(0)(c|n,u,T) represents the Maxwell-Boltzmann equilibrium distribution function, dependent on the number density n, macroscopic velocity u, and temperature T. The terms ϕ(1),ϕ(2), etc., are higher-order corrections that account for non-equilibrium effects, with each subsequent term incorporating higher powers of the Knudsen number Kn.

Derivation

The first-order term f(1) 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 ϕ(2). 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:

𝐮t+(𝐮)𝐮+p=(ν𝐮)+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.

Extensions

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.[5]

Eq. (1) τdusds98α1u*(du*ds)2=τu*τ01+u*

Eq. (2) 4516τdτds+94γ1τ(du*ds)294Ψu*dτdsdu*ds=32(ττ0)12(1u*)2τ0(1u*)[6]

Derivation

Template:Expand section Starting with the Boltzmann equation ft+ckfxk+Fkfck=J(f,f1)

See also

References

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Further reading

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