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Burnett Coefficients

  When we wish to generalize the linear constitutive relations, swarm theories and dense fluid theories depart rapidly from each other. The most obvious way to generalize the Newtonian constitutive relation is to write the viscous pressure tensor as    an arbitrary analytic function of the strain rate:

 

Here is a rank six tensor that is clearly symmetric with respect to interchanges of the and , and of the and indices. An arbitrary isotropic rank tensor has 15 independent components [Eu [1979]] , which is reduced to 7 components when the above symmetries are taken into account (see Appendix gif).If we further suppose that the fluid is monatomic, then must be symmetric, and the number of independent components reduces to 5, of which two are diagonal in the first two indices, and three are traceless. So at second order in the strain rate, there are five transport coefficients, two of which refer to bulk properties, and the   other three which describe shearing properties. Similarly, at the next order in strain rate, there will be 22 transport coefficients.

      Burnett [1935] developed a form of hydrodynamics that was more accurate than Navier-Stokes hydrodynamics by applying the Chapman-Enskog procedure to the Boltzmann equation. [See Chapter 7 and 15 of Chapman and Cowling

[1970] for a discussion] . This introduced 19 transport coefficients of which the 8 bulk coefficients are zero for a dilute gas. This left 6 coefficients for the correction to the viscous pressure tensor, and 5 for the thermal flux term. The constitutive relation   (gif) refers to a situation where there are no thermal or pressure gradients, and so the three shear components of can be identified with the remaining three Burnett coefficients in equation (15.3,8) of Chapman and Cowling [1970]. More will be said of the non-linear Burnett coefficients in chapter   gif, where tractable expressions are developed relating the coefficients to equilibrium correlation functions.

The generalization of the constitutive relation (gif) for swarms is different in that linearity in the swarm density must   be preserved:

Here the generalized transport coefficients are rank l tensors, and indicates the -fold scalar product.

A fully consistent derivation of this relation based on a Chapman-Enskog-like solution of the linear Boltzmann equation can   be found in Kumar et al. [1980]. It is thought that the higher order transport coefficients , with   , play a role only where the density gradients are not small, such as near the boundary of the apparatus containing the swarm. However, at large density gradients, this whole approach is doubtful, as non physical behaviour results [see

[1974]] . Analogous problems occur with Burnett and Super-Burnett level hydrodynamics in the theory of neutral gases [see [1983]] .    More will be discussed on the subject of higher-order transport coefficients in chapter gif, where certain experimental effects can be explained in terms of these coefficients.



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Next: Boltzmann Equation Up: Introduction Previous: Constitutive Relations



Russell Standish
Thu May 18 11:43:52 EST 1995