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Constitutive Relations

The non-equilibrium part of the pressure tensor is called the viscous pressure tensor  

Two centuries ago Newton realised that , which is zero at equilibrium, can be driven by the strain rate tensor . For atomic fluids close to equilibrium, the most general linear relation between the viscous pressure tensor and the strain rate tensor is

 

The fourth rank transport tensor is a function of the thermodynamic state of the system . It is independent of the strain rate . In fluids with no external field applied, must be isotropic, i.e. rotationally invariant.

There are three independent isotropic rank four tensors, [see Temple [1960]] defined by the possible multilinear invariants of four vectors , , and :

In atomic fluids, the force acting between atoms is parallel to the displacement between the atoms, i.e. a central force. This implies that P

is symmetricgif, and so (gif) becomes

where is the shear viscosity and is the     bulk viscosity. In molecular fluids, the intermolecular forces do not necessarily act parallel to the displacement between the molecules and the pressure is not necessarily symmetric, so a further term, vortex viscosity [de Groot and Mazur

[1962]] must be introduced.

The continuity relation (gif) gives an exact relationship between the velocity field and the pressure tensor. The Newtonian constitutive relation gives a relation   between the pressure tensor and the velocity field which is a good approximation for fluids close to equilibrium. By combining the continuity and Newtonian constitutive relations, we obtain the Navier-Stokes   equation of hydrodynamics:

In swarm physics, the only conserved quantity is mass (or equivalently charge), and even then only in the absence of reactions. The mass continuity equation is (gif) with an additional term of on the right hand side representing the net production of swarm particles due to reactions with the background gas. A momentum continuity equation would need to take into account the dynamics of the background gas, and so is not a useful relation for the theory. In this case, the constitutive relation must contain a constant term representing the average streaming velocity due to the electric field, as well as the term proportional to the gradient of :

 

Upon substituting (gif) into (gif), we obtain the diffusion equation:  

 

  The transport coefficients , and can be identified with the reaction rate , the system drift velocity and the coefficient of diffusion respectively. In free space, the transport coefficients of the swarm must satisfy   cylindrical symmetry with the major axis in the direction of the electric field. The only vectors with this property must be proportional to the electric field , and that any second rank tensor must be a linear combination of the unit tensor, and of the dyad . This means that the transport coefficients can be represented by three parameters: the drift   velocity and the two components of the diffusion coefficient, namely that which is aligned   with the field, , and that which is transverse to the field . We have . An alternative parameter to the drift velocity is the mobility:  



next up previous contents index
Next: Burnett Coefficients Up: Introduction Previous: Continuity Relations



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