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Title: Relaxation time approximation for relativistic dense matter

Journal Article · · Physical Review, D (Particles Fields); (United States)
; ; ;  [1]
  1. Departement d'Astrophysique Relativiste et de Cosmologie, Observatoire de Meudon, 92190 Meudon (France)

In this article the relaxation time approximation for a system of spin-1/2 fermions is studied with a view to calculating those transport properties obeyed by relativistic dense matter such as viscosity coefficients, thermal conductivities, spin diffusion, etc. This is achieved {ital via} the use of covariant Wigner functions. The collision term is, of course, linear in the deviation of the Wigner function from equilibrium, and {ital a} priori involves arbitrary functions of the four-momentum. These functions are restricted from physical arguments and from the requirement of Lorentz invariance. The kinetic equation obeyed by the Wigner function is then split into a mass-shell constraint and true'' kinetic equations, whose solution is sought within the Chapman-Enskog approximation. It is also realized that, in a relativistic quantum framework, there exist {ital two} expansion parameters: the new parameter occurs because of the existence of a new length scale defined by the Compton wavelength; in some cases (e.g., when the effective mass of the fermions goes to zero), this last quantity can be of the order of the mean free path. From the first-order solutions and from the Landau-Lifshitz matching conditions, the main transport properties of the system are obtained as functions of the macroscopic quantities (temperature, density, polarization) {ital and} of various relaxation times to be determined elsewhere by a specific physical model. Finally, all the results obtained are discussed and suggestions for some extensions are given.

OSTI ID:
7030237
Journal Information:
Physical Review, D (Particles Fields); (United States), Vol. 46:10; ISSN 0556-2821
Country of Publication:
United States
Language:
English