Relaxation time approximation for relativistic dense matter
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...
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Published in: | Physical review. D, Particles and fields Vol. 46; no. 10; pp. 4603 - 4629 |
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Main Authors: | , , , |
Format: | Journal Article |
Language: | English |
Published: |
Ridge, NY
American Physical Society
15-11-1992
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Subjects: | |
Online Access: | Get full text |
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Summary: | 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. |
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Bibliography: | ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 None |
ISSN: | 0556-2821 1089-4918 |
DOI: | 10.1103/PhysRevD.46.4603 |