The relativistic kinetic formalism revisited
Alfredo Sandoval-Villalbazo and
L.s Garcı́a-Colı́n
Physica A: Statistical Mechanics and its Applications, 2000, vol. 278, issue 3, 428-439
Abstract:
The relativistic Boltzmann equation is used to provide microscopical support to the relativistic Meixner–Prigogine scheme of linear irreversible thermodynamics. A suitable form of the chaotic velocities is employed in order to construct expressions for the total energy four-flux and the pressure tensor, a method that is not used in current approaches to the subject. The non-relativistic equations are shown to be satisfied within this formalism, and important cosmological implications of the theory, such as a modification of the expansion rate in Robertson–Walker–Friedman Universes are finally examined.
Date: 2000
References: View complete reference list from CitEc
Citations: View citations in EconPapers (1)
Downloads: (external link)
http://www.sciencedirect.com/science/article/pii/S037843719900607X
Full text for ScienceDirect subscribers only. Journal offers the option of making the article available online on Science direct for a fee of $3,000
Related works:
This item may be available elsewhere in EconPapers: Search for items with the same title.
Export reference: BibTeX
RIS (EndNote, ProCite, RefMan)
HTML/Text
Persistent link: https://EconPapers.repec.org/RePEc:eee:phsmap:v:278:y:2000:i:3:p:428-439
DOI: 10.1016/S0378-4371(99)00607-X
Access Statistics for this article
Physica A: Statistical Mechanics and its Applications is currently edited by K. A. Dawson, J. O. Indekeu, H.E. Stanley and C. Tsallis
More articles in Physica A: Statistical Mechanics and its Applications from Elsevier
Bibliographic data for series maintained by Catherine Liu ().