Functions of State for Spinor Gas in General Relativity
arXiv:0711.1243 · doi:10.4236/oalib.1103953
Abstract
The energy momentum tensor of perfect fluid is a simplified but successful model in astrophysics. In this paper, assuming the particles driven by gravity and moving along geodesics, we derived the functions of state in detail. The results show that, these functions have a little correction for the usual thermodynamics. The new functions naturally satisfy the causal condition and consist with relativity. For the self potentials of the particles we introduce an extra function , which acts like negative pressure and can be used to describe dark matter. The results are helpful to understand the relation and interaction between space-time and matter.
13 pages, no figure. arXiv admin note: text overlap with arXiv:0708.2962
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