Functions of State for Spinor Gas in General Relativity

HTML  XML Download Download as PDF (Size: 442KB)  PP. 1-11  
DOI: 10.4236/oalib.1103953    414 Downloads   887 Views  Citations
Author(s)

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 W, 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.

Share and Cite:

Gu, Y. (2017) Functions of State for Spinor Gas in General Relativity. Open Access Library Journal, 4, 1-11. doi: 10.4236/oalib.1103953.

Copyright © 2024 by authors and Scientific Research Publishing Inc.

Creative Commons License

This work and the related PDF file are licensed under a Creative Commons Attribution 4.0 International License.