Functions of State for Spinor Gas in General Relativity

TL;DR

This paper derives detailed state functions for a spinor gas in general relativity, revealing slight thermodynamic corrections and introducing a potential function that models dark matter, enhancing understanding of space-time and matter interactions.

Contribution

It provides a new derivation of state functions for spinor gases in general relativity, including a potential function for dark matter, with implications for astrophysics and cosmology.

Findings

State functions have slight thermodynamic corrections.

Introduces a potential function W acting like negative pressure.

Results satisfy causality and are consistent with relativity.

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.