Table of Contents
Fetching ...

Gravitational Equilibrium with Steady Flow and Relativistic Local Thermodynamics

Shuichi Yokoyama

TL;DR

The paper addresses how to define thermodynamic observables and derive consistent structure equations for a self-gravitating relativistic system with steady radial flow and spherical symmetry. It develops a framework that combines a current-carrying energy-momentum tensor with an off-diagonal metric component, analyzed in an instantaneous rest frame to extract geometric thermodynamic quantities that transform correctly to the moving frame. It presents extended structure equations that generalize the TOV equation to include radial flow and anisotropic pressure, and derives exact GR Poisson and heat-conduction relations tied to the local thermodynamics of the flowing system. This work provides a rigorous method to model steady energy transport in relativistic contexts and clarifies how local thermodynamics, gravity, and flow interrelate in non-static backgrounds.

Abstract

A relativistic self-gravitating equilibrium system with steady flow as well as spherical symmetry is discovered. The energy-momentum tensor contains the contribution of a current related to the flow and the metric tensor does an off-diagonal component to balance with the flow momentum. The presence of the off-diagonal component of the metric implies the radial motion of the reference frame, which gives rise to a problem how the relativistic effect is included in thermodynamic observables for such a general relativistic system. This problem is solved by taking an instantaneously rest frame in which geometric thermodynamic observables read as previously and giving them the special relativistic effect emerged from the inverse transformation to the original frame pointwise. The solution of the thermodynamic observables in accord with the laws of thermodynamics and the theory of relativity is presented. Finally the relativistic structure equations for the equilibrium are derived, from which the general relativistic Poisson equation as well as the heat conduction one are developed exactly.

Gravitational Equilibrium with Steady Flow and Relativistic Local Thermodynamics

TL;DR

The paper addresses how to define thermodynamic observables and derive consistent structure equations for a self-gravitating relativistic system with steady radial flow and spherical symmetry. It develops a framework that combines a current-carrying energy-momentum tensor with an off-diagonal metric component, analyzed in an instantaneous rest frame to extract geometric thermodynamic quantities that transform correctly to the moving frame. It presents extended structure equations that generalize the TOV equation to include radial flow and anisotropic pressure, and derives exact GR Poisson and heat-conduction relations tied to the local thermodynamics of the flowing system. This work provides a rigorous method to model steady energy transport in relativistic contexts and clarifies how local thermodynamics, gravity, and flow interrelate in non-static backgrounds.

Abstract

A relativistic self-gravitating equilibrium system with steady flow as well as spherical symmetry is discovered. The energy-momentum tensor contains the contribution of a current related to the flow and the metric tensor does an off-diagonal component to balance with the flow momentum. The presence of the off-diagonal component of the metric implies the radial motion of the reference frame, which gives rise to a problem how the relativistic effect is included in thermodynamic observables for such a general relativistic system. This problem is solved by taking an instantaneously rest frame in which geometric thermodynamic observables read as previously and giving them the special relativistic effect emerged from the inverse transformation to the original frame pointwise. The solution of the thermodynamic observables in accord with the laws of thermodynamics and the theory of relativity is presented. Finally the relativistic structure equations for the equilibrium are derived, from which the general relativistic Poisson equation as well as the heat conduction one are developed exactly.

Paper Structure

This paper contains 6 sections, 14 equations.