A Review of Macroscopic Motion in Thermodynamic Equilibrium
Juan R. Sanmartin

TL;DR
This review discusses the often-overlooked principle that macroscopic parts of an isolated system in thermodynamic equilibrium move collectively as a rigid body, with implications for space physics and different physical theories.
Contribution
It highlights a rarely discussed principle about macroscopic motion in equilibrium and explores its implications across various physical theories and space physics.
Findings
Macroscopic parts move as a rigid body in equilibrium
Dissipation increases internal energy and entropy
Different physics theories influence dissipation processes
Abstract
A principle on the macroscopic motion of systems in thermodynamic equilibrium, rarely discussed in texts, is reviewed: Very small but still macroscopic parts of a fully isolated system in thermal equilibrium move as if points of a rigid body, macroscopic energy being dissipated to increase internal energy, and increase entropy along. It appears particularly important in Space physics, when dissipation involves long-range fields at Electromagnetism and Gravitation, rather than short-range contact forces. It is shown how new physics, Special Relativity as regards Electromagnetism, first Newtonian theory then General Relativity as regards Gravitation, determine different dissipative processes involved in the approach to that equilibrium.
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Taxonomy
TopicsAdvanced Thermodynamics and Statistical Mechanics · Computational Physics and Python Applications
