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Le Chatelier-Braun principle in cosmological physics

Diego Pavon, Bin Wang

Abstract

Assuming that dark energy may be treated as a fluid with a well defined temperature, close to equilibrium, we argue that if nowadays there is a transfer of energy between dark energy and dark matter, it must be such that the latter gains energy from the former and not the other way around.

Le Chatelier-Braun principle in cosmological physics

Abstract

Assuming that dark energy may be treated as a fluid with a well defined temperature, close to equilibrium, we argue that if nowadays there is a transfer of energy between dark energy and dark matter, it must be such that the latter gains energy from the former and not the other way around.

Paper Structure

This paper contains 7 equations.