Le Châtelier–Braun principle in cosmological physics

By D. Pavón, Bin Wang. 2007

226 citations recorded by the source corpus.

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.

Subfields: Astronomy and Astrophysics, Statistical and Nonlinear Physics

View Paper: https://www.semanticscholar.org/paper/f5b672d85e073885ec6e690aef99dff4ed92928f