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.

6 pages, revtex file, no figures; version accepted for publication in General Relativity and Gravitation

References in corpus (10)

• Cosmology and the Fate of Dilatation Symmetry
• Interacting Dark Energy and Dark Matter: observational Constraints from Cosmological Parameters
• Testing the viability of the interacting holographic dark energy model by using combined observational constraints
• Thermodynamical description of the interaction between holographic dark energy and dark matter
• Holographic dark energy in Brans-Dicke theory
• Interacting holographic dark energy
• Matter density perturbations in interacting quintessence models
• Mass functions in coupled Dark Energy models
• Dark energy interacting with neutrinos and dark matter: a phenomenological theory
• Renormalization-group running cosmologies and the generalized second law

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