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Le Châtelier-Braun principle in cosmological physics. (English) Zbl 1162.83375
Summary: 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.
MSC:
83F05Relativistic cosmology
83C55Macroscopic interaction of the gravitational field with matter (general relativity)
80A10Classical thermodynamics, including relativistic
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