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Le Châtelier–Braun principle in cosmological physics

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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.

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Authors and Affiliations

  1. Department of Physics, Autonomous University of Barcelona, 08193, Bellaterra, Spain

    Diego Pavón

  2. Department of Physics, Fudan University, 200433, Shanghai, China

    Bin Wang

Authors
  1. Diego Pavón
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  2. Bin Wang
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Correspondence to Diego Pavón.

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Pavón, D., Wang, B. Le Châtelier–Braun principle in cosmological physics. Gen Relativ Gravit 41, 1–5 (2009). https://doi.org/10.1007/s10714-008-0656-y

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  • DOI: https://doi.org/10.1007/s10714-008-0656-y

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