Thermodynamical description of the interaction between holographic dark energy and dark matter

Bin Wang, Chi Yong Lin, Diego Pavón, Elcio Abdalla

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Resum

We present a thermodynamical description of the interaction between holographic dark energy and dark matter. If holographic dark energy and dark matter evolve separately, each of them remains in thermodynamic equilibrium. A small interaction between them may be viewed as a stable thermal fluctuation that brings a logarithmic correction to the equilibrium entropy. From this correction we obtain a physical expression for the interaction which is consistent with phenomenological descriptions and passes reasonably well the observational tests. © 2008 Elsevier B.V. All rights reserved.
Idioma originalAnglès
Pàgines (de-a)1-6
RevistaPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
Volum662
Número1
DOIs
Estat de la publicacióPublicada - 10 d’abr. 2008

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