Thermodynamical description of the interacting new agegraphic dark energy
A. Sheykhi, M. R. Setare
TL;DR
This paper explores the thermodynamical behavior of interacting new agegraphic dark energy and dark matter in a non-flat universe, linking their interaction to thermal fluctuations and equilibrium states.
Contribution
It provides a thermodynamical framework for understanding the interaction between dark energy and dark matter, incorporating stable thermal fluctuations.
Findings
Interaction affects thermodynamic equilibrium
Relation between interaction term and thermal fluctuation derived
Thermodynamical interpretation extends to non-flat universe
Abstract
We describe the thermodynamical interpretation of the interaction between new agegraphic dark energy and dark matter in a non-flat universe. When new agegraphic dark energy and dark matter evolve separately, each of them remains in thermodynamic equilibrium. As soon as an interaction between them is taken into account, their thermodynamical interpretation changes by a stable thermal fluctuation. We obtain a relation between the interaction term of the dark components and this thermal fluctuation.
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