Holographic dark energy and late cosmic acceleration
Diego Pavon

TL;DR
This paper proposes a holographic dark energy model based on the holographic principle, explaining the universe's late acceleration and addressing the coincidence problem, with implications for non-flat cosmologies.
Contribution
It introduces a holographic dark energy model that accounts for cosmic acceleration and alleviates the coincidence problem, extending to non-flat universes.
Findings
The model explains late cosmic acceleration.
It alleviates the coincidence problem.
Comments on a late transition to deceleration.
Abstract
It has been persuasively argued that the number of the effective degrees of freedom of a macroscopic system is proportional to its area rather than to its volume. This entails interesting consequences for cosmology. Here we present a model based on this "holographic principle" that accounts for the present stage of accelerated expansion of the Universe and significantly alleviates the coincidence problem also for non-spatially flat cosmologies. Likewise, we comment on a recently proposed late transition to a fresh decelerated phase.
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