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arXiv · hep-th/0410017

Dark Entropy: Holographic Cosmic Acceleration

Eric V. Linder
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Abstract

In cosmic holography, the fundamental quantity is the degrees of freedom on a horizon surface rather than the material contents within the volume. That is, the horizon area and hence cosmological expansion rate H is related to the entropy. Using this as a guide, we examine the consequences of an effective dark {\it entropy} on the past and future dynamics of the universe. The results, including nonmonotonic expansion behavior, are interesting apart from the theoretical motivation.

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Eric V. Linder. 2004-10-01. Dark Entropy: Holographic Cosmic Acceleration. https://arxiv.org/abs/hep-th/0410017

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