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The Holographic Dark Energy in a Non-flat Universe

Qing-Guo Huang·Miao Li
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Abstract

We study the model for holographic dark energy in a spatially closed universe, generalizing the proposal in hep-th/0403127 for a flat universe. We provide independent arguments for the choice of the parameter $c=1$ in the holographic dark energy model. On the one hand, $c$ can not be less than 1, to avoid violating the second law of thermodynamics. On the other hand, observation suggests $c$ be very close to 1, it is hard to justify a small deviation of $c$ from 1, if $c>1$.

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Qing-Guo Huang, Miao Li. 2004-04-23. The Holographic Dark Energy in a Non-flat Universe. https://doi.org/10.1088/1475-7516%2F2004%2F08%2F013

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