Weak Gravity Conjecture and Holographic Dark Energy Model with Interaction and Spatial Curvature

Details Weak Gravity Conjecture and Holographic Dark Energy Model with Interaction and Spatial Curvature Weak Gravity Conjecture and Holographic Dark Energy Model with Interaction and Spatial Curvature

2010-07-09

arxiv.org/abs/1007.1517v3

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

14 pages, 7 figures, typographical errors are corrected; conclusin is unchanged

Scientific paper

In the paper, we apply the weak gravity conjecture to the holographic quintessence model of dark energy. Three different holographic dark energy models are considered: without the interaction in the non-flat universe; with interaction in the flat universe; with interaction in the non-flat universe. We find that only in the models with the spatial curvature and interaction term proportional to the energy density of matter, it is possible for the weak gravity conjecture to be satisfied.

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