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

Cheng-Yi Sun
2011 Communications in Theoretical Physics  

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2010 pre-print arXiv:1007.1517v1 fatcat:mpjwqudeyvdqllue2famqejs7i

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2010 pre-print
arXiv:1007.1517v2 fatcat:ny6d6zjjojcwhlaaiyazxpgiaa
2010 accepted
arXiv:1007.1517v3 fatcat:itwie6ycsnhkpddfxyoruzt6tm
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.
doi:10.1088/0253-6102/56/1/33 fatcat:qa2ylqypyngyzb455bvxuhyxjq
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Cheng-Yi Sun. "Weak Gravity Conjecture and Holographic Dark Energy Model with Interaction and Spatial Curvature." Communications in Theoretical Physics 56.1 (2011) 193-198