arXiv · 1905.02555
Testing the Swampland: $H_0$ tension
Abstract
The de Sitter Swampland conjecture compels us to consider dark energy models where $λ(ϕ) \equiv |\nabla_ϕ V|/V$ is bounded below by a positive constant. Moreover, it has been argued for Quintessence models that the constant $λ$ scenario is the least constrained. Here we demonstrate that increasing $λ$ only exacerbates existing tension in the Hubble constant $H_0$. The identification of dark energy models that both evade observational bounds and alleviate $H_0$ tension constitutes a robust test for the Swampland program.
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Eoin Ó Colgáin, Hossein Yavartanoo. 2019-09-20. Testing the Swampland: $H_0$ tension. https://arxiv.org/abs/1905.02555
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