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• W2972256775 endingPage "134907" @default.
• W2972256775 startingPage "134907" @default.
• W2972256775 abstract "The de Sitter Swampland conjecture compels us to consider dark energy models where λ(ϕ)≡|∇ϕV|/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 H0. The identification of dark energy models that both evade observational bounds and alleviate H0 tension constitutes a robust test for the Swampland program." @default.
• W2972256775 created "2019-09-12" @default.
• W2972256775 creator A5028386025 @default.
• W2972256775 creator A5083324083 @default.
• W2972256775 date "2019-10-01" @default.
• W2972256775 modified "2023-10-18" @default.
• W2972256775 title "Testing the Swampland: H0 tension" @default.
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• W2972256775 doi "https://doi.org/10.1016/j.physletb.2019.134907" @default.
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