Dark energy and the refined de sitter conjecture

Dark energy and the refined de sitter conjecture

Blog Article

Abstract We revisit the phenomenology of quintessence models in light of the recently refined version of the de Sitter Swampland conjecture, which includes the possibility of unstable de Sitter critical points.We show that models of quintessence Non-communicable diseases and its risk factors among the transgender population in Kerala: a cross-sectional study can evade previously derived lower bounds on (1 + w), albeit with very finely-tuned initial conditions.In the absence of such Rethinking Potentials of Public Space and its Management Through Placemaking in Kuala Lumpur tuning or other rolling quintessence fields, a field with mass close to Hubble is required, which has a generic prediction for (1+ w).Slow-roll single field inflation models remain in tension.Other phenomenological constraints arising from the coupling of the quintessence field with the Higgs or the QCD axion are significantly relaxed.