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2024

Scant evidence for thawing quintessence

Wolf, William J., García-García, Carlos, Bartlett, Deaglan J. et al.

Understand

New constraints on the expansion rate of the Universe seem to favor evolving dark energy in the form of thawing quintessence models, i.e., models for which a canonical, minimally coupled scalar field has, at late times, begun to evolve away from potential energy domination.

We scrutinize the evidence for thawing quintessence by exploring what it predicts for the equation of state.
We show that, in terms of the usual Chevalier-Polarski-Linder parameters, ($w_0$, $w_a$), thawing quintessence is, in fact, only marginally consistent with a compilation of the current data.
Despite this, we embrace the possibility that thawing quintessence is dark energy and find constraints on the microphysics of this scenario.