2025/04/10 by William J. Wolf, Wolf, William J., Carlos García-García +5 · 1 voice · 30 citations
Physics and Astronomy · #Cosmology and Gravitation Theories #Galaxies: Formation, Evolution, Phenomena #Dark Matter and Cosmic Phenomena
paper · pdf · doi:10.1103/jysf-k72m
The recent observational evidence of deviations from the Lambda cold dark matter model points toward the presence of evolving dark energy. The simplest possibility consists of a cosmological scalar field φ, dubbed "quintessence," driving the accelerated expansion. We assess the evidence for the existence of such a scalar field. We find that, if the accelerated expansion is driven by quintessence, the data favor a potential energy V(φ) that is concave, i.e., m2=d2V/dφ2<0. Furthermore, and more significantly, the data strongly favor a scalar field that is nonminimally coupled to gravity [Bayes factor log(B)=7.34±0.6], leading to time variations in the gravitational constant on cosmological scales, and the existence of fifth forces on smaller scales. The fact that we do not observe such fifth forces implies that either new physics must come into play on noncosmological scales or that quintessence is an unlikely explanation for the observed cosmic acceleration.