arXiv:2004.05049·v2·Cosmology and Nongalactic Astrophysics
The tension: vs.
Guillermo Ballesteros🇪🇸 · Alessio Notari🇪🇸 · Fabrizio Rompineve🇺🇸
Abstract
We investigate whether the tension on between SHES 2019 and Planck 2018 can be alleviated by a variation of Newton's constant between the early and the late Universe. This changes the Hubble rate before recombination, similarly to adding extra relativistic degrees of freedom. We implement a varying in a scalar-tensor theory of gravity, with a non-minimal coupling . If the scalar starts in the radiation era at an initial value and with , a dynamical transition occurs naturally around the epoch of matter-radiation equality and the field evolves towards zero at late times. As a consequence, the tension between SHES (2019) and Planck 2018+BAO slightly decreases, as in models, to the 3.8 level. We then perform a fit to a combined Planck, BAO and supernovae (SHES and Pantheon) dataset. When including local constraints on Post-Newtonian (PN) parameters, we find and a marginal improvement of compared to CDM, at the cost of 2 extra parameters. In order to take into account scenarios where local constraints could be evaded, we also perform a fit without PN constraints and find and a more significant improvement with 2 extra parameters. For comparison, we find that the model gives and at the cost of one extra parameter, which disfavors the CDM limit just above 2, since . Overall, our varying model performs similarly to the model in respect to the tension, if a physical mechanism to remove PN constraints can be implemented.
Comments: 20 pages, 7 figures. v2: Pantheon dataset added, additional new results for model without PN constraints, additional short discussion of S8. Version accepted for publication in JCAP