Orateur
ALAIN BLANCHARD
(IRAP , OMP)
Description
The tension on the Hubble constant can be reformulated as a tension on the matter density parameter $\omega_M$. This has the advantage that $\omega_M$ is more directly connected to the CMB-derived parameters, unlike the Huble constant. With the recent DESI measurement, the tensoin is raised up to over6 $\sigma$, stronger than the tension on the Hubble constant.
Auteur principal
ALAIN BLANCHARD
(IRAP , OMP)
