Speaker
Prof.
ALAIN BLANCHARD
(IRAP , OMP)
Description
The Hubble tension, given the observed local measurement by SH0ES is known to be one of the major tension that the standard LCDM is facing. The recent results from Pantheon+ combined with the value inferred from SH0ES lead to a value of the reduced cosmological density parameter, $\omega_m$ that conflicts with the value inferred from the CMB for the LCDM model. However the situation does not really improve with alterative models twicked to solve the Hubble tension.
Author
Prof.
ALAIN BLANCHARD
(IRAP , OMP)
