Université de Montpellier
Tuesday, November 17, 2020
*Please note special time of 10:00 am
I introduce the audience to the gross features of primordial magnetic field evolution before recombination. Then, I will show how primordial magnetic fields can help relieve the Hubble tension. Permitting time, I will finally make some general statements about a large number of beyond LambdaCDM models proposed to solve the Hubble tension and why they usually do not completely achieve this goal.