(1) Presentation(s)
Jeu. 25/03/2021 14:00 webinaire ACHITOUV Ixandra (LUTh Meudon) Probing cosmology with the growth rate of cosmic structures (LUPM/Particules, Astroparticules, Cosmologie : Théorie) The growth rate of cosmic structures is a key quantity to probe gravitational interactions and dark energy. In the late-time Universe the growth rate becomes non-linear, making it more difficult to probe, but also makes it in principle a source of additional cosmological information than its linear counterpart. Pour plus d'informations, merci de contacter Lavalle J. |