Speaker
Ms
Flor de María Lozano Rodríguez
(Universidad de Guanajuato)
Description
In this work, the structure formation for different modified gravity models will be described: Brans Dicke, $f(R)$, DGP, Symmetron. Such description is made through cosmological simulations carried out with the MG-PICOLA code that follows the COmoving Lagrangian Acceleration method. From them, the mass power spectrum is obtained, which we will compare with the resulting ones for the cosmological standard model $\Lambda$CDM.
Author
Ms
Flor de María Lozano Rodríguez
(Universidad de Guanajuato)
