Speaker
José Halim Montes de Oca Yemha
(FESC-UNAM)
Description
In this study, we investigate Weakly Interacting Massive Particles as candidates for dark matter within an extended Standard Model framework that incorporates both scalar and fermion fields. We calculate the relic density and spin-independent scattering cross-section for these dark matter candidates and compare our results with the values reported by the PLANCK and XENON collaborations. Our results identify the parameter regions that are consistent with the observed constraints for the different dark matter candidates.
Authors
Estela Garcés
(FESC-UNAM)
Inti Ernesto Chavez Menez
(UNAM)
José Halim Montes de Oca Yemha
(FESC-UNAM)
