Extensions of the standard model are studied to explain the origin of the matter-antimatter asymmetry observed in the Universe, as well as its possible implications for experiments.
Search for candidates for the bulk of the non-luminous matter in the Universe. Theoretical study of different models providing dark matter candidates and their signals in direct or indirect detection experiments, as well as in cosmological observables.
Statistics of galaxy distribution and measurement of baryon acoustic oscillations.
Global analysis of data from solar, atmospheric, reactor and accelerator neutrino experiments. Experimental consequences of the existence of non-standard interactions. Neutrinos as probes in astrophysics (Sun, supernovae) and cosmology (CMB, LSS), neutrino astronomy.
Measurements of cosmic microwave radiation, the large-scale structure of the Universe and the abundance of light elements allow valuable information to be extracted about neutrinos and other relics of the Big Bang, which may be related to dark matter and dark energy.
We construct and analyse the phenomenological consequences of theoretical models that solve some open problems of the Standard Model, for example the nature of dark matter. In particular supersymmetric models.
