CN-3.1 Simulating and understanding structure formation from galactic to cosmological scales for well-motivated DM models
CN-3.2 Cosmological precision probes of dark sectors on large scales
CN-3.3 Impact of DM density and velocity distribution in the local group and around SMBH on indirect and direct detection searches
CN-3.4 Dark energy perturbations via fully nonlinear hydrodynamics
CN-3.5 Probing neutrinos with cosmological and terrestrial experiments
CN-3.6 Light axions as DM candidates
