While observational evidence of the so-called Dark Matter anomaly is growing up with more and more sophisticated measurements, we observe that a pure non-collisional fluid in the central regions of the galactic halos, baryonic matter dominated, cannot explain naturally the observed dynamical features. it was observed surprisingly that the DM cores have substantial correlations with the...
As the WIMP draws under increasing tension thanks to the ever increasing sensitivity of direct detection experiments, the majority of dark matter parameter space outside of the weak scale remains unexplored. Molecular and nano-scale systems are particularly well-suited to look for sub-GeV DM since their eV-scale electronic transitions may be excited through light dark matter interactions....
The study of dark matter (DM) encompasses a wide range of models that have been extensively investigated using accelerators, underground detectors, and astroparticle physics experiments. While numerous approaches have been employed, high-energy astrophysical observations offer distinct advantages in unravelling the nature of DM candidates that are challenging to explore within laboratory...
