to the Rescue?

Furthermore we argue that this is the minimum kinetic mixing in any theory with hidden gauge interactions and charge sym- metry breaking in the dark sector.. The outline of this

The identity of the dark matter remains a mystery, the mass of the Higgs boson is difficult to explain, and different cosmological observations are not quite consistent. I

The code is intended to be used to simulate axion or fuzzy dark matter models where the evolution of the dark matter component is determined by a coupled Schrödinger-Poisson

More interestingly, in Paper I we showed that both the ro- tation curves of low surface brightness spiral galaxies and the matter profiles in clusters of galaxies, obtained using

Matter density perturbations and effective gravitational con- stant in modified gravity models of dark energy. Gauge Invariant

Coannihilations between the dark matter candidate and other BSM particles with masses within 10–20% of the DM mass can significantly increase the DM annihilation rates in the

Since the dark matter particle is expected to have a very small cross section when interacting with any SM particle it is expected to pass right through the detector.. At CERN they

We investigate a well known scenario of interaction in the dark sector where the vacuum energy is interacting with cold dark matter throughout the cosmic evolution in light of