Three Paths to Particle Dark Matter

Probing the sub-GeV dark sector, neutrino-dark matter scattering and rare processes Importance & Status: New interactions of neutrinos with matter may alter the propagation

We mainly focus our analysis on probing the turbulence in the magnetised ionised ISM using Faraday rotation of pulsars, and dark matter in the Galaxy using a high-precision

The xenon target material is monitored for evidence of excess nuclear recoils that may be attributed to WIMP dark matter scattering, in particular for single scatter- ing

(15 more authors) (2012) Spin-dependent limits from the DRIFT-IId directional dark matter detector..

In section 3, we consider decaying WIMP DM models and use the IGRB spectrum along with minimal contributions to isotropic γ –ray flux from UHECR and unresolved point sources to

The differential event rate in Weakly Interacting Massive Particle (WIMP) direct detection exper- iments depends on the local dark matter density and velocity distribution..

Because the phase space integral in the thermal average for SIMP depends on the higher order of dark matter velocity than in the case of WIMP, SIMP case highly depends on the

If the density of dark matter/dark energy is uniform, ho- mogeneous and constant through the universe, and since the density is at the same order of the proton-nitron, then it