Toward a consistent picture for CRESST, CoGeNT, and DAMA

Abstract

Three dark matter direct detection experiments (DAMA/LIBRA, CoGeNT, and CRESST-II) have each reported signals which are not consistent with known backgrounds, but resemble that predicted for a dark matter particle with a mass of roughly $\ensuremath{\sim}10\text{ }\text{ }\mathrm{GeV}$ and an elastic scattering cross section with nucleons of $\ensuremath{\sim}{10}^{\ensuremath{-}41}--{10}^{\ensuremath{-}40}\text{ }\text{ }{\mathrm{cm}}^{2}$. In this article, we compare the signals of these experiments and discuss whether they can be explained by a single species of dark matter particle, without conflicting with the constraints of other experiments. We find that the spectrum of events reported by CoGeNT and CRESST-II are consistent with each other and with the constraints from CDMS-II, although some tension with xenon-based experiments remains. Similarly, the modulation signals reported by DAMA/LIBRA and CoGeNT appear to be compatible, although the corresponding amplitude of the observed modulations are a factor of at least a few higher than would be naively expected, based on the event spectra reported by CoGeNT and CRESST-II. This apparent discrepancy could potentially be resolved if tidal streams or other non-Maxwellian structures are present in the local distribution of dark matter.