Magnetic Fluffy Dark Matter

Abstract

We explore extensions of inelastic Dark Matter and Magnetic inelastic Dark Matter where the WIMP can scatter to a tower of heavier states. We assume a WIMP mass $m_{\ddot{I}}‡\sim \mathcal{O}(1-100)$ GeV and a constant splitting between successive states $\hat{I}´\sim \mathcal{O}(1-100)$ keV. For the spin-independent scattering scenario we find that the direct experiments CDMS and XENON strongly constrain most of the DAMA/LIBRA preferred parameter space, while for WIMPs that interact with nuclei via their magnetic moment a region of parameter space corresponding to $m_{\ddot{I}}‡\sim 11$ GeV and $\hat{I}´<15$ keV is allowed by all the present direct detection constraints.

16 pages, 6 figures, added comments about magnetic moment form factor to Sec 3.1.2 and results to Sec 3.2.2, final version to be published in JHEP