Magnetic Fluffy Dark Matter
arXiv:1111.2336 · doi:10.1007/JHEP02(2012)131
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 GeV and a constant splitting between successive states 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 GeV and 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
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