Journal
JOURNAL OF HIGH ENERGY PHYSICS
Volume -, Issue 2, Pages -Publisher
SPRINGER
DOI: 10.1007/JHEP02(2012)131
Keywords
Beyond Standard Model; Technicolor and Composite Models
Categories
Funding
- NSF [PHY05-51164, PHY-0970171]
- DOE [DE-FG02-94ER40840]
- DOE at University of Oregon [DE-FG02-96ER40969]
- Direct For Mathematical & Physical Scien
- Division Of Physics [0970171] Funding Source: National Science Foundation
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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(x) similar to O(1-100) GeV and a constant splitting between successive states delta similar to 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(x) similar to 11GeV and delta < 15ke Vis allowed by all the present direct detection constrain
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