1. Light magnetic dark matter in direct detection searches
- Author
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Paolo Panci, Jussi Virkajärvi, Chris Kouvaris, Eugenio Del Nobile, Francesco Sannino, Del Nobile, E., Kouvaris, C., Panci, P., Sannino, F., and Virkajarvi, J.
- Subjects
Particle physics ,Cosmology and Nongalactic Astrophysics (astro-ph.CO) ,dark matter detector ,Dark matter ,dark matter experiment ,FOS: Physical sciences ,chemistry.chemical_element ,Context (language use) ,Space (mathematics) ,Cross section (physics) ,High Energy Physics - Phenomenology (hep-ph) ,Xenon ,Thermal ,dark matter detectors ,dark matter experiments ,dark matter theory ,Mass parameter ,Physics ,Magnetic moment ,hep-ph ,Astronomy and Astrophysics ,High Energy Physics - Phenomenology ,chemistry ,astro-ph.CO ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We study a fermionic Dark Matter particle carrying magnetic dipole moment and analyze its impact on direct detection experiments. In particular we show that it can accommodate the DAMA, CoGeNT and CRESST experimental results. Assuming conservative bounds, this candidate is shown not to be ruled out by the CDMS, XENON and PICASSO experiments. We offer an analytic understanding of how the long-range interaction modifies the experimental allowed regions, in the cross section versus Dark Matter mass parameter space, with respect to the typically assumed contact interaction. Finally, in the context of a symmetric Dark Matter sector, we determine the associated thermal relic density, and further provide relevant constraints imposed by indirect searches and colliders., 32 pages, 5+1 figures; v2: matches version published on JCAP, dipole-dipole interaction added, discussion on its magnitude added in appendix, few typos corrected and some references added, results strengthened. arXiv admin note: text overlap with arXiv:1108.4661
- Published
- 2012
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