Improved Constraints on Inelastic Dark Matter
arXiv:0907.3940 · doi:10.1088/1475-7516/2009/09/010
Abstract
We perform an extensive study of the DAMA annual modulation data in the context of inelastic dark matter. We find that inelastic dark matter with mass m > 15 GeV is excluded at the 95% confidence level by the combination of DAMA spectral information and results from other direct detection experiments. However, at smaller m, inelastic dark matter constitutes a possible solution to the DAMA puzzle.
22 pages, 7 figures, Reference added, matches published version
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Cited by in corpus (34)
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- The Astrophysical Uncertainties Of Dark Matter Direct Detection Experiments
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- Capture of Inelastic Dark Matter in White Dwarves
- Global interpretation of direct Dark Matter searches after CDMS-II results
- Resolving astrophysical uncertainties in dark matter direct detection
- Effect of low mass dark matter particles on the Sun
- On the DAMA and CoGeNT Modulations
- Form Factor Dark Matter
- Exothermic Double-Disk Dark Matter
- New Limits on Dark Matter from Super-Kamiokande
- Halo-independent methods for inelastic dark matter scattering
- Resonant Dark Matter
- Implications on Inelastic Dark Matter from 100 Live Days of XENON100 Data
- The Cosmology of Composite Inelastic Dark Matter
- Neutrino-Flavoured Sneutrino Dark Matter
- Limits on inelastic dark matter from ZEPLIN-III
- AMEND: A Model Explaining Neutrino masses and Dark matter testable at the LHC and MEG
- Impure Thoughts on Inelastic Dark Matter
- A Warped Model of Dark Matter
- Decaying into the Hidden Sector
- Direct Detection of Dynamical Dark Matter
- Tools for Studying Low-Mass Dark Matter at Neutrino Detectors
- Nearly Supersymmetric Dark Atoms
- Revising inelastic dark matter direct detection by including the cosmic ray acceleration
- Parity Violation in Composite Inelastic Dark Matter Models
- The Poker Face of Inelastic Dark Matter: Prospects at Upcoming Direct Detection Experiments
- Disentangling Dark Matter Dynamics with Directional Detection
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- Peaked Signals from Dark Matter Velocity Structures in Direct Detection Experiments
- Magnetic Inelastic Dark Matter: Directional Signals Without a Directional Detector
- Studies of a three-stage dark matter and neutrino observatory based on multi-ton combinations of liquid xenon and liquid argon detectors
- TeV Scale Neutrino Mass Generation, Minimal Inelastic Dark Matter, and High Scale Leptogenesis
- Model-Independent Identification of Inelastic WIMPs from Direct Dark Matter Detection Experiments