Inelastic dark matter with spin-dependent couplings to protons and large modulation fractions in DAMA
arXiv:1512.00593 · doi:10.1088/1475-7516/2016/02/050
Abstract
We discuss a scenario where the DAMA modulation effect is explained by a Weakly Interacting Massive Particle (WIMP) which upscatters inelastically to a heavier state and predominantly couples to the spin of protons. In this scenario constraints from xenon and germanium targets are evaded dynamically, due to the suppression of the WIMP coupling to neutrons, while those from fluorine targets are evaded kinematically, because the minimal WIMP incoming speed required to trigger upscatters off fluorine exceeds the maximal WIMP velocity in the Galaxy, or is very close to it. In this scenario WIMP scatterings off sodium are usually sensitive to the large-speed tail of the WIMP velocity distribution and modulated fractions of the signal close to unity arise in a natural way. On the other hand, a halo-independent analysis with more conservative assumptions about the WIMP velocity distribution allows to extend the viable parameter space to configurations where large modulated fractions are not strictly necessary. We discuss large modulated fractions in the Maxwellian case showing that they imply a departure from the usual cosine time dependence of the expected signal in DAMA. However we explicitly show that the DAMA data is not sensitive to this distortion, both in time and frequency space, even in the extreme case of a 100 % modulated fraction. Moreover the same scenario provides an explanation of the maximum in the energy spectrum of the modulation amplitude detected by DAMA in terms of WIMPs whose minimal incoming speed matches the kinematic threshold for inelastic upscatters. For the elastic case the detection of such maximum suggests an inversion of the modulation phase below the present DAMA energy threshold, while this is not expected for inelastic scattering. This may allow to discriminate between the two scenarios in a future low-threshold analysis of the DAMA data.
28 pages, 11 figures, updated to published version
References in corpus (21)
- Dark Matter Results from 225 Live Days of XENON100 Data
- New results from DAMA/LIBRA
- The RAVE Survey: Constraining the Local Galactic Escape Speed
- Search for Low-Mass WIMPs with SuperCDMS
- Results from a Low-Energy Analysis of the CDMS II Germanium Data
- Improved Limits on Scattering of Weakly Interacting Massive Particles from Reanalysis of 2013 LUX data
- First dark matter search results from a 4-kg CFI bubble chamber operated in a deep underground site
- Dark Matter Search Results from the PICO-2L CF Bubble Chamber
- Constraints on Low-Mass WIMP Interactions on 19F from PICASSO
- Phase-space structure in the local dark matter distribution and its signature in direct detection experiments
- New Limits on Interactions between Weakly Interacting Massive Particles and Nucleons Obtained with CsI(Tl) Crystal Detectors
- Improved dark matter search results from PICO-2L Run 2
- Not so Coy Dark Matter explains DAMA (and the Galactic Center excess)
- Improved WIMP-search reach of the CDMS II germanium data
- Search for Low-Mass Dark Matter with CsI(Tl) Crystal Detectors
- Reevaluation of spin-dependent WIMP-proton interactions as an explanation of the DAMA data
- A systematic halo-independent analysis of direct detection data within the framework of Inelastic Dark Matter
- Generalized spin-dependent WIMP-nucleus interactions and the DAMA modulation effect
- Is the effect of the Sun's gravitational potential on dark matter particles observable?
- Gravitational Focusing and Substructure Effects on the Rate Modulation in Direct Dark Matter Searches
- Effective scalar four-fermion interaction for Ge-phobic exothermic dark matter and the CDMS-II Silicon excess
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- Probing DAMA/LIBRA in the full parameter space of WIMP effective models of inelastic scattering
- Halo-independent determination of the unmodulated WIMP signal in DAMA: the isotropic case
- New constraints on inelastic dark matter from IceCube
- Proton-philic spin-dependent inelastic Dark Matter (pSIDM) as a viable explanation of DAMA/LIBRA-phase2
- TeV Scale Neutrino Mass Generation, Minimal Inelastic Dark Matter, and High Scale Leptogenesis
- The effect of hydrodynamical simulation inspired dark matter velocity profile on directional detection of dark matter
- From direct detection to relic abundance: the case of proton-philic spin-dependent inelastic Dark Matter
- Constraints on inelastic dark matter from the CDEX-1B experiment
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