Prospects For Identifying Dark Matter With CoGeNT
arXiv:1011.3076 · doi:10.1088/1475-7516/2011/02/002
Abstract
It has previously been shown that the excess of events reported by the CoGeNT collaboration could be generated by elastically scattering dark matter particles with a mass of approximately 5-15 GeV. This mass range is very similar to that required to generate the annual modulation observed by DAMA/LIBRA and the gamma rays from the region surrounding the Galactic Center identified within the data of the Fermi Gamma Ray Space Telescope. To confidently conclude that CoGeNT's excess is the result of dark matter, however, further data will likely be needed. In this paper, we make projections for the first full year of CoGeNT data, and for its planned upgrade. Not only will this body of data more accurately constrain the spectrum of nuclear recoil events, and corresponding dark matter parameter space, but will also make it possible to identify seasonal variations in the rate. In particular, if the CoGeNT excess is the product of dark matter, then one year of CoGeNT data will likely reveal an annual modulation with a significance of 2-3. The planned CoGeNT upgrade will not only detect such an annual modulation with high significance, but will be capable of measuring the energy spectrum of the modulation amplitude. These measurements will be essential to irrefutably confirming a dark matter origin of these events.
6 pages, 6 figures
References in corpus (22)
- New results from DAMA/LIBRA
- Results from the Final Exposure of the CDMS II Experiment
- First Results from the XENON10 Dark Matter Experiment at the Gran Sasso National Laboratory
- The RAVE Survey: Constraining the Local Galactic Escape Speed
- First Dark Matter Results from the XENON100 Experiment
- Compatibility of DAMA/LIBRA dark matter detection with other searches
- Large-Mass Ultra-Low Noise Germanium Detectors: Performance and Applications in Neutrino and Astroparticle Physics
- CoGeNT Interpretations
- The Astrophysical Uncertainties Of Dark Matter Direct Detection Experiments
- Annual Modulation of Dark Matter in the Presence of Streams
- Implications of CoGeNT and DAMA for Light WIMP Dark Matter
- Model Independent Form Factors for Spin Independent Neutralino-Nucleon Scattering from Elastic Electron Scattering Data
- A Consistent Dark Matter Interpretation For CoGeNT and DAMA/LIBRA
- A light scalar WIMP through the Higgs portal and CoGeNT
- Constraints on inelastic dark matter from XENON10
- Low-threshold analysis of CDMS shallow-site data
- DAMA and WIMP dark matter
- New limits on spin-independent and spin-dependent couplings of low-mass WIMP dark matter with a germanium detector at a threshold of 220 eV
- Dependence of direct detection signals on the WIMP velocity distribution
- Compatibility of DAMA/LIBRA dark matter detection with other searches in light of new Galactic rotation velocity measurements
- A CoGeNT confirmation of the DAMA signal
- Design and Characterization of a Neutron Calibration Facility for the Study of sub-keV Nuclear Recoils
Cited by in corpus (14)
- Search for an Annual Modulation in a P-type Point Contact Germanium Dark Matter Detector
- The Dark Z' Portal: Direct, Indirect and Collider Searches
- Direct detection of dark matter in models with a light Z'
- Toward A Consistent Picture For CRESST, CoGeNT and DAMA
- On the DAMA and CoGeNT Modulations
- Implications of CoGeNT's New Results For Dark Matter
- A Leptophobic Z' And Dark Matter From Grand Unification
- A Two-Singlet Model for Light Cold Dark Matter
- Dark Forces At The Tevatron
- Probing dark matter streams with CoGeNT
- The Galactic Center Region Gamma Ray Excess from A Supersymmetric Leptophilic Higgs Model
- Evidence for dark matter modulation in CoGeNT?
- Constraining the Milky Way Dark Matter Density Profile with Gamma-Rays with Fermi-LAT
- Integrating In Dark Matter Astrophysics at Direct Detection Experiments