Cosmic-ray antiproton constraints on light dark matter candidates
arXiv:1112.0678 · doi:10.1088/1742-6596/375/1/012032
Abstract
Some direct detection experiments have recently collected excess events that could be interpreted as a dark matter (DM) signal, pointing to particles in the 10 GeV mass range. We show that scenarios in which DM can self-annihilate with significant couplings to quarks are likely excluded by the cosmic-ray (CR) antiproton data, provided the annihilation is S-wave dominated when DM decouples in the early universe. These limits apply to most of supersymmetric candidates, eg in the minimal supersymmetric standard model (MSSM) and in the next-to-MSSM (NMSSM), and more generally to any thermal DM particle with hadronizing annihilation final states.
Contribution to the proceedings of TAUP-2011 (Munich, 5-9 IX 2011). 4 pages
References in corpus (8)
- Results from a Search for Light-Mass Dark Matter with a P-type Point Contact Germanium Detector
- Results from a Low-Energy Analysis of the CDMS II Germanium Data
- Galactic secondary positron flux at the Earth
- Updated CMB constraints on Dark Matter annihilation cross-sections
- New Limits on Dark Matter from Super-Kamiokande
- 10 GeV dark matter candidates and cosmic-ray antiprotons
- Cosmic-ray antiproton constraints on light singlino-like dark matter candidates
- Impact of the spectral hardening of TeV cosmic rays on the prediction of the secondary positron flux