Closing in on mass-degenerate dark matter scenarios with antiprotons and direct detection
arXiv:1207.1431 · doi:10.1088/1475-7516/2012/11/017
Abstract
Over the last years both cosmic-ray antiproton measurements and direct dark matter searches have proved particularly effective in constraining the nature of dark matter candidates. The present work focusses on these two types of constraints in a minimal framework which features a Majorana fermion as the dark matter particle and a scalar that mediates the coupling to quarks. Considering a wide range of coupling schemes, we derive antiproton and direct detection constraints using the latest data and paying close attention to astrophysical and nuclear uncertainties. Both signals are strongly enhanced in the presence of degenerate dark matter and scalar masses, but we show that the effect is especially dramatic in direct detection. Accordingly, the latest direct detection limits take the lead over antiprotons. We find that antiproton and direct detection data set stringent lower limits on the mass splitting, reaching 19% at a 300 GeV dark matter mass for a unity coupling. Interestingly, these limits are orthogonal to ongoing collider searches at the Large Hadron Collider, making it feasible to close in on degenerate dark matter scenarios within the next years.
14 pages, 6 figures
References in corpus (33)
- Dark Matter Results from 225 Live Days of XENON100 Data
- Trigonometric Parallaxes of Massive Star Forming Regions: VI. Galactic Structure, Fundamental Parameters and Non-Circular Motions
- First results from DAMA/LIBRA and the combined results with DAMA/NaI
- New results from DAMA/LIBRA
- Results from a Search for Light-Mass Dark Matter with a P-type Point Contact Germanium Detector
- The Milky Way's Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars
- The RAVE Survey: Constraining the Local Galactic Escape Speed
- Results from a Low-Energy Analysis of the CDMS II Germanium Data
- The redshift dependence of the structure of massive LCDM halos
- First Dark Matter Results from the XENON100 Experiment
- Hadronic Uncertainties in the Elastic Scattering of Supersymmetric Dark Matter
- The DAMA/LIBRA apparatus
- Indirect search for dark matter with micrOMEGAs2.4
- Weak Corrections are Relevant for Dark Matter Indirect Detection
- On the local dark matter density
- First dark matter search results from a 4-kg CFI bubble chamber operated in a deep underground site
- New Gamma-Ray Contributions to Supersymmetric Dark Matter Annihilation
- Constraints on WIMP Dark Matter from the High Energy PAMELA data
- Galactic masers and the Milky Way circular velocity
- Improved Limits on Spin-Dependent WIMP-Proton Interactions from a Two Liter CFI Bubble Chamber
- A Consistent Dark Matter Interpretation For CoGeNT and DAMA/LIBRA
- The Dark Matter at the End of the Galaxy
- Gluon contribution to the dark matter direct detection
- The galactic antiproton spectrum at high energies: background expectation vs. exotic contributions
- On the Importance of Electroweak Corrections for Majorana Dark Matter Indirect Detection
- Measurement of cosmic-ray low-energy antiproton spectrum with the first BESS-Polar Antarctic flight
- Complementarity of Dark Matter Direct Detection Targets
- Nuclear spin structure in dark matter search: The finite momentum transfer limit
- First Results of the Phase II SIMPLE Dark Matter Search
- Search for annual modulation in low-energy CDMS-II data
- 10 GeV dark matter candidates and cosmic-ray antiprotons
- Neutralino annihilation to q qbar g
- Saas-Fee Lecture Notes: Multi-messenger Astronomy and Dark Matter
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- Searching for lepton portal dark matter with colliders and gravitational waves
- Stop Co-Annihilation in the Minimal Supersymmetric Standard Model Revisited
- A calculation for vector dark matter direct detection