Dark Matter Annihilation into Four-Body Final States and Implications for the AMS Antiproton Excess
arXiv:1709.07410 · doi:10.1103/PhysRevD.97.023003
Abstract
We consider dark matter annihilation into a general set of final states of Standard Model particles, including two-body and four-body final states that result from the decay of intermediate states. For dark matter masses ~10-10^5 GeV, we use updated data from Planck and from high gamma-ray experiments such as Fermi-LAT, MAGIC, and VERITAS to constrain the annihilation cross section for each final state. The Planck constraints are the most stringent over the entire mass range for annihilation into light leptons, and the Fermi-LAT constraints are the most stringent for four-body final states up to masses ~10^4 GeV. We consider these constraints in light of the recent AMS antiproton results, and show that for light mediators it is possible to explain the AMS data with dark matter, and remain consistent with Fermi-LAT Inner Galaxy measurements, for m_χ~ 60-100 GeV mass dark matter and mediator masses m_ϕ/ m_χ~< 1.
12 pages, 6 figures
References in corpus (8)
- PYTHIA 6.4 Physics and Manual
- CMB Constraints on WIMP Annihilation: Energy Absorption During the Recombination Epoch
- Weak Corrections are Relevant for Dark Matter Indirect Detection
- Possible Evidence For Dark Matter Annihilation In The Inner Milky Way From The Fermi Gamma Ray Space Telescope
- Updated CMB constraints on Dark Matter annihilation cross-sections
- A Comprehensive Search for Dark Matter Annihilation in Dwarf Galaxies
- The Semi-Hooperon: Gamma-ray and anti-proton excesses in the Galactic Center
- High Statistics Measurement of the Positron Fraction in Primary Cosmic Rays with the Alpha Magnetic Spectrometer on the International Space Station