A Multi-frequency analysis of dark matter annihilation interpretations of recent anti-particle and gamma-ray excesses in cosmic structures
arXiv:1508.01386 · doi:10.1088/1475-7516/2016/05/013
Abstract
The Fermi-LAT observation of a gamma-ray excess from the galactic-centre, as well as the PAMELA, AMS, and AMS-2 anti-particle excesses, and the recent claim of a Fermi-LAT excess in the Reticulum-2 dwarf galaxy have been put forward as signatures compatible with of neutralino dark matter. These are of particular interest as the neutralino annihilation models which fit these observations might have observable consequences from radio to gamma-ray emission. Since dark matter is expected to be a major matter constituent of cosmic structure, these multi-frequency consequences should also be common to structures across the mass spectrum. Thus, in this work we make predictions for the multi-frequency spectra of three well-known sources dominated by dark matter, e.g. the Coma cluster, the galaxy M81, and the Draco dwarf galaxy using models favoured by dark matter interpretations of the aforementioned observations. We pay special attention to the consequences for these models when their cross-sections are renormalised to reproduce the recent gamma-ray excess observed in the Reticulum-2 dwarf galaxy, which throw a dark matter interpretation of this excess into doubt. We find that the multi-frequency data of Coma and Draco disfavour the dark matter interpretation of the AMS, PAMELA and Fermi anti-particle excess. Models derived from Fermi-LAT galactic centre observations present somewhat lesser conflicts. We determine the detection prospects of the Square Kilometre Array, the Cherenkov Telescope Array, as well as the ASTROGAM and ASTRO-H satellites for the studied models. This demonstrates that ASTRO-H is well positioned to probe the X-ray emissions from neutralino annihilation. Thus, multi-frequency observation with the next generation experiments will allow for unprecedented sensitivity to the neutralino parameter space.
40 pages, 17 figures, 4 Tables. Submitted to JCAP
References in corpus (23)
- CRATES: An All-Sky Survey of Flat-Spectrum Radio Sources
- PAMELA - A Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics
- An Ultraviolet-to-Radio Broadband Spectral Atlas of Nearby Galaxies
- Strong support for the millisecond pulsar origin of the Galactic center GeV excess
- A Tale of Tails: Dark Matter Interpretations of the Fermi GeV Excess in Light of Background Model Systematics
- Evidence for Unresolved Gamma-Ray Point Sources in the Inner Galaxy
- Gamma-ray and radio tests of the e+e- excess from DM annihilations
- Search for Gamma-Ray Emission from DES Dwarf Spheroidal Galaxy Candidates with Fermi-LAT Data
- Detecting dark matter WIMPs in the Draco dwarf: a multi-wavelength perspective
- A Comprehensive Search for Dark Matter Annihilation in Dwarf Galaxies
- Indication of Gamma-ray Emission from the Newly Discovered Dwarf Galaxy Reticulum II
- Disrupted Globular Clusters Can Explain the Galactic Center Gamma Ray Excess
- Dwarf Galaxy Dark Matter Density Profiles Inferred from Stellar and Gas Kinematics
- Search for gamma-ray emission from the Coma Cluster with six years of Fermi-LAT data
- What Does The PAMELA Antiproton Spectrum Tell Us About Dark Matter?
- Dark matter annihilation and decay profiles for the Reticulum II dwarf spheroidal galaxy
- A description of the Galactic Center excess in the Minimal Supersymmetric Standard Model
- Boosting the annihilation boost: Tidal effects on dark matter subhalos and consistent luminosity modeling
- Degree of Polarization and Source Counts of Faint Radio Sources from Stacking Polarized Intensity
- Local Group dSph radio survey with ATCA (II): Non-thermal diffuse emission
- Local Group dSph radio survey with ATCA (III): Constraints on Particle Dark Matter
- New Limits On Gamma-Ray Emission From Galaxy Clusters
- Fermi/LAT observations of Dwarf Galaxies highly constrain a Dark Matter Interpretation of Excess Positrons seen in AMS-02, HEAT, and PAMELA
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- Integral X-ray constraints on sub-GeV Dark Matter
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- Dark matter in the Reticulum II dSph: a radio search
- SKA-Phase 1 sensitivity for synchrotron radio emission from multi-TeV Dark Matter candidates
- Radio constraints on dark matter annihilation in Canes Venatici I with LOFAR
- Heavy dark matter particle annihilation in dwarf spheroidal galaxies: radio signals at the SKA telescope
- Universal profiles for radio searches of dark matter in dwarf galaxies
- Constraining annihilating dark matter by radio data of M33
- Can SKA--Phase 1 go much beyond the LHC in supersymmetry search?
- A general study of decaying scalar dark matter: existing limits and projected radio signals at the SKA
- The role of Dark Matter sub-halos in the non-thermal emission of galaxy clusters
- Stringent constraint on the radio signal from dark matter annihilation in dwarf spheroidal galaxies using the TGSS
- Constraints on dark matter annihilation from the FAST observation of the Coma Berenices dwarf galaxy
- Galaxy clusters in high definition: a dark matter search
- A new target object for constraining annihilating dark matter
- A Multi-frequency analysis of possible Dark Matter Contributions to M31 Gamma-Ray Emissions
- An excess of excesses examined via dark matter radio emissions from galaxies
- Synchrotron Emission from Dark Matter in Galactic Subhalos. A Look into the Smith Cloud
- Connecting multi-lepton anomalies at the LHC and in Astrophysics with MeerKAT/SKA
- Search for decaying heavy dark matter in an effective interaction framework: a comparison of -ray and radio observations
- Prospects of future MeV telescopes in probing weak-scale Dark Matter
- Multi-frequency test of dark matter annihilation into long-lived particles in Sirius
- Hunting dark matter in galaxy clusters with non-thermal electrons
- Dark matter, extra-terrestrial gamma-rays and the MSSM: a viability study
- What Can Gamma-rays from Space tell us About the Madala Hypothesis?