PPPC 4 DM secondary: A Poor Particle Physicist Cookbook for secondary radiation from Dark Matter
arXiv:1505.01049 · doi:10.1088/1475-7516/2015/09/037
Abstract
We enlarge the set of recipes and ingredients at disposal of any poor particle physicist eager to cook up signatures from weak-scale Dark Matter models by computing two secondary emissions due to DM particles annihilating or decaying in the galactic halo, namely the radio signals from synchrotron emission and the gamma rays from bremsstrahlung. We consider several magnetic field configurations and propagation scenarios for electrons and positrons. We also provide an improved energy loss function for electrons and positrons in the Galaxy, including synchrotron losses in the different configurations, bremsstrahlung losses, ionization losses and Inverse Compton losses with an updated InterStellar Radiation Field.
25 pages, many figures. v2: a small clarification on the use of custom galactic magnetic fields added, matches version published on JCAP. All results are available at http://www.marcocirelli.net/PPPC4DMID.html
Cited by in corpus (20)
- MadDM v.3.0: a Comprehensive Tool for Dark Matter Studies
- Sensitivity Projections for Dark Matter Searches with the Fermi Large Area Telescope
- Dark Matter's secret liaisons: phenomenology of a dark U(1) sector with bound states
- Integral X-ray constraints on sub-GeV Dark Matter
- Multiwavelength Analysis of Dark Matter Annihilation and RX-DMFIT
- Constraints on heavy decaying dark matter from 570 days of LHAASO observations
- Decaying dark matter at IceCube and its signature on High Energy gamma experiments
- New minimal, median, and maximal propagation models for dark matter searches with Galactic cosmic rays
- Late decaying 2-component dark matter scenario as an explanation of the AMS-02 positron excess
- Higgsino Dark Matter Confronts 14 years of Fermi Gamma Ray Data
- Muonphilic Dark Matter explanation of gamma-ray galactic center excess: a comprehensive analysis
- Multi-TeV dark matter density in the inner Milky Way halo: spectral and dynamical constraints
- Towards understanding thermal history of the Universe through direct and indirect detection of dark matter
- Oscillating Composite Asymmetric Dark Matter
- What Could be the Observational Signature of Dark Matter in Globular Clusters?
- Astrophysical constraints from synchrotron emission on very massive decaying dark matter
- Strong Constraints on Dark Photon and Scalar Dark Matter Decay from INTEGRAL and AMS-02 data
- Some Implications of the Leptonic Annihilation of Dark Matter: Possible Galactic Radio Emission Signatures and the Excess Radio Flux of Extragalactic Origin
- Signatures of Dark Matter in Cosmic-Ray Observations
- Neutrino production in the central dark-matter spikes of active galaxies