PPPC 4 DM secondary: a Poor Particle Physicist Cookbook for secondary radiation from Dark Matter

Jatan Buch Marco Cirelli Gaëlle Giesen Marco Taoso 1
1 IPHT - Institut de Physique Théorique - UMR CNRS 3681
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.
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Journal articles
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https://hal-cea.archives-ouvertes.fr/cea-01221157
Contributor : Emmanuelle de Laborderie <>
Submitted on : Tuesday, October 27, 2015 - 3:00:12 PM
Last modification on : Thursday, February 7, 2019 - 3:46:22 PM

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CEA | CNRS | DSM-IPHT | CEA-UPSAY | UNIV-PARIS-SACLAY | CEA-DRF

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Jatan Buch, Marco Cirelli, Gaëlle Giesen, Marco Taoso. PPPC 4 DM secondary: a Poor Particle Physicist Cookbook for secondary radiation from Dark Matter. Journal of Cosmology and Astroparticle Physics, Institute of Physics (IOP), 2015, 2015 (09), ⟨10.1088/1475-7516/2015/9/037⟩. ⟨cea-01221157⟩

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