par Mambrini, Yann;Tytgat, Michel ;Zaharijas, Gabrijela;Zaldívar, Bryan
Référence Journal of Cosmology and Astroparticle Physics, 1211, page (038)
Publication Publié, 2012
Référence Journal of Cosmology and Astroparticle Physics, 1211, page (038)
Publication Publié, 2012
Article révisé par les pairs
Résumé : | In this work we confront dark matter models to constraints that may be derived from radio synchrotron radiation from the Galaxy, taking into account the astrophysical uncertainties and we compare these to bounds set by accelerator and complementary indirect dark matter searches. Specifically we apply our analysis to three popular particle physics models. First, a generic effective operator approach, in which case we set bounds on the corresponding mass scale, and then, two specific UV completions, the Z′ and Higgs portals. We show that for many candidates, the radio synchrotron limits are competitive with the other searches, and could even give the strongest constraints (as of today) with some reasonable assumptions regarding the astrophysical uncertainties. © 2012 IOP Publishing Ltd and Sissa Medialab srl. |