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Title: Radio Signal Constraints on Galactic Dark Matter Annihilation

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.3462665· OSTI ID:21410186
 [1];  [2];  [3];  [1];  [3]
  1. Universita 'Federico II', Dipartimento di Scienze Fisiche, Napoli (Italy)
  2. Department of Physics and Astronomy, University of Aarhus, Ny Munkegade, Bygn. 1520 8000 Aarhus (Denmark)
  3. INFN Sezione di Napoli, Complesso Universitario di Monte S. Angelo, Via Cintia, I-80126 Napoli (Italy)

Annihilation of Dark Matter usually produces together with gamma rays comparable amounts of electrons and positrons. The e{sup +}e{sup -} gyrating in the galactic magnetic field then produce secondary synchrotron radiation which thus provides an indirect mean to constrain the DM signal itself. To this purpose, we calculate the radio emission from the galactic halo as well as from its expected substructures and we then compare it with the measured diffuse radio background. We employ a multi-frequency approach using data in the relevant frequency range 100 MHz-100 GHz, as well as the WMAP Haze data at 23 GHz. The derived constraints are of the order <{sigma}{sub A}{sup v}> = 10{sup -24} cm{sup 3}s{sup -1} for a DM mass m{sub {kappa}}= 100 GeV even though sensibly depending on the astrophysical uncertainties.

OSTI ID:
21410186
Journal Information:
AIP Conference Proceedings, Vol. 1241, Issue 1; Conference: Conference on invisible universe, Paris (France), 29 Jun - 3 Jul 2009; Other Information: DOI: 10.1063/1.3462665; (c) 2010 American Institute of Physics; ISSN 0094-243X
Country of Publication:
United States
Language:
English