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Title: Updated galactic radio constraints on Dark Matter

Abstract

We perform a detailed analysis of the synchrotron signals produced by dark matter annihilations and decays. We consider different set-ups for the propagation of electrons and positrons, the galactic magnetic field and dark matter properties. We then confront these signals with radio and microwave maps, including PLANCK measurements, from a frequency of 22 MHz up to 70 GHz. We derive two sets of constraints: conservative and progressive, the latter based on a modeling of the astrophysical emission. Radio and microwave constraints are complementary to those obtained with other indirect detection methods, especially for dark matter annihilating into leptonic channels.

Authors:
 [1];  [2]
  1. Laboratoire de Physique Théorique et Hautes Energies (LPTHE),UMR 7589 CNRS & UPMC, 4 Place Jussieu, Paris, F-75252 (France)
  2. Instituto de Física Teórica (IFT) UAM/CSIC,calle Nicolás Cabrera 13-15, Cantoblanco, Madrid, 28049 (Spain)
Publication Date:
Sponsoring Org.:
SCOAP3, CERN, Geneva (Switzerland)
OSTI Identifier:
22572122
Resource Type:
Journal Article
Resource Relation:
Journal Name: Journal of Cosmology and Astroparticle Physics; Journal Volume: 2016; Journal Issue: 07; Other Information: PUBLISHER-ID: JCAP07(2016)041; OAI: oai:repo.scoap3.org:16559; cc-by Article funded by SCOAP3. Content from this work may be used under the terms of the Creative Commons Attribution 3.0 License. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.; Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; ANNIHILATION; ASTROPHYSICS; COSMIC ELECTRONS; COSMIC POSITRONS; COSMIC RADIO SOURCES; GALAXIES; GHZ RANGE 01-100; INTERSTELLAR MAGNETIC FIELDS; LIMITING VALUES; MHZ RANGE 01-100; NONLUMINOUS MATTER; RELICT RADIATION; SPACE VEHICLES; SYNCHROTRON RADIATION

Citation Formats

Cirelli, Marco, and Taoso, Marco. Updated galactic radio constraints on Dark Matter. United States: N. p., 2016. Web. doi:10.1088/1475-7516/2016/07/041.
Cirelli, Marco, & Taoso, Marco. Updated galactic radio constraints on Dark Matter. United States. doi:10.1088/1475-7516/2016/07/041.
Cirelli, Marco, and Taoso, Marco. Mon . "Updated galactic radio constraints on Dark Matter". United States. doi:10.1088/1475-7516/2016/07/041.
@article{osti_22572122,
title = {Updated galactic radio constraints on Dark Matter},
author = {Cirelli, Marco and Taoso, Marco},
abstractNote = {We perform a detailed analysis of the synchrotron signals produced by dark matter annihilations and decays. We consider different set-ups for the propagation of electrons and positrons, the galactic magnetic field and dark matter properties. We then confront these signals with radio and microwave maps, including PLANCK measurements, from a frequency of 22 MHz up to 70 GHz. We derive two sets of constraints: conservative and progressive, the latter based on a modeling of the astrophysical emission. Radio and microwave constraints are complementary to those obtained with other indirect detection methods, especially for dark matter annihilating into leptonic channels.},
doi = {10.1088/1475-7516/2016/07/041},
journal = {Journal of Cosmology and Astroparticle Physics},
number = 07,
volume = 2016,
place = {United States},
year = {Mon Jul 25 00:00:00 EDT 2016},
month = {Mon Jul 25 00:00:00 EDT 2016}
}