University of Hertfordshire

From the same journal

From the same journal

By the same authors

Radio constraints on dark matter annihilation in Canes Venatici I with LOFAR

Research output: Contribution to journalArticle


  • staa1657

    Accepted author manuscript, 1.41 MB, PDF document

  • Martin Vollmann
  • Volker Heesen
  • Timothy Shimwell
  • Martin J. Hardcastle
  • Marcus Brüggen
  • Günter Sigl
  • Huub Röttgering
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Original languageEnglish
Article numberstaa1657
JournalMonthly Notices of the Royal Astronomical Society
Early online date13 Jun 2020
Publication statusE-pub ahead of print - 13 Jun 2020


Dwarf galaxies are dark matter-dominated and therefore promising targets for the search for weakly interacting massive particles (WIMPs), which are well-known candidates for dark matter. Annihilation of WIMPs produce ultra-relativistic cosmic-ray electrons and positrons that emit synchrotron radiation in the presence of magnetic fields. For typical magnetic field strengths (few $\mu $G) and $\mathcal O$(GeV-TeV) WIMP masses (and thus typical electron energies of the same order) this emission peaks at hundreds of MHz. Here, we use the non-detection of 150-MHz radio continuum emission from the dwarf spheroidal galaxy `Canes Venatici I' with the LOw-Frequency ARray (LOFAR) to derive constraints on the annihilation cross section of WIMPs into primary electron-positron and other fundamental particle-antiparticle pairs. In this first-of-its-kind LOFAR study, we obtain new constraints on annihilating WIMP dark matter (DM). Using conservative estimates for the magnetic field strengths and diffusion coefficients, we obtain limits that are comparable with those by the Fermi Large Area Telescope (Fermi-LAT) using gamma-ray observations. Assuming s-wave annihilation and WIMPs making up 100% of the DM density, our limits exclude several thermal WIMP realisations in the $[2,20]$-GeV mass range. A more ambitious multi-wavelength and multi-target LOFAR study could improve these limits by a few orders of magnitude.


This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2020 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

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