Published May 26, 2015 | Version v1
Journal article

Dark matter with topological defects in the Inert Doublet Model

  • 1. Department of Physics and Helsinki Institute of Physics, Helsinki University, P.O. Box 64, Helsinki, 00014 (Finland)
  • 2. Department of Physics and Astronomy, University of Sussex,Falmer Hill, Brighton, BN1 9QH (United Kingdom)
  • 3. Department of Physics, Royal Holloway University of London,Egham Hill, Egham, Surrey, TW20 0EX (United Kingdom)

Description

We examine the production of dark matter by decaying topological defects in the high mass region mDM≫mW of the Inert Doublet Model, extended with an extra U(1) gauge symmetry. The density of dark matter states (the neutral Higgs states of the inert doublet) is determined by the interplay of the freeze-out mechanism and the additional production of dark matter states from the decays of topological defects, in this case cosmic strings. These decays increase the predicted relic abundance compared to the standard freeze-out only case, and as a consequence the viable parameter space of the Inert Doublet Model can be widened substantially. In particular, for a given dark matter annihilation rate lower dark matter masses become viable. We investigate the allowed mass range taking into account constraints on the energy injection rate from the diffuse γ-ray background and Big Bang Nucleosynthesis, together with constraints on the dark matter properties coming from direct and indirect detection limits. For the Inert Doublet Model high-mass region, an inert Higgs mass as low as ∼200 GeV is permitted. There is also an upper limit on string mass per unit length, and hence the symmetry breaking scale, from the relic abundance in this scenario. Depending on assumptions made about the string decays, the limits are in the range 1012 GeV to 1013 GeV

Availability note (English)

Available from http://dx.doi.org/10.1088/1475-7516/2015/05/048; Available from http://repo.scoap3.org/record/10465

Additional details

Publishing Information

Journal Title
Journal of Cosmology and Astroparticle Physics
Journal Volume
2015
Journal Issue
05
Journal Page Range
p. 48
ISSN
1475-7516

Optional Information

Notes
PUBLISHER-ID: JCAP05(2015)048; OAI: oai:repo.scoap3.org:10465
Funding organization
SCOAP3, CERN, Geneva (Switzerland)