Published August 29, 2012 | Version v1
Journal article

Higgs dark matter in UEDs: A good WIMP with bad detection prospects

  • 1. Department of Theoretical Physics, School of Engineering Sciences, KTH Royal Institute of Technology–AlbaNova University Center, Roslagstullsbacken 21, 106 91 Stockholm (Sweden)
  • 2. Physics and Astronomy, University of Southampton, Highfield, Southampton SO17 1BJ (United Kingdom)
  • 3. Department of Theoretical Physics, School of Engineering Sciences, KTH Royal Institute of Technology-AlbaNova University Center, Roslagstullsbacken 21, 106 91 Stockholm (Sweden)

Description

We study the first Kaluza-Klein excitation of the Higgs boson in universal extra dimensions as a dark matter candidate. The first-level Higgs boson could be the lightest Kaluza-Klein particle, which is stable due to the conservation of Kaluza-Klein parity, in non-minimal models where boundary localized terms modify the mass spectrum. We calculate the relic abundance and find that it agrees with the observed dark matter density if the mass of the first-level Higgs boson is slightly above 2 TeV, not considering coannihilations and assuming no relative mass splitting among the first-level Kaluza-Klein modes. In the case of coannihilations and a non-zero mass splitting, the mass of the first-level Higgs boson can range from 1 TeV to 4 TeV. We study also the prospects for detection of this dark matter candidate in direct as well as indirect detection experiments. Although the first-level Higgs boson is a typical weakly interacting massive particle, an observation in any of the conventional experiments is very challenging.

Availability note (English)

Available from http://dx.doi.org/10.1016/j.physletb.2012.07.037

Additional details

Identifiers

DOI
10.1016/j.physletb.2012.07.037;
arXiv
arXiv:1204.5186v2;
PII
S0370-2693(12)00777-0;

Publishing Information

Journal Title
Physics Letters. Section B
Journal Volume
715
Journal Issue
1-3
Journal Page Range
p. 164-169
ISSN
0370-2693
CODEN
PYLBAJ

Optional Information

Copyright
Copyright (c) 2012 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.