Combined analysis of effective Higgs portal dark matter models

Open Access
Authors
  • A. Beniwal
  • F. Rajec
  • C. Savage
  • P. Scott
Publication date 01-06-2016
Journal Physical Review D. Particles and Fields
Article number 115016
Volume | Issue number 93 | 11
Number of pages 31
Organisations
  • Faculty of Science (FNWI) - Institute of Physics (IoP)
  • Faculty of Science (FNWI) - Institute of Physics (IoP) - Institute for Theoretical Physics Amsterdam (ITFA)
  • Faculty of Science (FNWI)
Abstract
We combine and extend the analyses of effective scalar, vector, Majorana and Dirac fermion Higgs portal models of dark matter (DM), in which DM couples to the Standard Model (SM) Higgs boson via an operator of the form ODMHH . For the fermion models, we take an admixture of scalar ¯¯¯ψψ and pseudoscalar ¯¯¯ψiγ5ψ interaction terms. For each model, we apply constraints on the parameter space based on the Planck measured DM relic density and the LHC limits on the Higgs invisible branching ratio. For the first time, we perform a consistent study of the indirect detection prospects for these models based on the WMAP7/Planck observations of the cosmic microwave background, a combined analysis of 15 dwarf spheroidal galaxies by Fermi-LAT and the upcoming Cherenkov Telescope Array (CTA). We also perform a correct treatment of the momentum-dependent direct search cross section that arises from the pseudoscalar interaction term in the fermionic DM theories. We find, in line with previous studies, that current and future direct search experiments such as LUX and XENON1T can exclude much of the parameter space, and we demonstrate that a joint observation in both indirect and direct searches is possible for high mass weakly interacting massive particles. In the case of a pure pseudoscalar interaction of a fermionic DM candidate, future gamma-ray searches are the only class of experiment capable of probing the high mass range of the theory.
Document type Article
Note © 2016 American Physical Society
Language English
Published at https://doi.org/10.1103/PhysRevD.93.115016
Published at https://www.scopus.com/inward/record.uri?eid=2-s2.0-84976416361&doi=10.1103%2fPhysRevD.93.115016&partnerID=40&md5=57b949fe3c04fc0b90d46e617e7bcb20
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PhysRevD.93 (Final published version)
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