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Combined analysis of effective Higgs portal dark matter models
KTH, Centres, Nordic Institute for Theoretical Physics NORDITA.
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2016 (English)In: Physical Review D, ISSN 2470-0010, Vol. 93, no 11, 115016Article in journal (Refereed) PublishedText
Abstract [en]

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)-H-dagger. For the fermion models, we take an admixture of scalar.. and pseudoscalar (psi) over bari gamma(5)psi 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.

Place, publisher, year, edition, pages
American Physical Society , 2016. Vol. 93, no 11, 115016
Keyword [en]
Cherenkov Telescope Array, Automatic-Generation, Feynman-Rules, Crab-Nebula, Lhc, Scalar, Boson, Searches, Particle, Package
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:kth:diva-189670DOI: 10.1103/PhysRevD.93.115016ISI: 000377804300002ScopusID: 2-s2.0-84976416361OAI: oai:DiVA.org:kth-189670DiVA: diva2:949069
Note

QC 20160715

Available from: 2016-07-15 Created: 2016-07-11 Last updated: 2016-07-15Bibliographically approved

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Savage, Christopher
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