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dc.contributor.authorKainulainen, Kimmo
dc.contributor.authorTuominen, Kimmo
dc.contributor.authorVirkajärvi, Jussi
dc.date.accessioned2015-09-08T05:47:09Z
dc.date.available2015-09-08T05:47:09Z
dc.date.issued2015
dc.identifier.citationKainulainen, K., Tuominen, K., & Virkajärvi, J. (2015). A model for dark matter, naturalness and a complete gauge unification. <i>Journal of Cosmology and Astroparticle Physics</i>, <i>2015</i>(7), Article 034. <a href="https://doi.org/10.1088/1475-7516/2015/07/034" target="_blank">https://doi.org/10.1088/1475-7516/2015/07/034</a>
dc.identifier.otherCONVID_24822604
dc.identifier.otherTUTKAID_66773
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/46787
dc.description.abstractWe consider dark matter in a minimal extension of the Standard Model (SM) which breaks electroweak symmetry dynamically and leads to a complete unification of the SM and technicolor coupling constants. The unification scale is determined to be MU ≈ 2.2 × 1015 GeV and the unified coupling αU ≈ 0.0304. Moreover, unification strongly suggest that the technicolor sector of the model must become strong at the scale of (TeV) . The model also contains a tightly constrained sector of mixing neutral fields stabilized by a discrete symmetry. We find the lightest of these states can be DM with a mass in the range 0mDM ≈ 3–080 GeV . We find a large set of parameters that satisfy all available constraints from colliders and from dark matter search experiments. However, most of the available parameter space is within the reach of the next generation of DM search experiments. The model is also sensitive to a modest improvement in the measurement of the precision electroweak parameters.en
dc.language.isoeng
dc.relation.ispartofseriesJournal of Cosmology and Astroparticle Physics
dc.subject.otherdark matter experiments
dc.subject.otherdark matter theory
dc.subject.otherparticle physics - cosmology connection
dc.titleA model for dark matter, naturalness and a complete gauge unification
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201509072827
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2015-09-07T15:15:07Z
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn1475-7516
dc.relation.numberinseries7
dc.relation.volume2015
dc.type.versionpublishedVersion
dc.rights.copyright© 2015 the Authors. Article funded by SCOAP3. Content from this work may be used under the terms of the Creative Commons Attribution 3.0 License.
dc.rights.accesslevelopenAccessfi
dc.relation.grantnumber278722
dc.rights.urlhttp://creativecommons.org/licenses/by/3.0/
dc.relation.doi10.1088/1475-7516/2015/07/034
dc.relation.funderSuomen Akatemiafi
dc.relation.funderAcademy of Finlanden
jyx.fundingprogramAkatemiahanke, SAfi
jyx.fundingprogramAcademy Project, AoFen
jyx.fundinginformationWe acknowledge the financial support from the Academy of Finland, projects 278722 and 267842.
dc.type.okmA1


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© 2015 the Authors. Article funded by SCOAP3. Content from this work may be used
under the terms of the Creative Commons Attribution 3.0 License.
Ellei muuten mainita, aineiston lisenssi on © 2015 the Authors. Article funded by SCOAP3. Content from this work may be used under the terms of the Creative Commons Attribution 3.0 License.