Fits to non-supersymmetric SO(10) models with type I and II seesaw mechanisms using renormalization group evolution

dc.contributorHáskóli Íslandsen_US
dc.contributorUniversity of Icelanden_US
dc.contributor.authorOhlsson, Tommy
dc.contributor.authorPernow, Marcus
dc.contributor.departmentRaunvísindastofnun (HÍ)en_US
dc.contributor.departmentScience Institute (UI)en_US
dc.contributor.schoolVerkfræði- og náttúruvísindasvið (HÍ)en_US
dc.contributor.schoolSchool of Engineering and Natural Sciences (UI)en_US
dc.date.accessioned2020-04-20T11:34:37Z
dc.date.available2020-04-20T11:34:37Z
dc.date.issued2019-06-18
dc.descriptionPublisher's version (útgefin grein)en_US
dc.description.abstractWe consider numerical fits to non-supersymmetric SO(10)-based models in which neutrino mass is generated by the type-I or type-II seesaw mechanism or a combination of both. The fits are performed with a sophisticated top-down procedure, taking into account the renormalization group equations of the gauge and Yukawa couplings, integrating out relevant degrees of freedom at their corresponding mass scales, and using recent data for the Standard Model observables. We find acceptable fits for normal neutrino mass ordering only and with neutrino mass generated by either type-I seesaw only or a combination of types I and II seesaw in which type-I seesaw is dominant. Furthermore, we find predictions from the best fit regarding the small neutrino masses, the effective neutrinoless double beta decay mass, and the leptonic CP-violating phase. Finally, we show that the fits are rather insensitive to the chosen value of the unification scale.en_US
dc.description.sponsorshipThe authors wish to thank Sofiane M. Boucenna for collaboration in early stages of this project. T.O. acknowledges support by the Swedish Research Council (Vetenskapsr˚adet) through contract No. 2017-03934 and the KTH Royal Institute of Technology for a sabbatical period at the University of Iceland. M.P. thanks “Stiftelsen Olle Engkvist Byggm¨astare” and “Roland Gustafssons Stiftelse f¨or teoretisk fysik” for financial support. Numerical computations were performed on resources provided by the Swedish National Infrastructure for Computing (SNIC) at PDC Center for High Performance Computing (PDC-HPC) at KTH Royal Institute of Technology in Stockholm, Sweden under project numbers PDC-2018-49 and SNIC 2018/3-559.en_US
dc.description.versionPeer Revieweden_US
dc.format.extent85en_US
dc.identifier.citationOhlsson, T., Pernow, M. Fits to non-supersymmetric SO(10) models with type I and II seesaw mechanisms using renormalization group evolution. Journal of High Energy Physics 2019, 85 (2019). https://doi.org/10.1007/JHEP06(2019)085en_US
dc.identifier.doi10.1007/JHEP06(2019)085
dc.identifier.issn1029-8479
dc.identifier.journalJournal of High Energy Physicsen_US
dc.identifier.urihttps://hdl.handle.net/20.500.11815/1706
dc.language.isoenen_US
dc.publisherSpringer Science and Business Media LLCen_US
dc.relation.ispartofseriesJournal of High Energy Physics;2019(6)
dc.relation.urlhttp://link.springer.com/content/pdf/10.1007/JHEP06(2019)085.pdfen_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectBeyond Standard Modelen_US
dc.subjectGUTen_US
dc.subjectNeutrino Physicsen_US
dc.subjectEðlisfræðien_US
dc.subjectAtómfræðien_US
dc.titleFits to non-supersymmetric SO(10) models with type I and II seesaw mechanisms using renormalization group evolutionen_US
dc.typeinfo:eu-repo/semantics/articleen_US
dcterms.licenseThis article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited.en_US

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