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

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dc.contributor Háskóli Íslands
dc.contributor University of Iceland
dc.contributor.author Ohlsson, Tommy
dc.contributor.author Pernow, Marcus
dc.date.accessioned 2020-04-20T11:34:37Z
dc.date.available 2020-04-20T11:34:37Z
dc.date.issued 2019-06-18
dc.identifier.citation Ohlsson, 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)085
dc.identifier.issn 1029-8479
dc.identifier.uri https://hdl.handle.net/20.500.11815/1706
dc.description Publisher's version (útgefin grein)
dc.description.abstract We 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.
dc.description.sponsorship The 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.
dc.format.extent 85
dc.language.iso en
dc.publisher Springer Science and Business Media LLC
dc.relation.ispartofseries Journal of High Energy Physics;2019(6)
dc.rights info:eu-repo/semantics/openAccess
dc.subject Beyond Standard Model
dc.subject GUT
dc.subject Neutrino Physics
dc.subject Eðlisfræði
dc.subject Atómfræði
dc.title Fits to non-supersymmetric SO(10) models with type I and II seesaw mechanisms using renormalization group evolution
dc.type info:eu-repo/semantics/article
dcterms.license This 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.
dc.description.version Peer Reviewed
dc.identifier.journal Journal of High Energy Physics
dc.identifier.doi 10.1007/JHEP06(2019)085
dc.relation.url http://link.springer.com/content/pdf/10.1007/JHEP06(2019)085.pdf
dc.contributor.department Raunvísindastofnun (HÍ)
dc.contributor.department Science Institute (UI)
dc.contributor.school Verkfræði- og náttúruvísindasvið (HÍ)
dc.contributor.school School of Engineering and Natural Sciences (UI)


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