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) |