Show simple item record

dc.contributor.authorDas, C.R.
dc.contributor.authorMaalampi, Jukka
dc.contributor.authorPulido, J.
dc.contributor.authorVihonen, Sampsa
dc.date.accessioned2017-11-14T11:44:18Z
dc.date.available2017-11-14T11:44:18Z
dc.date.issued2017
dc.identifier.citationDas, C.R., Maalampi, J., Pulido, J., & Vihonen, S. (2017). Optimizing the θ23 octant search in long baseline neutrino experiments. In <i>Neutrino 2016 : XXVII International Conference on Neutrino Physics and Astrophysics</i> (Article 012219). Institute of Physics Publishing. Journal of Physics: Conference Series, 888. <a href="https://doi.org/10.1088/1742-6596/888/1/012219" target="_blank">https://doi.org/10.1088/1742-6596/888/1/012219</a>
dc.identifier.otherCONVID_27341566
dc.identifier.otherTUTKAID_75639
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/55873
dc.description.abstractDetermination of the θ 23 octant will be an important goal for the next generation of neutrino oscillation experiments, as it will show whether the true value of θ 23 lies in the high octant, θ 23 > 45°, or in the low octant, θ 23 < 45°. In this work we investigate the prospects of studying the θ 23 octant in future long baseline neutrino experiments. Using the GLoBES software, we study the sensitivity to θ 23 octant in terms of baseline length and beam sharing and use the LBNO setup as our benchmark. We also show the interference on the octant determination that arises from the unconstrained CP violation angle δ CP. In our results, we show the impact of matter effects on the octant determination potential and establish a connection between the beam sharing and mass hierarchy.
dc.language.isoeng
dc.publisherInstitute of Physics Publishing
dc.relation.ispartofNeutrino 2016 : XXVII International Conference on Neutrino Physics and Astrophysics
dc.relation.ispartofseriesJournal of Physics: Conference Series
dc.subject.otherneutrino oscillation experiments
dc.subject.othermixing angle
dc.titleOptimizing the θ23 octant search in long baseline neutrino experiments
dc.typeconferenceObject
dc.identifier.urnURN:NBN:fi:jyu-201711104220
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/ConferencePaper
dc.date.updated2017-11-10T16:15:09Z
dc.type.coarhttp://purl.org/coar/resource_type/c_5794
dc.description.reviewstatuspeerReviewed
dc.relation.issn1742-6588
dc.type.versionpublishedVersion
dc.rights.copyright© 2017 the Authors. This is an open access article distributed under the terms of the Creative Commons Attribution License.
dc.rights.accesslevelopenAccessfi
dc.relation.conferenceInternational Conference on Neutrino Physics and Astrophysics
dc.subject.ysoneutriinot
jyx.subject.urihttp://www.yso.fi/onto/yso/p5219
dc.rights.urlhttp://creativecommons.org/licenses/by/3.0
dc.relation.doi10.1088/1742-6596/888/1/012219
dc.type.okmA4


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record

© 2017 the Authors. This is an open access article distributed under the terms of the Creative Commons Attribution License.
Except where otherwise noted, this item's license is described as © 2017 the Authors. This is an open access article distributed under the terms of the Creative Commons Attribution License.