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dc.contributor.authorDas, C. R.
dc.contributor.authorPulido, João
dc.contributor.authorMaalampi, Jukka
dc.contributor.authorVihonen, Sampsa
dc.date.accessioned2018-03-09T11:13:40Z
dc.date.available2018-03-09T11:13:40Z
dc.date.issued2018
dc.identifier.citationDas, C. R., Pulido, J., Maalampi, J., & Vihonen, S. (2018). Determination of the θ23 octant in long baseline neutrino experiments within and beyond the standard model. <i>Physical Review D</i>, <i>97</i>(3), Article 035023. <a href="https://doi.org/10.1103/PhysRevD.97.035023" target="_blank">https://doi.org/10.1103/PhysRevD.97.035023</a>
dc.identifier.otherCONVID_27931183
dc.identifier.otherTUTKAID_76969
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/57289
dc.description.abstractThe recent data indicate that the neutrino mixing angle θ 23 deviates from the maximal-mixing value of 45°, showing two nearly degenerate solutions, one in the lower octant (LO) ( θ 23 < 4 5 ° ) and one in the higher octant (HO) ( θ 23 > 4 5 ° ). We investigate, using numerical simulations, the prospects for determining the octant of θ 23 in the future long baseline oscillation experiments. We present our results as contour plots on the ( θ 23 − 4 5 ° , δ )–plane, where δ is the C P phase, showing the true values of θ 23 for which the octant can be experimentally determined at 3 σ , 2 σ and 1 σ confidence level. In particular, we study the impact of the possible nonunitarity of neutrino mixing on the experimental determination of θ 23 in those experiments.
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.ispartofseriesPhysical Review D
dc.subject.otherneutrino oscillations
dc.subject.othersterile neutrinos
dc.subject.otherneutrino detectors
dc.titleDetermination of the θ23 octant in long baseline neutrino experiments within and beyond the standard model
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201803071677
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2018-03-07T13:15:16Z
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn2470-0010
dc.relation.numberinseries3
dc.relation.volume97
dc.type.versionpublishedVersion
dc.rights.copyright© the Authors, 2018. Published by the American Physical Society. Funded by SCOAP3. This is an open access article distributed under the terms of the Creative Commons License.
dc.rights.accesslevelopenAccessfi
dc.subject.ysoneutriinot
dc.subject.ysoMonte Carlo -menetelmät
jyx.subject.urihttp://www.yso.fi/onto/yso/p5219
jyx.subject.urihttp://www.yso.fi/onto/yso/p6361
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1103/PhysRevD.97.035023
dc.type.okmA1


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© the Authors, 2018. Published by the American Physical Society. Funded by SCOAP3. This is an open access article distributed under the terms of the Creative Commons License.
Except where otherwise noted, this item's license is described as © the Authors, 2018. Published by the American Physical Society. Funded by SCOAP3. This is an open access article distributed under the terms of the Creative Commons License.