dc.contributor.author | Das, C. R. | |
dc.contributor.author | Pulido, João | |
dc.contributor.author | Maalampi, Jukka | |
dc.contributor.author | Vihonen, Sampsa | |
dc.date.accessioned | 2018-03-09T11:13:40Z | |
dc.date.available | 2018-03-09T11:13:40Z | |
dc.date.issued | 2018 | |
dc.identifier.citation | Das, 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.other | CONVID_27931183 | |
dc.identifier.other | TUTKAID_76969 | |
dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/57289 | |
dc.description.abstract | The 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.iso | eng | |
dc.publisher | American Physical Society | |
dc.relation.ispartofseries | Physical Review D | |
dc.subject.other | neutrino oscillations | |
dc.subject.other | sterile neutrinos | |
dc.subject.other | neutrino detectors | |
dc.title | Determination of the θ23 octant in long baseline neutrino experiments within and beyond the standard model | |
dc.type | article | |
dc.identifier.urn | URN:NBN:fi:jyu-201803071677 | |
dc.contributor.laitos | Fysiikan laitos | fi |
dc.contributor.laitos | Department of Physics | en |
dc.type.uri | http://purl.org/eprint/type/JournalArticle | |
dc.date.updated | 2018-03-07T13:15:16Z | |
dc.type.coar | http://purl.org/coar/resource_type/c_2df8fbb1 | |
dc.description.reviewstatus | peerReviewed | |
dc.relation.issn | 2470-0010 | |
dc.relation.numberinseries | 3 | |
dc.relation.volume | 97 | |
dc.type.version | publishedVersion | |
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.accesslevel | openAccess | fi |
dc.subject.yso | neutriinot | |
dc.subject.yso | Monte Carlo -menetelmät | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p5219 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p6361 | |
dc.rights.url | https://creativecommons.org/licenses/by/4.0/ | |
dc.relation.doi | 10.1103/PhysRevD.97.035023 | |
dc.type.okm | A1 | |