dc.contributor.author | KM3NeT collaboration | |
dc.contributor.author | JUNO collaboration | |
dc.date.accessioned | 2022-06-15T05:49:33Z | |
dc.date.available | 2022-06-15T05:49:33Z | |
dc.date.issued | 2022 | |
dc.identifier.citation | KM3NeT collaboration, JUNO collaboration. (2022). Combined sensitivity of JUNO and KM3NeT/ORCA to the neutrino mass ordering. <i>Journal of High Energy Physics</i>, <i>2022</i>(3), Article 55. <a href="https://doi.org/10.1007/JHEP03(2022)055" target="_blank">https://doi.org/10.1007/JHEP03(2022)055</a> | |
dc.identifier.other | CONVID_145708418 | |
dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/81706 | |
dc.description.abstract | This article presents the potential of a combined analysis of the JUNO and KM3NeT/ORCA experiments to determine the neutrino mass ordering. This combination is particularly interesting as it significantly boosts the potential of either detector, beyond simply adding their neutrino mass ordering sensitivities, by removing a degeneracy in the determination of ∆m231 between the two experiments when assuming the wrong ordering. The study is based on the latest projected performances for JUNO, and on simulation tools using a full Monte Carlo approach to the KM3NeT/ORCA response with a careful assessment of its energy systematics. From this analysis, a 5σ determination of the neutrino mass ordering is expected after 6 years of joint data taking for any value of the oscillation parameters. This sensitivity would be achieved after only 2 years of joint data taking assuming the current global best-fit values for those parameters for normal ordering. | en |
dc.format.mimetype | application/pdf | |
dc.language.iso | eng | |
dc.publisher | Springer Science and Business Media LLC | |
dc.relation.ispartofseries | Journal of High Energy Physics | |
dc.rights | CC BY 4.0 | |
dc.title | Combined sensitivity of JUNO and KM3NeT/ORCA to the neutrino mass ordering | |
dc.type | research article | |
dc.identifier.urn | URN:NBN:fi:jyu-202206153316 | |
dc.contributor.laitos | Fysiikan laitos | fi |
dc.contributor.laitos | Department of Physics | en |
dc.type.uri | http://purl.org/eprint/type/JournalArticle | |
dc.type.coar | http://purl.org/coar/resource_type/c_2df8fbb1 | |
dc.description.reviewstatus | peerReviewed | |
dc.relation.issn | 1126-6708 | |
dc.relation.numberinseries | 3 | |
dc.relation.volume | 2022 | |
dc.type.version | publishedVersion | |
dc.rights.copyright | © 2022 the Authors | |
dc.rights.accesslevel | openAccess | fi |
dc.type.publication | article | |
dc.subject.yso | ilmaisimet | |
dc.subject.yso | neutriinot | |
dc.subject.yso | tutkimuslaitteet | |
dc.subject.yso | hiukkasfysiikka | |
dc.format.content | fulltext | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p4220 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p5219 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p2440 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p15576 | |
dc.rights.url | https://creativecommons.org/licenses/by/4.0/ | |
dc.relation.doi | 10.1007/JHEP03(2022)055 | |
dc.type.okm | A1 | |