학술논문

Determining the neutrino mass ordering and oscillation parameters with KM3NeT/ORCA
Document Type
article
Author
S. AielloA. AlbertS. Alves GarreZ. AlyA. AmbrosoneF. AmeliM. AndreG. AndroulakisM. AnghinolfiM. AnguitaG. AntonM. ArdidS. ArdidJ. AublinC. BagatelasB. BaretS. Basegmez du PreeM. BendahmanF. BenfenatiE. BerbeeA. M. van den BergV. BertinS. BiagiM. BissingerM. BoettcherM. Bou CaboJ. BoumaazaM. BoutaM. BouwhuisC. BozzaH. BrânzaşR. BruijnJ. BrunnerR. BrunoE. BuisR. BuompaneJ. BustoB. CaiffiD. CalvoA. CaponeV. CarreteroP. CastaldiS. CelliM. ChababN. ChauA. ChenS. CherubiniV. ChiarellaT. ChiarusiM. CircellaR. CocimanoJ. A. B. CoelhoA. ColeiroM. Colomer MollaR. ConiglioneP. CoyleA. CreusotA. CruzG. CuttoneR. DallierB. De MartinoM. De PalmaM. Di MarinoI. Di PalmaA. F. DíazD. Diego-TortosaC. DistefanoA. DomiC. DonzaudD. DornicM. DörrD. DrouhinT. EberlA. EddyamouiT. van EedenD. van EijkI. El BojaddainiD. ElsaesserA. EnzenhöferV. EspinosaP. FermaniG. FerraraM. D. FilipovićF. FilippiniL. A. FuscoT. GalA. Garcia SotoF. GarufiY. GateletN. GeißelbrechtL. GialanellaE. GiorgioS. R. GozziniR. GraciaK. GrafD. GrassoG. GrellaD. GuderianC. GuidiJ. HaefnerS. HallmannH. HamdaouiH. van HarenA. HeijboerA. HekaloL. HennigJ. J. Hernández-ReyJ. HofestädtF. HuangW. Idrissi IbnsalihG. IlluminatiC. W. JamesM. de JongP. de JongB. J. JungM. KadlerP. KalaczyńskiO. KalekinU. F. KatzN. R. Khan ChowdhuryG. KistauriF. van der KnaapP. KooijmanA. KouchnerM. KreterV. KulikovskiyR. LahmannM. LamoureuxG. LarosaC. LastoriaR. Le BretonS. Le StumO. LeonardiF. LeoneE. LeonoraN. LessingG. LeviM. LincettoM. Lindsey ClarkT. LipreauF. LonghitanoD. Lopez-CotoL. MadererJ. MańczakK. MannheimA. MargiottaA. MarinelliC. MarkouL. MartinJ. A. Martínez-MoraA. MartiniF. MarzaioliS. MastroianniK. W. MelisG. MieleP. MigliozziE. MignecoP. MijakowskiL. S. MirandaC. M. MolloM. MorgantiM. MoserA. MoussaR. MullerM. MusumeciL. NautaS. NavasC. A. NicolauB. Ó. FearraighM. O’SullivanM. OrganokovA. OrlandoJ. Palacios GonzálezG. PapalashviliR. PapaleoC. PastoreA. M. PăunG. E. PăvălaşC. PellegrinoM. Perrin-TerrinV. PestelP. PiattelliC. PieterseK. PikounisO. PisantiC. PoirèV. PopaT. PradierG. PühlhoferS. PulvirentiO. RabyangF. RaffaelliN. RandazzoS. RazzaqueD. RealS. ReckG. RiccobeneA. RomanovA. RovelliF. Salesa GreusD. F. E. SamtlebenA. Sánchez LosaM. SanguinetiA. SantangeloD. SantonocitoP. SapienzaJ. SchnabelM. F. SchneiderJ. SchumannH. M. SchutteJ. SenecaI. SguraR. ShanidzeA. SharmaA. SinopoulouB. SpissoM. SpurioD. StavropoulosS. M. StellacciM. TaiutiY. TayalatiE. TenlladoH. ThiersenS. TingayV. TsourapisE. TzamariudakiD. TzanetatosV. Van ElewyckG. VasileiadisF. VersariD. VivoloG. de WasseigeJ. WilmsR. WojaczyńskiE. de WolfT. YousfiS. ZavatarelliA. ZegarelliD. ZitoJ. D. ZornozaJ. ZúñigaN. ZywuckaKM3NeT Collaboration
Source
European Physical Journal C: Particles and Fields, Vol 82, Iss 1, Pp 1-16 (2022)
Subject
Astrophysics
QB460-466
Nuclear and particle physics. Atomic energy. Radioactivity
QC770-798
Language
English
ISSN
1434-6044
1434-6052
Abstract
Abstract The next generation of water Cherenkov neutrino telescopes in the Mediterranean Sea are under construction offshore France (KM3NeT/ORCA) and Sicily (KM3NeT/ARCA). The KM3NeT/ORCA detector features an energy detection threshold which allows to collect atmospheric neutrinos to study flavour oscillation. This paper reports the KM3NeT/ORCA sensitivity to this phenomenon. The event reconstruction, selection and classification are described. The sensitivity to determine the neutrino mass ordering was evaluated and found to be 4.4 $$\sigma $$ σ if the true ordering is normal and 2.3 $$\sigma $$ σ if inverted, after 3 years of data taking. The precision to measure $$\varDelta m^2_{32}$$ Δ m 32 2 and $$\theta _{23}$$ θ 23 were also estimated and found to be $$85 . 10^{-6}~{\mathrm{eV}^{2}}$$ 85 . 10 - 6 eV 2 and $$(^{+1.9}_{-3.1})^{\circ }$$ ( - 3.1 + 1.9 ) ∘ for normal neutrino mass ordering and, $$75 . 10^{-6}~{\mathrm{eV}^{2}}$$ 75 . 10 - 6 eV 2 and $$(^{+2.0}_{-7.0})^{\circ }$$ ( - 7.0 + 2.0 ) ∘ for inverted ordering. Finally, a unitarity test of the leptonic mixing matrix by measuring the rate of tau neutrinos is described. Three years of data taking were found to be sufficient to exclude event rate variations larger than 20% at $$3\sigma $$ 3 σ level.