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| 001 | 357212 | ||
| 005 | 20260319124957.0 | ||
| 024 | 7 | _ | |a 10.48550/ARXIV.2405.18008 |2 doi |
| 024 | 7 | _ | |a arXiv:2405.18008 |2 arXiv |
| 037 | _ | _ | |a GSI-2025-00355 |
| 041 | _ | _ | |a English |
| 088 | _ | _ | |a arXiv:2405.18008 |2 arXiv |
| 100 | 1 | _ | |a Juno Collaboration |0 P:(DE-HGF)0 |b 0 |e Corresponding author |
| 245 | _ | _ | |a Potential to Identify the Neutrino Mass Ordering with Reactor Antineutrinos in JUNO |
| 260 | _ | _ | |c 2024 |b arXiv |
| 336 | 7 | _ | |a Preprint |b preprint |m preprint |0 PUB:(DE-HGF)25 |s 1769435732_503618 |2 PUB:(DE-HGF) |
| 336 | 7 | _ | |a WORKING_PAPER |2 ORCID |
| 336 | 7 | _ | |a Electronic Article |0 28 |2 EndNote |
| 336 | 7 | _ | |a preprint |2 DRIVER |
| 336 | 7 | _ | |a ARTICLE |2 BibTeX |
| 336 | 7 | _ | |a Output Types/Working Paper |2 DataCite |
| 520 | _ | _ | |a The Jiangmen Underground Neutrino Observatory (JUNO) is a multi-purpose neutrino experiment under construction in South China. This paper presents an updated estimate of JUNO's sensitivity to neutrino mass ordering using the reactor antineutrinos emitted from eight nuclear reactor cores in the Taishan and Yangjiang nuclear power plants. This measurement is planned by studying the fine interference pattern caused by quasi-vacuum oscillations in the oscillated antineutrino spectrum at a baseline of 52.5~km and is completely independent of the CP violating phase and neutrino mixing angle $θ_{23}$. The sensitivity is obtained through a joint analysis of JUNO and Taishan Antineutrino Observatory (TAO) detectors utilizing the best available knowledge to date about the location and overburden of the JUNO experimental site, local and global nuclear reactors, JUNO and TAO detector responses, expected event rates and spectra of signals and backgrounds, and systematic uncertainties of analysis inputs. We find that a 3$σ$ median sensitivity to reject the wrong mass ordering hypothesis can be reached with an exposure to approximately 6.5 years $\times$ 26.6 GW thermal power. |
| 536 | _ | _ | |a 612 - Cosmic Matter in the Laboratory (POF4-612) |0 G:(DE-HGF)POF4-612 |c POF4-612 |f POF IV |x 0 |
| 588 | _ | _ | |a Dataset connected to DataCite |
| 650 | _ | 7 | |a High Energy Physics - Experiment (hep-ex) |2 Other |
| 650 | _ | 7 | |a FOS: Physical sciences |2 Other |
| 693 | _ | _ | |1 EXP:(DE-Ds200)JUNO-2022 |0 EXP:(DE-Ds200)JUNO-2022 |a JUNO Experiment at Jiangmen Underground Neutrino Observatory in China ( - ; other) |x 0 |
| 773 | _ | _ | |a 10.48550/ARXIV.2405.18008 |p 39 p. |
| 787 | 0 | _ | |a Abusleme, Angel et.al. |d Bristol [u.a.] : IOP Publ., 2025 |i RelatedTo |0 GSI-2025-01102 |r |t Potential to identify neutrino mass ordering with reactor antineutrinos at JUNO* |
| 909 | C | O | |p VDB |o oai:repository.gsi.de:357212 |
| 910 | 1 | _ | |a GSI Helmholtzzentrum für Schwerionenforschung GmbH |0 I:(DE-Ds200)20121206GSI |k GSI |b 0 |6 P:(DE-HGF)0 |
| 913 | 1 | _ | |a DE-HGF |b Forschungsbereich Materie |l Matter and the Universe |1 G:(DE-HGF)POF4-610 |0 G:(DE-HGF)POF4-612 |3 G:(DE-HGF)POF4 |2 G:(DE-HGF)POF4-600 |4 G:(DE-HGF)POF |v Cosmic Matter in the Laboratory |x 0 |
| 914 | 1 | _ | |y 2024 |
| 920 | _ | _ | |l yes |
| 920 | 1 | _ | |0 I:(DE-Ds200)FFN-20210302OR452 |k FFN |l FAIR Forschung NRW |x 0 |
| 980 | _ | _ | |a preprint |
| 980 | _ | _ | |a VDB |
| 980 | _ | _ | |a I:(DE-Ds200)FFN-20210302OR452 |
| 980 | _ | _ | |a UNRESTRICTED |
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