001     911312
005     20230328130140.0
024 7 _ |a 10.1088/1674-1137/ac8bc9
|2 doi
024 7 _ |a 0254-3052
|2 ISSN
024 7 _ |a 1674-1137
|2 ISSN
024 7 _ |a 2058-6132
|2 ISSN
024 7 _ |a 2128/32563
|2 Handle
024 7 _ |a WOS:000928183400001
|2 WOS
037 _ _ |a FZJ-2022-04605
041 _ _ |a English
082 _ _ |a 530
100 1 _ |a He, Miao
|0 0000-0002-6813-4553
|b 0
|e Corresponding author
245 _ _ |a Sub-percent Precision Measurement of Neutrino Oscillation Parameters with JUNO
260 _ _ |a Bristol [u.a.]
|c 2022
|b IOP Publ.
336 7 _ |a article
|2 DRIVER
336 7 _ |a Output Types/Journal article
|2 DataCite
336 7 _ |a Journal Article
|b journal
|m journal
|0 PUB:(DE-HGF)16
|s 1675429821_29945
|2 PUB:(DE-HGF)
336 7 _ |a ARTICLE
|2 BibTeX
336 7 _ |a JOURNAL_ARTICLE
|2 ORCID
336 7 _ |a Journal Article
|0 0
|2 EndNote
520 _ _ |a JUNO is a multi-purpose neutrino observatory under construction in the south of China. This publication presents new sensitivity estimates for the measurement of the ∆m$^2_{31}$, ∆m$^2_{21}$, sin$^2θ_{12}$, and sin$^2θ_{13}$ oscillation parameters using reactor antineutrinos, which is one of the primary physics goals of the experiment. The sensitivities are obtained using the best knowledge available to date on the location and overburden of the experimental site, the nuclear reactors in the surrounding area and beyond, the detector response uncertainties, and the reactor antineutrino spectral shape constraints expected from the TAO satellite detector. It is found that the ∆m$^2_{21}$ and sin$^2θ_{12}$ oscillation parameters will be determined to better than 0.5% precision in six years of data collection. In the same period, the ∆m$^2_{31}$ parameter willbe determined to about 0.2% precision for each mass ordering hypothesis. The new precision represents approximately an order of magnitude improvement over existing constraints for these three parameters.
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
700 1 _ |a Göttel, Alexandre
|0 P:(DE-Juel1)177019
|b 1
700 1 _ |a Kampmann, Philipp
|0 P:(DE-Juel1)171633
|b 2
700 1 _ |a Liu, Runxuan
|0 P:(DE-Juel1)179374
|b 3
700 1 _ |a Ludhova, Livia
|0 P:(DE-Juel1)168122
|b 4
700 1 _ |a Pelicci, Luca
|0 P:(DE-Juel1)186943
|b 5
700 1 _ |a Rifai, Mariam
|0 P:(DE-Juel1)185809
|b 6
700 1 _ |a Schever, Michaela
|0 P:(DE-Juel1)169445
|b 7
700 1 _ |a Settanta, Giulio
|0 P:(DE-Juel1)180506
|b 8
700 1 _ |a Vollbrecht, Moritz Cornelius
|0 P:(DE-Juel1)179551
|b 9
773 _ _ |a 10.1088/1674-1137/ac8bc9
|0 PERI:(DE-600)2491278-5
|p 123001
|t Chinese physics / C
|v 46
|y 2022
|x 0254-3052
856 4 _ |u https://juser.fz-juelich.de/record/911312/files/Abusleme_2022_Chinese_Phys._C_46_123001.pdf
|y OpenAccess
909 C O |o oai:juser.fz-juelich.de:911312
|p openaire
|p open_access
|p VDB
|p driver
|p dnbdelivery
910 1 _ |a Forschungszentrum Jülich
|0 I:(DE-588b)5008462-8
|k FZJ
|b 1
|6 P:(DE-Juel1)177019
910 1 _ |a Forschungszentrum Jülich
|0 I:(DE-588b)5008462-8
|k FZJ
|b 3
|6 P:(DE-Juel1)179374
910 1 _ |a Forschungszentrum Jülich
|0 I:(DE-588b)5008462-8
|k FZJ
|b 4
|6 P:(DE-Juel1)168122
910 1 _ |a Forschungszentrum Jülich
|0 I:(DE-588b)5008462-8
|k FZJ
|b 5
|6 P:(DE-Juel1)186943
910 1 _ |a Forschungszentrum Jülich
|0 I:(DE-588b)5008462-8
|k FZJ
|b 6
|6 P:(DE-Juel1)185809
910 1 _ |a Forschungszentrum Jülich
|0 I:(DE-588b)5008462-8
|k FZJ
|b 9
|6 P:(DE-Juel1)179551
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 2022
915 _ _ |a Creative Commons Attribution CC BY 3.0
|0 LIC:(DE-HGF)CCBY3
|2 HGFVOC
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0200
|2 StatID
|b SCOPUS
|d 2022-11-13
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0150
|2 StatID
|b Web of Science Core Collection
|d 2022-11-13
915 _ _ |a JCR
|0 StatID:(DE-HGF)0100
|2 StatID
|b CHINESE PHYS C : 2021
|d 2022-11-13
915 _ _ |a WoS
|0 StatID:(DE-HGF)0113
|2 StatID
|b Science Citation Index Expanded
|d 2021-01-27
915 _ _ |a OpenAccess
|0 StatID:(DE-HGF)0510
|2 StatID
915 _ _ |a IF < 5
|0 StatID:(DE-HGF)9900
|2 StatID
|d 2022-11-13
915 _ _ |a SCOAP3
|0 StatID:(DE-HGF)0570
|2 StatID
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0571
|2 StatID
|b SCOAP3 sponsored Journal
|d 2021-01-27
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)1150
|2 StatID
|b Current Contents - Physical, Chemical and Earth Sciences
|d 2022-11-13
915 _ _ |a National-Konsortium
|0 StatID:(DE-HGF)0430
|2 StatID
|d 2022-11-13
|w ger
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0160
|2 StatID
|b Essential Science Indicators
|d 2021-01-27
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0199
|2 StatID
|b Clarivate Analytics Master Journal List
|d 2022-11-13
920 _ _ |l yes
920 1 _ |0 I:(DE-Juel1)IKP-2-20111104
|k IKP-2
|l Experimentelle Hadrondynamik
|x 0
980 _ _ |a journal
980 _ _ |a VDB
980 _ _ |a UNRESTRICTED
980 _ _ |a I:(DE-Juel1)IKP-2-20111104
980 1 _ |a FullTexts


LibraryCollectionCLSMajorCLSMinorLanguageAuthor
Marc 21