Hauptseite > Publikationsdatenbank > JUNO potential in non-oscillation physics > print

001     911292
005     20221114130838.0
024 7 _ |a 10.22323/1.398.0229
|2 doi
024 7 _ |a 2128/32539
|2 Handle
037 _ _ |a FZJ-2022-04585
100 1 _ |a Göttel, Alexandre
|0 P:(DE-Juel1)177019
|b 0
|e Corresponding author
|u fzj
111 2 _ |a The European Physical Society Conference on High Energy Physics
|c Online conference
|d 2021-07-26 - 2021-07-30
|w jointly organized by Universität Hamburg and the research center DESY
245 _ _ |a JUNO potential in non-oscillation physics
260 _ _ |c 2022
|b Sissa Medialab Trieste, Italy
295 1 0 |a Proceedings of The European Physical Society Conference on High Energy Physics — PoS(EPS-HEP2021) - Sissa Medialab Trieste, Italy, 2022. - ISBN - doi:10.22323/1.398.0229
300 _ _ |a Volume 398
336 7 _ |a CONFERENCE_PAPER
|2 ORCID
336 7 _ |a Conference Paper
|0 33
|2 EndNote
336 7 _ |a INPROCEEDINGS
|2 BibTeX
336 7 _ |a conferenceObject
|2 DRIVER
336 7 _ |a Output Types/Conference Paper
|2 DataCite
336 7 _ |a Contribution to a conference proceedings
|b contrib
|m contrib
|0 PUB:(DE-HGF)8
|s 1668416296_11751
|2 PUB:(DE-HGF)
336 7 _ |a Contribution to a book
|0 PUB:(DE-HGF)7
|2 PUB:(DE-HGF)
|m contb
520 _ _ |a The Jiangmen Underground Neutrino Observatory (JUNO) is a next-generation liquid scintillator experiment being built in the Guangdong province in China. JUNO's target mass of 20 kton will be contained in a 35.4 m acrylic vessel, itself submerged in a water pool, under about 700 m of granite overburden. Surrounding the acrylic vessel are 17612 20'' PMTs and 25600 3'' PMTs. The main goal of JUNO, whose construction is scheduled for completion in 2022, is a 3-4σ determination of the neutrino mass ordering (MO) using reactor neutrinos within six years, as well as a precise measurement of $θ_{12}$, $Δm^2_{21}$, and $Δm^2_{31}$. JUNO's large target mass, low background, and dual calorimetry, leading to an excellent energy resolution and low threshold, allows for a rich physics program with many applications in neutrino physics. The large target mass will allow for high-statistics solar-, geo-, and atmospheric neutrino measurements. JUNO will also be able to measure neutrinos from galactic core-collapse supernovae, detecting about 10,000 events for a supernova at 10 kpc, and achieve a 3σ discovery of the diffuse supernova neutrino background in ten years. It can also study non-standard interactions e.g. proton decay, indirect dark matter searches, and probe for Lorentz invariance violations. This paper covers this extensive range of non-oscillation topics on which JUNO will be able to shed light.
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 CrossRef Conference
773 _ _ |a 10.22323/1.398.0229
856 4 _ |u https://juser.fz-juelich.de/record/911292/files/EPS-HEP2021_229.pdf
|y OpenAccess
909 C O |o oai:juser.fz-juelich.de:911292
|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 0
|6 P:(DE-Juel1)177019
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 OpenAccess
|0 StatID:(DE-HGF)0510
|2 StatID
920 _ _ |l yes
920 1 _ |0 I:(DE-Juel1)IKP-2-20111104
|k IKP-2
|l Experimentelle Hadrondynamik
|x 0
980 _ _ |a contrib
980 _ _ |a VDB
980 _ _ |a UNRESTRICTED
980 _ _ |a contb
980 _ _ |a I:(DE-Juel1)IKP-2-20111104
980 1 _ |a FullTexts

LibraryCollectionCLSMajorCLSMinorLanguageAuthor
Marc 21