000897153 001__ 897153
000897153 005__ 20211104141509.0
000897153 0247_ $$2Handle$$a2128/28877
000897153 037__ $$aFZJ-2021-03643
000897153 041__ $$aEnglish
000897153 1001_ $$0P:(DE-Juel1)177019$$aGöttel, Alexandre$$b0$$eCorresponding author
000897153 1112_ $$a2021 European Physical Society Conference on High Energy Physics$$cOnline (Hamburg)$$d2021-07-26 - 2021-07-30$$wGermany
000897153 245__ $$aJUNO potential in non-oscillation physics
000897153 260__ $$c2021
000897153 3367_ $$033$$2EndNote$$aConference Paper
000897153 3367_ $$2DataCite$$aOther
000897153 3367_ $$2BibTeX$$aINPROCEEDINGS
000897153 3367_ $$2DRIVER$$aconferenceObject
000897153 3367_ $$2ORCID$$aLECTURE_SPEECH
000897153 3367_ $$0PUB:(DE-HGF)6$$2PUB:(DE-HGF)$$aConference Presentation$$bconf$$mconf$$s1636007609_4688$$xPanel discussion
000897153 520__ $$aThe Jiangmen Underground Neutrino Observatory (JUNO) is a next-generation liquid scintillator experiment being built in Guangdong province in China. JUNO's target mass of 20 kton will be contained in a 35.4 m acrylic vessel, itself submerged in a water pool, under about 650 m of granite overburden. Surrounding the acrylic vessel are 17612 20'' PMTs and 25600 3'' PMTs. The main goal of JUNO, whose construction is scheduled for completion in 2022, is a 3-4σ determination of the neutrino mass ordering (MO) using reactor neutrinos within six years, as well as a precise measurement of $θ_{12}$, $δM^2_{21}$, and $δM^2_{31}$.JUNO's large target mass, low background, and dual calorimetry, leading to an excellent energy resolution and low threshold, allows for a rich physics program with many applications in neutrino physics. The large target mass will allow for high-statistics solar-, geo-, and atmospheric neutrino measurements. JUNO will also be able to measure neutrinos from galactic core-collapse supernovae, detecting about 10,000 events for a supernova at 10 kpc, and achieve a 3σ discovery of the diffuse supernova neutrino background in ten years. It can also study non-standard interactions e.g. proton decay, indirect dark matter searches, and probe for lorentz invariance violations. This talk will cover this extensive range of non-oscillation topics on which JUNO will be able to shed light.
000897153 536__ $$0G:(DE-HGF)POF4-612$$a612 - Cosmic Matter in the Laboratory (POF4-612)$$cPOF4-612$$fPOF IV$$x0
000897153 8564_ $$uhttps://juser.fz-juelich.de/record/897153/files/EPS_HEP.pdf$$yOpenAccess
000897153 909CO $$ooai:juser.fz-juelich.de:897153$$popenaire$$popen_access$$pVDB$$pdriver
000897153 9101_ $$0I:(DE-588b)5008462-8$$6P:(DE-Juel1)177019$$aForschungszentrum Jülich$$b0$$kFZJ
000897153 9131_ $$0G:(DE-HGF)POF4-612$$1G:(DE-HGF)POF4-610$$2G:(DE-HGF)POF4-600$$3G:(DE-HGF)POF4$$4G:(DE-HGF)POF$$aDE-HGF$$bForschungsbereich Materie$$lMatter and the Universe$$vCosmic Matter in the Laboratory$$x0
000897153 9141_ $$y2021
000897153 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess
000897153 920__ $$lyes
000897153 9201_ $$0I:(DE-Juel1)IKP-2-20111104$$kIKP-2$$lExperimentelle Hadrondynamik$$x0
000897153 9801_ $$aFullTexts
000897153 980__ $$aconf
000897153 980__ $$aVDB
000897153 980__ $$aUNRESTRICTED
000897153 980__ $$aI:(DE-Juel1)IKP-2-20111104