001018463 001__ 1018463 001018463 005__ 20231128201905.0 001018463 0247_ $$2datacite_doi$$a10.34734/FZJ-2023-04826 001018463 037__ $$aFZJ-2023-04826 001018463 041__ $$aEnglish 001018463 1001_ $$0P:(DE-Juel1)196820$$aMalyshkin, Yury$$b0$$ufzj 001018463 1112_ $$aInternational Workshop on Multi-messenger Tomography of the Earth$$cParis$$d2023-07-03 - 2023-07-07$$wFrance 001018463 245__ $$aJUNO's Perspective for Geoneutrinos 001018463 260__ $$c2023 001018463 3367_ $$033$$2EndNote$$aConference Paper 001018463 3367_ $$2DataCite$$aOther 001018463 3367_ $$2BibTeX$$aINPROCEEDINGS 001018463 3367_ $$2DRIVER$$aconferenceObject 001018463 3367_ $$2ORCID$$aLECTURE_SPEECH 001018463 3367_ $$0PUB:(DE-HGF)6$$2PUB:(DE-HGF)$$aConference Presentation$$bconf$$mconf$$s1701168982_28677$$xInvited 001018463 520__ $$aJiangmen Underground Neutrino Observatory (JUNO) is a neutrino experiment being built in Southern China to measure neutrinos produced in nuclear power plants at a distance of 52.5 km. Having the main goal to improve the knowledge about neutrino oscillations, fundamental properties of these particles, JUNO will also be able to observe neutrinos of natural origin such as from the Sun, supernovae, the Earth atmosphere and its interior. The latter are called geoneutrinos and can serve as a proxy for investigation of the Earth’s radiogenic heat. Using inverse beta-decay as the detection channel, JUNO is sensitive to geoneutrinos produced in beta-decays of U-238 and Th-232 radioactive isotopes. JUNO will collect in one year about 400 geoneutrinos, what is more than the present-day statistics measured by Borexino and KamLAND together. This talk will report the JUNO expected sensitivity to geoneutrino measurement including some preliminary results of an updated analysis. 001018463 536__ $$0G:(DE-HGF)POF4-612$$a612 - Cosmic Matter in the Laboratory (POF4-612)$$cPOF4-612$$fPOF IV$$x0 001018463 8564_ $$uhttps://indico.in2p3.fr/event/30001/ 001018463 8564_ $$uhttps://juser.fz-juelich.de/record/1018463/files/2023-07-06%20%5BMMTE%5D%20Geoneutrino%20Sensitivity%20of%20JUNO.pdf$$yOpenAccess 001018463 909CO $$ooai:juser.fz-juelich.de:1018463$$popenaire$$popen_access$$pVDB$$pdriver 001018463 9101_ $$0I:(DE-588b)5008462-8$$6P:(DE-Juel1)196820$$aForschungszentrum Jülich$$b0$$kFZJ 001018463 9131_ $$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$$x0 001018463 9141_ $$y2023 001018463 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess 001018463 9201_ $$0I:(DE-Juel1)IKP-2-20111104$$kIKP-2$$lExperimentelle Hadrondynamik$$x0 001018463 9801_ $$aFullTexts 001018463 980__ $$aconf 001018463 980__ $$aVDB 001018463 980__ $$aUNRESTRICTED 001018463 980__ $$aI:(DE-Juel1)IKP-2-20111104