Neutrino Astrophysics with JUNO

Lorenz, Sebastian; JUNO Collaboration

Contribution to a conference proceedings/Contribution to a book

PUBDB-2016-05619

Neutrino Astrophysics with JUNO

Lorenz, S. ; JUNO Collaboration (Collaboration author)

2016
Verlag Deutsches Elektronen-Synchrotron Hamburg
ISBN: 978-3-945931-08-0

Lorenz, Sebastian "Neutrino Astrophysics with JUNO" in Proceedings, Magellan Workshop: Connecting Neutrino Physics and Astronomy / Dahmke, Stefan K.G., Meyer, Mikko, Vanhoefer, Laura (eds.), Deutsches Elektronen-Synchrotron, DESY : 2016 ; Magellan Workshop, 2016-03-17 - 2016-03-18, Hamburg
Magellan Workshop, Hamburg, Germany, 17 Mar 2016 - 18 Mar 2016 Hamburg : Verlag Deutsches Elektronen-Synchrotron, DESY-PROC 121-128 (2016) [10.3204/DESY-PROC-2016-05/20]

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Please use a persistent id in citations: doi:10.3204/DESY-PROC-2016-05/20

Abstract: The Jiangmen Underground Neutrino Observatory will aim for the determination of the neutrino mass hierarchy with a medium baseline reactor $\overline{\nu}_e$ oscillation experiment. With its 20\,kt liquid scintillator detector, it will also be sensitive to astrophysical low-energy neutrinos. In case of a typical galactic core-collapse supernova, $\sim5000$ neutrino interactions will be detected via the inverse beta decay alone. Moreover, a $3\sigma$ evidence for the diffuse supernova neutrino background seems within reach after ten years of measurement. The performance of the experiment's solar neutrino program will decisively depend on the achieved radiopurity and cosmogenic background rejection efficiency.

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