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000890224 037__ $$aFZJ-2021-00811
000890224 041__ $$aEnglish
000890224 082__ $$a530
000890224 1001_ $$0P:(DE-Juel1)168122$$aLudhova, Livia$$b0$$eCorresponding author
000890224 1112_ $$aDISCRETE 2018$$cVienna$$d2018-11-26 - 2018-11-30$$gDISCRETE 2019$$wAustria
000890224 245__ $$aOverview on solar, geo, and reactor neutrino experiments
000890224 260__ $$aBristol$$bIOP Publ.$$c2020
000890224 300__ $$a1-8
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000890224 520__ $$aNeutrino physics has made a substantial progress in recent years: ranging from the discovery of new phenomena, as neutrino oscillations, up to the development of milestone experimental techniques, going, at the end, hand-in-hand. Today, we are able to do precision neutrino physics, as well as we have succeeded in using neutrinos as new tools to gain information about astrophysical objects. In spite of this enormous progress, many fundamental questions remain unanswered. This contribution concentrates on low-energy MeV neutrinos emitted from our Sun, along the radioactive decays inside the Earth (geoneutrinos), and reactor neutrinos. For each of these three fields, the present-day motivation, open questions, as well as the latest experimental results and future perspectives are discussed.
000890224 536__ $$0G:(DE-HGF)POF3-612$$a612 - Cosmic Matter in the Laboratory (POF3-612)$$cPOF3-612$$fPOF III$$x0
000890224 773__ $$0PERI:(DE-600)2166409-2$$a10.1088/1742-6596/1586/1/012034$$p012034$$tJournal of physics / Conference Series$$v1586$$x1742-6588$$y2020
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