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024 7 _ |a 10.1088/1742-6596/1586/1/012034
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024 7 _ |a 2128/27063
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037 _ _ |a FZJ-2021-00811
041 _ _ |a English
082 _ _ |a 530
100 1 _ |a Ludhova, Livia
|0 P:(DE-Juel1)168122
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111 2 _ |a DISCRETE 2018
|g DISCRETE 2019
|c Vienna
|d 2018-11-26 - 2018-11-30
|w Austria
245 _ _ |a Overview on solar, geo, and reactor neutrino experiments
260 _ _ |a Bristol
|c 2020
|b IOP Publ.
300 _ _ |a 1-8
336 7 _ |a CONFERENCE_PAPER
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520 _ _ |a Neutrino 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.
536 _ _ |a 612 - Cosmic Matter in the Laboratory (POF3-612)
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773 _ _ |a 10.1088/1742-6596/1586/1/012034
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856 4 _ |u https://juser.fz-juelich.de/record/890224/files/Ludhova_2020_J._Phys.%20_Conf._Ser._1586_012034.pdf
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914 1 _ |y 2020
915 _ _ |a Creative Commons Attribution CC BY 3.0
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