Abstract

After a long a glorious history, marked by the first direct proofs of neutrino existence and of the mixing between the first and third neutrino generations, the reactor antineutrino experiments are still well alive and will continue to give important contributions to the development of elementary particle physics and astrophysics. In parallel to the SBL (short baseline) experiments, that will be dedicated mainly to the search for sterile neutrinos, a new kind of experiments will start playing an important role: reactor experiments with a “medium” value, around 50 km, of the baseline, somehow in the middle between the SBL and the LBL (long baselines), like KamLAND, which in the recent past gave essential contributions to the developments of neutrino physics. These new medium baseline reactor experiments can be very important, mainly for the study of neutrino mass ordering. The first example of this kind, the liquid scintillator JUNO experiment, characterized by a very high mass and an unprecedented energy resolution, will soon start data collecting in China. Its main aspects are discussed here, together with its potentialities for what concerns the mass ordering investigation and also the other issues that can be studied with this detector, spanning from the accurate oscillation parameter determination to the study of solar neutrinos, geoneutrinos, atmospheric neutrinos and neutrinos emitted by supernovas and to the search for signals of potential Lorentz invariance violation.

Highlights

  • IntroductionThe nuclear power plants are an ideal source of pure and intense electron antineutrino (νe ) beams, emitted in the radioactive decays of the fissile products of the nuclear fission

  • Milestones of Reactor Antineutrino ExperimentsThe nuclear power plants are an ideal source of pure and intense electron antineutrino beams, emitted in the radioactive decays of the fissile products of the nuclear fission

  • The main recent contribution of short baseline experiments (SBL) experiments to the knowledge of neutrino physics has been for sure the proof that the mixing angle between the first and third neutrino generations (θ13 )

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Summary

Introduction

The nuclear power plants are an ideal source of pure and intense electron antineutrino (νe ) beams, emitted in the radioactive decays of the fissile products of the nuclear fission. As a matter of fact, hints of a possible events deficit, with respect to the theoretical predictions in absence of oscillation, seem to come by more recent reanalyses of the first SBL reactor experiments data, in the light of new more precise determination of antineutrino fluxes [11,12], that predicted a systematic increase of the flux above 2 MeV. An important milestone of reactor experiments history, which had a great impact on all neutrino physics, has been the study of the 1–2 mixing sector performed, since the first years of the new millennium, by KamLAND [19] This experiment, that used a 1kton liquid scintillator detector located at the enlarged Kamiokande site, was a long-baseline (LBL) experiment, with a medium distance (from the 51 different reactors producing the νe flux to the detector) of the order of 200 km. We will finish our paper with a critical summary of the main achievements of reactor neutrino physics and a brief discussion of the challenges they could face in the near future

Short-Baseline Reactor Experiments
Recent Results of the SBL Experiments
Open Issues in SBL Reactor Experiments
Future of Reactor Neutrino Experiments
The Neutrino Mass Ordering
Present Status of the Mass Ordering Determination
Reactor Neutrino Physics and Mass Ordering Determination
The JUNO Experiment and Its Potentialities
The JUNO Detector Main Features
Mass Ordering Study with JUNO Experiment
Mass and Mixing Parameters Measurement
Solar Neutrino Physics at JUNO
Geoneutrinos and SuperNova Neutrinos Measurements with a Reactor Experiment
Atmospheric Neutrino Studies at JUNO
Search for LIV Signals and Other Exotic Studies at JUNO
Discussion and Conclusions
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