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Title: Neutrino physics with JUNO

Journal Article · · Journal of Physics. G, Nuclear and Particle Physics
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The Jiangmen Underground Neutrino Observatory (JUNO), a 20 kton multi-purpose underground liquid scintillator detector, was proposed with the determination of the neutrino mass hierarchy (MH) as a primary physics goal. The excellent energy resolution and the large fiducial volume anticipated for the JUNO detector offer exciting opportunities for addressing many important topics in neutrino and astro-particle physics. In this document, we present the physics motivations and the anticipated performance of the JUNO detector for various proposed measurements. Following an introduction summarizing the current status and open issues in neutrino physics, we discuss how the detection of antineutrinos generated by a cluster of nuclear power plants allows the determination of the neutrino MH at a 3–4σ significance with six years of running of JUNO. The measurement of antineutrino spectrum with excellent energy resolution will also lead to the precise determination of the neutrino oscillation parameters $${\mathrm{sin}}^{2}{\theta }_{12}$$, $${\rm{\Delta }}{m}_{21}^{2}$$, and $$| {\rm{\Delta }}{m}_{{ee}}^{2}| $$ to an accuracy of better than 1%, which will play a crucial role in the future unitarity test of the MNSP matrix. The JUNO detector is capable of observing not only antineutrinos from the power plants, but also neutrinos/antineutrinos from terrestrial and extra-terrestrial sources, including supernova burst neutrinos, diffuse supernova neutrino background, geoneutrinos, atmospheric neutrinos, and solar neutrinos. As a result of JUNO's large size, excellent energy resolution, and vertex reconstruction capability, interesting new data on these topics can be collected. For example, a neutrino burst from a typical core-collapse supernova at a distance of 10 kpc would lead to ~5000 inverse-beta-decay events and ~2000 all-flavor neutrino–proton ES events in JUNO, which are of crucial importance for understanding the mechanism of supernova explosion and for exploring novel phenomena such as collective neutrino oscillations. Detection of neutrinos from all past core-collapse supernova explosions in the visible universe with JUNO would further provide valuable information on the cosmic star-formation rate and the average core-collapse neutrino energy spectrum. Antineutrinos originating from the radioactive decay of uranium and thorium in the Earth can be detected in JUNO with a rate of ~400 events per year, significantly improving the statistics of existing geoneutrino event samples. Atmospheric neutrino events collected in JUNO can provide independent inputs for determining the MH and the octant of the $${\theta }_{23}$$ mixing angle. Detection of the 7Be and 8B solar neutrino events at JUNO would shed new light on the solar metallicity problem and examine the transition region between the vacuum and matter dominated neutrino oscillations. Regarding light sterile neutrino topics, sterile neutrinos with $${10}^{-5}\;{{\rm{eV}}}^{2}\lt {\rm{\Delta }}{m}_{41}^{2}\lt {10}^{-2}\;{{\rm{eV}}}^{2}$$ and a sufficiently large mixing angle $${\theta }_{14}$$ could be identified through a precise measurement of the reactor antineutrino energy spectrum. Meanwhile, JUNO can also provide us excellent opportunities to test the eV-scale sterile neutrino hypothesis, using either the radioactive neutrino sources or a cyclotron-produced neutrino beam. The JUNO detector is also sensitive to several other beyondthe-standard-model physics. Examples include the search for proton decay via the $$p\to {K}^{+}+\bar{\nu }$$ decay channel, search for neutrinos resulting from dark-matter annihilation in the Sun, search for violation of Lorentz invariance via the sidereal modulation of the reactor neutrino event rate, and search for the effects of non-standard interactions. The proposed construction of the JUNO detector will provide a unique facility to address many outstanding crucial questions in particle and astrophysics in a timely and cost-effective fashion. Furthermore, it holds the great potential for further advancing our quest to understanding the fundamental properties of neutrinos, one of the building blocks of our Universe.

Research Organization:
Brookhaven National Laboratory (BNL), Upton, NY (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP)
Grant/Contract Number:
SC00112704
OSTI ID:
1354633
Report Number(s):
BNL-113776-2017-JA; R&D Project: PO-022; KA2201020
Journal Information:
Journal of Physics. G, Nuclear and Particle Physics, Vol. 43, Issue 3; ISSN 0954-3899
Publisher:
IOP PublishingCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 388 works
Citation information provided by
Web of Science

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New results from DAMA/LIBRA journal March 2010
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Historical Supernovae book January 2003
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Precise Measurement of the Neutrino Mixing Parameter θ 23 from Muon Neutrino Disappearance in an Off-Axis Beam journal May 2014
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Analytic approximations for three neutrino oscillation parameters and probabilities in matter journal July 2001
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The Cosmic Core-collapse Supernova Rate does not match the Massive-Star Formation Rate text January 2011
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Antineutrino astronomy and geophysics journal July 1984
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Solar Neutrinos journal January 2013
Determination of neutrino mass hierarchy and θ 13 with a remote detector of reactor antineutrinos journal October 2008
Observation of geo-neutrinos journal April 2010
Standard Solar Composition journal January 1998
Search for Neutrinos from the Sun journal May 1968
Present Status of the Theoretical Predictions for the Cl 37 Solar-Neutrino Experiment journal May 1968
Dark Matter Candidates from Particle Physics and Methods of Detection text January 2010
Tests of the standard electroweak model in nuclear beta decay journal September 2006
The solar chemical composition journal October 2006
Leptogenesis for Pedestrians text January 2004
Complete results for five years of GNO solar neutrino observations journal June 2005
Mimicking diffuse supernova antineutrinos with the sun as a source journal April 2010
The Borexino detector at the Laboratori Nazionali del Gran Sasso
  • Alimonti, G.; Arpesella, C.; Back, H.
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Neutrino Scattering on Atomic Electrons in Searches for the Neutrino Magnetic Moment journal November 2010
Uncertainties in the anti-neutrino production at nuclear reactors journal March 2009
Results from a Search for Light-Mass Dark Matter with a P-type Point Contact Germanium Detector text January 2010
Presupernova Evolution of Massive Single and Binary Stars journal September 2012
Supernova Relic Neutrino search with neutron tagging at Super-Kamiokande-IV journal January 2015
Solar Neutrinos: Status and Prospects journal August 2013
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Search for νμ→νe oscillations in the NOMAD experiment journal September 2003
Erratum to “Golden measurements at a neutrino factory” journal January 2001
First Results from KamLAND: Evidence for Reactor Antineutrino Disappearance text January 2003
Microscopic theories of neutrino- 12 C reactions journal May 2000
Detecting the diffuse supernova neutrino background with LENA journal February 2015
Two-dimensional hydrodynamic core-collapse supernova simulations with spectral neutrino transport: II. Models for different progenitor stars journal September 2006
Antineutrino background from spent-fuel storage in sensitive searches for θ 13 at reactors journal February 2006
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Sterile neutrinos: the dark side of the light fermions text January 2009
The next-generation liquid-scintillator neutrino observatory LENA journal June 2012
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The Diffuse Supernova Neutrino Background journal November 2010
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Neutrino Mass Ordering from Oscillations and Beyond: 2018 Status and Future Prospects journal October 2018
sin2 θ W estimate and bounds on nonstandard interactions at source and detector in the solar neutrino low-energy regime journal July 2017
Muon tracking with the fastest light in the JUNO central detector journal March 2018
Extracting Majorana properties from strong bounds on neutrinoless double beta decay journal February 2017
Laser calibration system in JUNO journal January 2019
CP symmetries as guiding posts: revamping tri-bi-maximal mixing. Part I journal March 2019
DarkSide-20k: A 20 tonne two-phase LAr TPC for direct dark matter detection at LNGS journal March 2018
The design of the small prototype for the central detector of JUNO journal August 2018
CP Symmetries as Guiding Posts: Revamping Tri-Bi-Maximal Mixing-I text January 2018
The development of $$^{222}\hbox {Rn}$$222Rn detectors for JUNO prototype journal January 2018
CP-violation and non-standard interactions at the MOMENT journal July 2016
Constraining the nonstandard interaction parameters in long baseline neutrino experiments journal March 2016
Implications of residual C P symmetry for leptogenesis in a model with two right-handed neutrinos journal October 2017
Assessing the viability of A 4 , S 4 , and A 5 flavor symmetries for description of neutrino mixing journal June 2018
Constraint on the solar Δ m 2 using 4000 days of short baseline reactor neutrino data journal December 2019
Non-negligible oscillation effects in the crustal geoneutrino calculations journal December 2019
Quark and lepton mixing patterns from a common discrete flavor symmetry with a generalized C P symmetry journal September 2018
Lepton mixing predictions from S 4 in the tridirect C P approach to two right-handed neutrino models journal April 2019
Neutrino versus antineutrino oscillation parameters at DUNE and Hyper-Kamiokande experiments journal November 2017
Neutrino-nucleus cross-sections at supernova neutrino energies text January 2017
Development of an analysis to probe the neutrino mass ordering with atmospheric neutrinos using three years of IceCube DeepCore data: IceCube Collaboration journal January 2020
Study on the radon removal for the water system of Jiangmen Underground Neutrino Observatory journal September 2018
Radioactive contamination of scintillators journal March 2018
Improved statistical determination of absolute neutrino masses via radiative emission of neutrino pairs from atoms journal June 2016
Looking into analytical approximations for three-flavor neutrino oscillation probabilities in matter journal December 2016
Nonstandard interactions and resolving the ordering of neutrino masses at DUNE and other long baseline experiments journal September 2016
Lepton Number Violation: Seesaw Models and Their Collider Tests journal May 2018
Electroweak symmetric dark matter balls journal September 2019
Development of an analysis to probe the neutrino mass ordering with atmospheric neutrinos using three years of IceCube DeepCore data text January 2020
Alternative schemes of predicting lepton mixing parameters from discrete flavor and C P symmetry journal January 2017
Radioactive contamination of scintillators text January 2018
Presupernova neutrino events relating to the final evolution of massive stars text January 2016
Supernova neutrino physics with xenon dark matter detectors: A timely perspective text January 2016
Neutrino spin and spin-flavor oscillations in transversal matter currents with standard and nonstandard interactions journal December 2018
Pinpointing astrophysical bursts of low-energy neutrinos embedded into the noise journal August 2018
PandaX-III: Searching for neutrinoless double beta decay with high pressure 136Xe gas time projection chambers journal April 2017
Lepton mixing predictions from infinite group series D 9n, 3n (1) with generalized CP journal May 2016
Sterile neutrino search at NEOS Experiment text January 2016
Confronting tridirect C P -symmetry models with neutrino oscillation experiments journal September 2019
Strong Bayesian evidence for the normal neutrino hierarchy journal June 2017
Neutrino signals of core-collapse supernovae in underground detectors journal August 2018
Combined sensitivity to the neutrino mass ordering with JUNO, the IceCube Upgrade, and PINGU journal February 2020
Neutrinos from Beta Processes in a Presupernova: Probing the Isotopic Evolution of a Massive Star journal December 2017

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