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modules outside the cross. The height and width of the arms are 10 metres (33 ft). A single module consists of alternating layers of iron and a plastic scintillator. An additional 4 veto layers of the scintillator surround the module on the sides to distinguish particles entering from the outside from those produced by interactions inside the module. The total mass of iron in one module is 7.1 tons and constitutes 96% of the module weight. On the neutrino beam axis, in the middle of the cross between the vertical and horizontal arm, there is an additional module built only from layers of the plastic scintillator (Proton Module) with a mass of 0.55 tons. Its purpose is to register quasielastic interactions and compare the obtained results with the simulations.
2013:. The fraction of neutrons that will be captured in SK is 50% for 0.01% Gd concentration and 90% for 0.1% concentration – the planned final Gd concentration in SK. The signal from neutron capture is delayed by a fraction of a millisecond (the time the neutron travels across the water before the capture plus the time when Gd remains in the excited state) with respect to the charged lepton signal and usually appears within a distance of 50 cm (the distance travelled by the neutron before the capture) from the neutrino interaction point. Such a double flash event (the first flash from the charged lepton, the second flash from the Gd deexcitation photons) is a signature of an antineutrino interaction.
1713:
additional final state particles: high angle particles thanks to the increased angular acceptance, and less energetic particles because of lower detection thresholds. This detector acceptance improvement is important to cover almost the same phase space available at the far detector (SK). In addition, final state particles will allow probing nuclear effects which are essential for constraining the systematic effects of the oscillation analysis. It is an important step as well in the transition to using semi-inclusive or exclusive models in neutrino oscillation physics, as opposed to current inclusive models which use only the final state lepton in their predictions.
881:) Detector (P0D) contains 40 plastic scintillator module planes, which in the central part are interleaved with 2.8 cm thick bags fillable of water and thick brass sheets, and in two peripheral regions scintillator modules are sandwiched with lead sheets. By comparison of the amount of interaction between modes with and without water in the bags, it is possible to extract the number of neutrino interactions occurring on the water – the target material inside the far detector Super-Kamiokande. The size of the entire active P0D volume is around 2.1 m × 2.2 m × 2.4 m (X×Y×Z) and its mass with and without water is 15.8 and 12.9 tons respectively.
106:. The properties and composition of the neutrino flux are first measured by a system of near detectors located 280 metres (920 ft) from the beam production place at the J-PARC site, and then again in the Super-Kamiokande detector. Comparison of the content of different neutrino flavours in these two locations allows measurement of the oscillations probability on the way between near and far detectors. Super-Kamiokande is able to detect interactions of both, muon and electron neutrinos, and thus measure the disappearance of muon neutrino flux, as well as electron neutrino appearance in the beam.
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1627:
maintain their sandwiched structure and continue to detect forward going leptons and high momentum hadrons. The upstream part which now hosts the P0D sub-detector will be replaced by three novel sub-detectors: a scintillating 3D target (Super Fine-Grained
Detector or SuperFGD), two new TPCs on top and below the SuperFGD (High-Angle TPCs or HATPCs), and six Time-of-Flight (TOF) detectors surrounding the new structure. Each of these sub-detectors is briefly described below. The installation of the new sub-detectors into ND280 will be done in 2022.
551:
1054:
565:
539:
856:
822:
810:
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757:
1587:, as well as too high momentum threshold to reconstruct a large part of produced pions and knocked-out nucleons (protons and neutrons). In Charged Current Quasi-Elastic (CCQE) interactions, the dominating interaction in the ND280 near detector, kinematics of produced lepton is enough in the reconstruction of the incoming neutrino energy. However, other types of neutrino interactions in which additional particles (
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1019:
scintillator layers only, while the second FGD is composed of alternating layers of scintillator and water. The second FGD is partially composed of water because the Super-Kamiokande detector is water-based. Cross sections on carbon and on the water can be determined from a comparison of neutrino interactions in the two FGDs.
1985:) is proportional to the particle mass, and in water it equals 0.8 MeV for electrons, 160 MeV for muons and 1400 MeV for protons. Thus, protons released in neutrino interactions often fall below the threshold and remain undetected. Neutron, as a neutral particle, does not produce Cherenkov light. However, it can be
1274:, respectively. Due to relatively large mass, muons usually do not change their direction and thus produce a well-defined cone of Cherenkov light observed by PMTs as a clear, sharp ring. In contrast, electrons, because of smaller mass, are more susceptible to scattering and almost always produce electromagnetic
1626:
The
Upgrade of the ND280 detector (ND280 Upgrade) addresses these requirements by replacing a part of the P0D sub-detector with three types of new sub-detectors. The existing downstream part, consisting of two Fine-Grained scintillation Detectors (FGDs) and three Time Projection Chambers (TPCs), will
1521:
In
February 2020, the proton beam power reached 515 kW with 2.7x10 protons per pulse and with 2.48 seconds between pulses (so-called repetition cycle). To reach 750 kW, the repetition cycle will be reduced to 1.32 s with 2.0x10 protons per pulse, while for 1.3 MW the repetition cycle has to
1379:
The construction of the neutrino beamline started in 2004 and it was successfully commissioned in 2009. Construction of the entire INGRID detector and majority of the ND280 detector (without barrel part of the electromagnetic calorimeter) was completed in 2009. The missing part of the calorimeter was
1649:
designed to detect the light emitted by the particles produced during the interactions in the target. Unlike the current FGDs, the SuperFGD has a three-fold projective 2D readouts providing a quasi-3D readout. This readout configuration increases the detection of short tracks almost uniformly in all
1538:
will also be increased from 250 kA to 320 kA. This will increase the amount of right-sign neutrinos (neutrinos in the neutrino mode beam and anti-neutrinos in the anti-neutrino mode beam) by 10%, and reduce the amount of wrong-sign neutrinos (anti-neutrinos in the neutrino-mode beam and neutrinos in
1157:
The new detector will provide measurements of various charged-current neutrino interaction channels with high precision, lower momentum threshold and full angular acceptance. These will constrain flux and cross-section models uncertainties for the particles produced at high angles. These assets will
1027:
The
Electromagnetic Calorimeter (ECal) surrounds the inner detectors (P0D, TPCs, FGDs) and consists of scintillator layers sandwiched with lead absorber sheets. Its role is to detect neutral particles, especially photons, and measure their energy and direction, as well as to detect charged particles
795:
The main purpose of the INGRID detector is the monitoring of the direction and intensity of the beam on a daily basis by direct detection of neutrino interactions. The INGRID detector consists of 16 identical modules arranged in the shape of a cross, 7 in a vertical and 7 in a horizontal arm, plus 2
721:
far detector and one of the near detectors, ND280. The average energy of neutrinos decreases with the deviation from the beam axis. The off-axis angle was chosen to 2.5° to maximize the probability of oscillation at a distance corresponding to the far detector, which for 295 kilometres (183 mi)
1118:
modules like a sandwich. The modules can be rearranged easily to adapt the magnetic field to the particular needs of the experiment. The magnetic field is created only inside the ferrite so it is very power efficient compared to magnets that have to magnetize empty spaces around them like the ND280
1036:
The Side Muon Range
Detector (SMRD) consists of scintillator modules which are inserted into the gaps in the magnet. The SMRD records muons escaping the inner parts of the detector at large angles with respect to the beam direction. The remaining types of particles (except for neutrinos) are mostly
834:
The ND280 detector is used to measure the flux, energy spectrum and electron neutrino beam pollution for the same off-axis angle as for the far detector. ND280 also investigates various types of muon and electron neutrino and antineutrino interactions. All this allows estimating the expected number
997:
the gas along their track. The ionisation electrons drift from the cathode to the sides of the TPC, where they are detected by the MicroMegas providing a 3D image of a path of the traversing charged particle. Y and Z coordinates are based on the position of the detected ionisation electrons on the
726:
quasielastic interactions, for which it is possible to reconstruct the energy of the interacting neutrino only on the basis of the momentum and direction of the produced charged lepton. The higher neutrino energies are suppressed by the off-axis configuration, decreasing the number of interactions
1712:
The impact the ND280 Upgrade will have on the analyses at T2K is two-fold. Firstly, an increase in statistics thanks to the 2 ton SuperFGD target will allow to nearly double the amount of data in certain samples. Secondly and more relevant, the new configuration will allow for better detection of
838:
ND280 is composed of the set of inner sub-detectors: Pi-Zero detector and a tracker with 2 Fine-Grained
Detectors interleaved with 3 Time Projection Chambers, placed inside of a metal frame called a basket. The basket is surrounded by the electromagnetic calorimeter and a magnet recycled from the
1417:
loaded into the Super-Kamiokande far detector was taken. In 2021–2022 a major upgrade of the neutrino beamline and the ND280 near detector will be performed. From 2023 till 2026 neutrino data will be taken within the second phase of the T2K experiment (T2K-II). In 2027, the successor of the T2K
1018:
Two Fine-Grained
Detectors (FGDs) are placed after the first and second TPCs. Together the FGDs and TPCs make up the tracker of ND280. The FGDs provide the active target mass for the neutrino interactions and are able to measure the short tracks of proton recoil. The first FGD is composed of
1161:
Location at the same distance of 280 meters from the graphite target as ND280 and INGRID detectors, but at a different off-axis angle of 1.5 degrees, causes that the energy spectrum of the neutrino beam is peaked around different energies for each of the off-axis angles corresponding to the
1158:
also facilitate detection of low momentum hadrons produced in the interaction of the neutrino with bounded states of 2 nucleons or through reinteractions inside the target nucleus of particles produced by the neutrino, and thus better modelling of such interactions in the far detector.
1404:
in March 2011. The proton beam power, and thus the neutrino beam intensity, was constantly growing, reaching by
February 2020 the power of 515 kW and a total number of accumulated protons on target of 3.6×10 protons with 55% of data in neutrino-mode and 45% in antineutrino-mode.
746:
WAGASCI-BabyMIND (WAter Grid SCIntillator
Detector – prototype Magnetized Iron Neutrino Detector) is a magnetised neutrino detector located at 1.5° off-axis angle, built to explore the energy spectrum variation with the off-axis angle and cross-sections at higher average neutrino
1546:
and a minor upgrade of the focusing horn power supplies, all of which will be installed during the long shutdown in 2021. Increasing the horn current will require using an additional (third) horn power supply. Meanwhile, the higher proton beam power demands enhancement of the
346:, rejecting at the 3σ (99.7%) significance level almost half of the possible values, ruling out the both CP conserving points at the significance level of 95% and giving a strong hint that CP violation may be large in the neutrino sector. The CP violation is one of the
488:, which is in slight tension with the T2K result. The T2K best-fit point lies in the region disfavoured by NOvA at the confidence level of 90%. There are ongoing works to obtain a joint fit to data from both experiments to quantify consistency between them.
735:
The near detector complex is located at a distance of 280 metres (920 ft) from the graphite target. Its purpose is to measure the neutrino flux before oscillations and to study neutrino interactions. The system consists of three main detectors:
328:(i.e. from −180° to 180°) and can be measured by comparing oscillations of neutrinos to those of antineutrinos. The CP symmetry would be conserved, and thus the oscillation probabilities would be the same for neutrinos and antineutrinos, for
1703:
for each crossing track with a timing resolution of the order of 140 ps. The capability to determine track direction sense has been proven in the actual ND280 to be critical to reduce background generated outside the active inner detectors.
1621:
Finally, the total fiducial volume (the mass available for neutrino interactions) of the tracker part of the ND280 detector, characterised with a better reconstruction ability, needs to be enlarged in order to increase the rate of neutrino
2137:
Veto is a part of a detector where no activity should be registered to accept an event. Such requirement allows constraining the number of background events in a selected sample; here the background from particles produced outside of the
2108:
will be built. Part of the beam related upgrade works and the upgrade of the ND280 detector will be performed yet before the start of phase II of the T2K experiment. The HK experiment is expected to start operation around the year 2027.
1399:
T2K experiment started to take neutrino data for a physics analysis in
January 2010, initially with an incomplete ND280 detector, and starting from November 2010 with the full setup. The data taking was interrupted for one year by the
370:
in quark section was confirmed already in 1964, but it is too small to explain the observed matter-antimatter imbalance. The strong CP violation in the neutrino sector could lead to matter excess production through the process called
1113:
One BabyMIND (prototype Magnetized Iron Neutrino Detector) that is a magnetized muon spectrometer to detect forward-going muons. BabyMIND sports an original configuration of scintillation modules intertwined with magnetized
972:
decay can be mis-reconstructed as an electron in the Super-Kamiokande detector, thus this reaction can mimic electron neutrino interactions and constitute an important background in electron neutrino appearance measurement.
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located at one or both ends of the fibres. Scintillator bars are organised into layers, where bars in two neighbouring layers are perpendicular to each other providing together 3D information about the traversing particles.
6843:
1617:
High-angle and backwards-going tracks must be well-reconstructed. This is achieved by increasing the angular acceptance and the efficiency of the discrimination between backward from forward going tracks using timing
1678:
modules technology for track reconstruction. The main novel feature of the HATPCs, aside from their high angle coverage, is the use of the resistive MicroMegas technology. The latter consists of applying a layer of
1473:(matter-antimatter) asymmetry. Achievement of these goals requires the reduction of statistical and systematic errors. Thus a significant upgrade of the beamline and the ND280 detector, doping of SK water with
1683:
material to increase the charge-sharing capabilities of the MicroMegas modules. This reduces the number of readout channels and allows for a spatial resolution which is as good as the one in the current TPCs.
2045:) into SK water was done in July–August 2020 and lead to a 0.011% concentration of Gd. T2K collected its first data with Gd in SK in March–April 2021. Usage of gadolinium-doped water will allow studying
1434:
Phase II of the T2K experiment is expected to start at the beginning of 2023 and last until 2026, following by the commencement of the HK experiment. The physics goals of T2K-II are a measurement of the
1080:
detectors (WAGASCI, WAter-Grid-SCIntillator-Detector) that act as the main water targets and particle trackers. The 3D grid-like structure of scintillator bars creates hollow cavities filled with water.
510:
parameters, cross-section measurements which will extend our understanding of neutrino interactions and thus improve theoretical models used in neutrino generators, as well as further constrain on the
1150:
O cross-section estimate from the CH one. The fraction of water in WAGASCI water-scintillator modules is 80% enabling a measurement of the charged-current neutrino cross-section ratio between water (H
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46:
by the international cooperation of about 500 physicists and engineers with over 60 research institutions from several countries from Europe, Asia and North America and it is a recognized
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T2K Collaboration (September 2019). "Measurement of the muon neutrino charged-current cross sections on water, hydrocarbon and iron, and their ratios, with the T2K on-axis detectors".
3166:
T2K Collaboration (21 June 2016). "Measurement of double-differential muon neutrino charged-current interactions on C8H8 without pions in the final state using the T2K off-axis beam".
1583:), but it also has a number of limitations, like low reconstruction efficiency of particles produced almost perpendicular and backward with respect to the direction of the interacting
2100:(HK) experiment, will use the upgraded system of the currently used accelerator and neutrino beamline and upgraded set of the near detector. Apart from that, a new far detector, the
469:
oscillation channels. NOvA is conducted in the United States and measures accelerator neutrino oscillation at the distance of 810 km on the way between beam production place in
1650:
directions. Due to its geometry and coupled with the TOF and the HATPCs, the SuperFGD has the capability to detect fast-neutrons, which could be useful in the reconstruction of the
617:
and directed into a tunnel called the decay volume. Depending on the horns polarity, either positive or negative particles are focused. Positive pions and kaons decay mainly into
3300:
T2K Collaboration (21 February 2020). "First combined measurement of the muon neutrino and antineutrino charged-current cross section without pions in the final state at T2K".
6838:
5233:
Hyper-Kamiokande Proto-Collaboration (19 May 2015). "Physics potential of a long-baseline neutrino oscillation experiment using a J-PARC neutrino beam and Hyper-Kamiokande".
4598:
Hyper-Kamiokande Proto-Collaboration (19 May 2015). "Physics Potential of a Long Baseline Neutrino Oscillation Experiment Using J-PARC Neutrino Beam and Hyper-Kamiokande".
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The SuperFGD is a 2 by 2 by 0.5 metres (6 ft 7 in × 6 ft 7 in × 1 ft 8 in) detector consisting of approximately 2 million 1 cm
835:
and type of interactions in the far detector, reducing the systematic error in the neutrino oscillations analysis associated with models of neutrino interactions and flux.
1426:
detector. The building of an additional Intermediate Water Cherenkov detector at a distance of around 2 kilometres (1.2 mi) is also considered for the HK experiment.
1522:
be further decreased to 1.16 s and the number of protons per pulse has to increase to 3.2x10. In addition to increasing the primary proton beam power, the current in the
1674:(HATPCs) will surround the SuperFGD in the plane perpendicular to the incoming neutrino beam. Their design is similar to that of the existing TPCs, as they both use the
4574:
3367:
T2K Collaboration (26 January 2017). "First measurement of the muon neutrino charged current single pion production cross section on water with the T2K near detector".
2967:
T2K Collaboration (27 February 2020). "Measurement of the charged-current electron (Anti-)neutrino inclusive cross-sections at the T2K off-axis near detector ND280".
2039:
3509:
T2K Collaboration (31 October 2014). "Measurement of the neutrino-oxygen neutral-current interaction cross section by observing nuclear deexcitation gamma rays".
6848:
4909:"Characterization of charge spreading and gain of encapsulated resistive Micromegas detectors for the upgrade of the T2K Near Detector Time Projection Chambers"
5328:
2439:
T2K Collaboration (2015). "Measurements of neutrino oscillation in appearance and disappearance channels by the T2K experiment with 6.6E20 protons on target".
474:
6813:
83:
in neutrino oscillations. The measurement of the neutrino-antineutrino oscillation asymmetry may bring us closer to the explanation of the existence of our
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1119:
one. However, the magnetic field is not homogeneous over the travel volume of the muons, and this poses a still open challenge for momentum reconstruction.
6495:
6391:
6095:
4538:
1614:
The detector needs to efficiently detect the nucleons in the final state of neutrino interactions. For this, the detection thresholds need to be lowered.
3705:
3099:
T2K Collaboration (7 May 2013). "Measurement of the inclusive numu charged current cross section on carbon in the near detector of the T2K experiment".
6014:
6722:
6365:
5601:
3233:
T2K Collaboration (11 December 2015). "Measurement of the numu charged-current quasielastic cross section on carbon with the ND280 detector at T2K".
589:: first to 400 MeV energy by the Linac linear accelerator, then up to 3 GeV by the RCS (Rapid Cycle Synchrotron), and finally up to 30 GeV by the MR
6642:
2070:'s are the most reactive in SK but were yet indistinguishable from neutrinos from other sources. It will also improve the detector performance for
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MicroMegas modules, and X coordinate is based on the electrons drift time. In the magnetic field, the curvature of this path allows to determine
701:
are stopped by a 75-ton block of graphite (so-called beam dump) and in the ground, while neutrinos travel underground towards the far detector.
2005:, which then produce Cherenkov light. Gadolinium is a naturally occurring element with the highest cross-section on the capture of neutrons at
6462:
1733:
of the registered particle. That means it is not possible to distinguish neutrino from antineutrino interaction based on a charge of produced
6692:
6566:
6334:
2900:
T2K Collaboration (30 April 2019). "Search for light sterile neutrinos with the T2K far detector Super-Kamiokande at a baseline of 295 km".
6141:
2364:
T2K Collaboration (2014). "Precise Measurement of the Neutrino Mixing Parameter θ23 from Muon Neutrino Disappearance in an Off-Axis Beam".
1603:
in the reconstructed neutrino energy spectrum. Thus, it is essential to optimize the detector to be sensitive to additional particles and
6370:
2222:
1201:
Super-Kamiokande detector is located 1000 m underground in the Mozumi Mine, under Mount Ikeno in the Kamioka area of Hida city. It is a
6607:
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installed in the fall of 2010. T2K far detector is the large Super-Kamiokande detector, which has been running since 1996 and studying
1106:
Two WallMRD (Wall Muon Range Detector) that are non-magnetized muon spectrometers to detect side going muons. They are made of passive
1166:
of measurements from these detectors will provide an improved constraint on the neutrino cross-sections as a function of their energy.
6951:
6712:
6591:
6581:
6299:
5713:
5439:
2192:
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6803:
4682:
T2K Collaboration and J-PARC Neutrino Facility Group (14 August 2019). "J-PARC Neutrino Beamline Upgrade Technical Design Report".
3744:
517:
phase and confirmation if the CP symmetry is conserved or violated in the neutrino oscillation at the 3σ significance level in the
6470:
5211:
2286:
T2K Collaboration (2011). "Indication of Electron Neutrino Appearance from an Accelerator-produced Off-axis Muon Neutrino Beam".
2262:
50:
experiment (RE13). T2K collected data within its first phase of operation from 2010 till 2021. The second phase of data taking (
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5156:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
4913:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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power until the start of the HK experiment. The beam power should reach 750 kW in 2022 and then grow to 1.3 MW by 2029.
1278:, observed by PMTs as a ring with fuzzy edges. Neutrino energy is calculated based on the direction and energy of a charged
722:
is maximal for around 600 MeV neutrinos. In this neutrino energy range, the dominant type of neutrino interactions are
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6571:
6360:
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and were consistent with the previous measurements of oscillation parameters measured by the Super-Kamiokande detector for
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interaction studies. It provided the first neutrino beam data using a full detector setup during the 2019/2020 winter run.
94:
facility (Japan Proton Accelerator Research Complex) in Tokai on the east coast of Japan. The beam is directed towards the
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Reduction of the repetition cycle will require a series of hardware upgrades, including a major upgrade of the Main Ring
1006:
of the particle, and the amount of the ionisation electrons per unit distance is used to identify particles based on the
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6798:
3434:
T2K Collaboration (4 November 2016). "Measurement of Coherent π+ Production in Low Energy Neutrino-Carbon Scattering".
1057:
The predicted T2K neutrino flux at the site of the WAGASCI-BabyMIND (red line) and of the ND280 (black line) detectors
347:
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280:(CC) interactions, CC interactions without pions and with single pion in the final state, coherent pion production,
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Since the start of the data taking in 2010, the T2K experiment succeeded to provide a list of world-class results:
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target, the magnetic horns and the beam dump, as well as disposal of a larger amount of irradiated cooling water.
1360:
detector, located 250 km away. The K2K experiment results confirmed at the confidence level of 99.9985% (4.3
2101:
2002:
1495:/ discrimination in the far detector, as well as improvements in the software and analysis methods will be done.
775:. The light produced by traversing charged particles in the plastic scintillator bars and planes is collected by
4822:
3767:
3036:"Measurement of the electron neutrino charged-current interaction rate on water with the T2K ND280 pi0 detector"
1123:
All the active material in the detectors is made up of plastic scintillator and is read as explained in section
6752:
6647:
6344:
5753:
5370:
4534:
4041:"The new experiment WAGASCI for water to hydrocarbon neutrino cross section measurement using the J-PARC beam"
252:), which was the first time when neutrinos produced in one flavour was explicitly observed in another flavour.
6818:
3805:
NOvA Collaboration (2022). "Improved measurement of neutrino oscillation parameters by the NOvA experiment".
2833:
T2K Collaboration (16 March 2015). "Search for short baseline nue disappearance with the T2K near detector".
1462:
or more of the matter-antimatter asymmetry in the neutrino sector in a wide range of possible true values of
6793:
1571:
The current design of the ND280 detector is optimized for the detection and reconstruction of forward-going
6930:
6762:
6672:
6622:
6319:
6150:
5621:
5557:
5525:
4261:
T2K UK Collaboration (17 October 2013). "The electromagnetic calorimeter for the T2K near detector ND280".
3997:
Antonova, M.; et al. (April 2017). "Baby MIND: A magnetised spectrometer for the WAGASCI experiment".
6910:
6314:
6309:
6127:
5826:
5545:
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5122:
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T2K Collaboration (5 August 2013). "Evidence of electron neutrino appearance in a muon neutrino beam".
1038:
1224:
emitted by charged particles moving in water faster than light in this medium. Its goal is to measure
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5531:
1418:
experiment – the Hyper-Kamiokande (HK) experiment – will be launched with the new, 250,000-ton water
1045:. Finally, it can help identify beam interactions in the surrounding walls and in the magnet itself.
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4859:
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6002:
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analysis, which will be achieved thanks to its complementarity with respect to the ND280 detector:
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5469:
4467:
K2K Collaboration (12 October 2006). "Measurement of neutrino oscillation by the K2K experiment".
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4908:
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1401:
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The main goal of the WAGASCI-BabyMIND detector is a reduction of the systematic error in the T2K
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765:
273:
203:
2009:
energy. For 25 meV neutrons, the cross-section for gadolinium is about 10 times higher than for
743:
ND280 detector located 2.5° away from the beam axis, i.e. at the same angle as the far detector.
6168:
6053:
5886:
4143:
T2K ND280 TPC collaboration (May 2011). "Time projection chambers for the T2K near detectors".
727:
with meson production, which are background in the oscillation analysis in the T2K experiment.
2214:
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1061:
WAGASCI-BabyMIND is a new detector located next to the INGRID and ND280 detectors, devoted to
375:
and thus such measurement would be important step to understand how the Universe were formed.
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oscillation parameters based on studies in the near ND280 and far Super-Kamiokande detectors.
39:
35:
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The T2K experiment operated in the current form until 2020. In 2021 the first data run with
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The Super-Kamiokande Collaboration (2022). "First gadolinium loading to Super-Kamiokande".
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5028:
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4733:
4656:
Hyper-Kamiokande Proto-Collaboration (28 November 2018). "Hyper-Kamiokande Design Report".
4617:
4486:
4390:
4347:
4280:
4221:
4162:
4109:
4052:
3930:
3855:
T2K Collaboration (13 September 2016). "Proposal for an Extended Run of T2K to 20E21 POT".
3676:
3595:
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2634:
2589:
2526:
2383:
2305:
2079:
1692:
The six Time-of-Flight (TOF) detectors surrounding the HATPCs and SuperFGD are a series of
1508:
1458:
with a precision of 1.7° and 1%, respectively, as well as a confirmation at the level of 3
1436:
1393:
1365:
1341:
1321:
1213:
1131:
768:
in ND280, the entire active material (enabling particle tracking) of the near detectors is
710:
586:
578:
156:
2184:
556:
Superconducting magnets under construction in 2008 to veer the proton beam towards Kamioka
8:
6915:
6702:
6682:
6289:
6019:
5980:
5870:
5207:
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4621:
4490:
4394:
4351:
4292:
4284:
4225:
4166:
4113:
4090:
Assylbekov, S; et al. (September 2012). "The T2K ND280 off-axis pi–zero detector".
4056:
3934:
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2789:
2722:
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2593:
2530:
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layers designed to identify the particle direction sense through the measurement of the
713:
was realized. The neutrino beam at J-PARC is designed so that it can be directed 2 to 3
6828:
6617:
6556:
6276:
6195:
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5703:
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3376:
3335:
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3268:
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3175:
3134:
3108:
3047:
3002:
2976:
2935:
2909:
2868:
2842:
2801:
2775:
2734:
2708:
2650:
2624:
2550:
2516:
2505:"Constraint on the matter–antimatter symmetry-violating phase in neutrino oscillations"
2466:
2448:
2407:
2373:
2329:
2295:
1998:
1459:
1361:
1163:
1084:
Thanks to such a structure, a high water to scintillator mass ratio was obtained (80% H
985:(TPCs) are gas-tight rectangular boxes, with a cathode plane in the centre and readout
776:
6788:
6250:
4402:
2646:
2254:
1324:
parameters relevant for muon neutrino disappearance and electron neutrino appearance.
6396:
6375:
6222:
5988:
5962:
5908:
5856:
5814:
5794:
5643:
5639:
5449:
5398:
5388:
5193:
5105:
5009:(24 September 2012). "From eV to EeV: Neutrino cross sections across energy scales".
4987:
4889:
4751:
4633:
4453:
4439:
4367:
4129:
3890:
Hyper-Kamiokande Collaboration (28 November 2018). "Hyper-Kamiokande Design Report".
3836:
3639:
3469:
3339:
3272:
3006:
2939:
2654:
2615:
Mohapatra, R N; et al. (1 November 2007). "Theory of neutrinos: a white paper".
2601:
2554:
2542:
2399:
2321:
1813:). In (anti)neutrino-nucleus interactions, apart from a charged lepton production, a
1604:
1600:
1088:
O + 20% CH) and the acceptance is high and approximately constant in all directions.
847:
and instrumented with scintillator planes constituting the Side Muon Range Detector.
740:
INGRID detector (Interactive Neutrino GRID) located on the axis of the neutrino beam,
62:
54:) is expected to start in 2023 and last until commencement of the successor of T2K –
6031:
5291:
5056:
4778:
T2K Collaboration (11 January 2019). "T2K ND280 Upgrade – Technical Design Report".
4681:
4506:
4300:
3950:
3548:
3481:
3406:
3205:
3138:
2872:
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2504:
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23:
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6107:
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5802:
5743:
5723:
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5416:
5358:
5286:
5260:
5181:
5091:
5044:
5036:
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4938:
4881:
4741:
4625:
4494:
4431:
4398:
4355:
4288:
4229:
4170:
4117:
4070:
4060:
3938:
3824:
3775:
3684:
3603:
3536:
3465:
3461:
3394:
3327:
3260:
3193:
3126:
3065:
2994:
2927:
2860:
2793:
2726:
2642:
2597:
2534:
2458:
2395:
2391:
2317:
2313:
2097:
2091:
2006:
1423:
1357:
1349:
1194:
1176:
718:
363:
276:
measurements of electron and muon neutrinos and antineutrinos, including inclusive
266:
192:
95:
84:
31:
4381:
The Super-Kamiokande Collaboration (April 2003). "The Super-Kamiokande detector".
1981:
Cherenkov energy threshold (minimal total energy of a charged particle to produce
1053:
585:
facility using a proton beam gradually accelerated to 30 GeV by a system of three
6612:
6416:
6103:
6083:
6069:
6043:
6006:
5918:
5914:
5896:
5882:
5848:
5834:
5830:
5822:
5757:
5737:
5719:
5685:
5541:
5507:
5491:
5354:
2580:
Fukugita, M.; Yanagida, T. (June 1986). "Barygenesis without grand unification".
1986:
1730:
1535:
1381:
1275:
1233:
1202:
999:
889:
723:
654:, forming a muon neutrino beam, while negative pions and kaons decay mainly into
550:
351:
281:
277:
196:
103:
4435:
4328:
Aoki, S; et al. (January 2013). "The T2K Side Muon Range Detector (SMRD)".
3828:
3331:
2998:
2159:
6889:
6884:
6864:
6697:
6091:
6065:
6061:
5970:
5944:
5810:
5798:
5699:
5689:
5661:
5625:
5609:
5473:
5392:
5306:
5185:
5040:
4942:
4498:
4359:
4233:
4202:
T2K ND280 FGD Collaboration (December 2012). "The T2K fine-grained detectors".
4174:
4121:
3942:
3706:"Skewed neutrino behavior could help explain matter's dominion over antimatter"
3689:
3643:
3540:
3398:
3264:
3197:
3130:
3070:
3035:
2931:
2864:
2797:
2730:
2462:
1818:
1729:, which so far was filled with ultra-pure water. SK is not able to measure the
1700:
1389:
1385:
1373:
1337:
1333:
1115:
844:
840:
714:
5301:
5296:
2538:
1721:
The third element to be improved within T2K – phase II is the introduction of
6945:
6087:
6035:
5966:
5892:
5874:
5844:
5765:
5761:
5727:
5669:
5597:
5567:
5549:
5511:
5481:
5457:
5428:
5410:
5382:
4991:
4893:
4755:
4637:
1990:
1646:
1523:
1515:
1369:
1007:
855:
779:
614:
69:
66:
27:
993:-based drift gas under atmospheric pressure. Charged particles crossing TPC
954:
This reaction can mimic electron neutrino interactions because photons from
538:
491:
Future upgrades of T2K is expected to provide more precise measurements of Δ
214:
The confirmation of electron neutrino appearance in the muon neutrino beam (
6637:
6047:
5992:
5974:
5940:
5936:
5806:
5657:
5575:
5465:
3779:
3473:
2546:
2403:
2325:
1696:
1651:
1636:
1543:
1470:
1100:
1077:
772:
564:
382:
experiment is the other neutrino oscillation experiment capable to measure
372:
367:
355:
307:
206:
for different types of neutrinos and targets in an energy range of few GeV.
80:
5264:
4629:
3607:
114:
T2K experiment was proposed in 2003 with the following measurement goals:
5948:
5930:
5904:
5878:
5818:
5647:
5589:
5585:
5495:
5366:
5362:
1997:. High energy photons (for gadolinium their total energy is about 8 MeV)
1825:, for neutrinos it is mostly a proton and for antineutrinos – a neutron:
1639:
1042:
590:
5048:
4906:
821:
6657:
6561:
6401:
5922:
5771:
5665:
5571:
5553:
5477:
5404:
5006:
4481:
4426:
4075:
2629:
1722:
1474:
1414:
994:
809:
99:
72:. It also provided the world best measurement of oscillation parameter
6406:
1563:
98:
far detector located 295 kilometres (183 mi) away in the city of
6411:
6079:
6010:
5519:
5453:
4814:
2075:
2071:
1994:
478:
5232:
4655:
4597:
3911:
T2K Collaboration (2 January 2013). "T2K neutrino flux prediction".
1567:
Scheme of the inner part of the ND280 detector after planned upgrade
1028:
providing additional information relevant for their identification.
989:
modules at both sides parallel to the cathode. TPCs are filled with
6894:
6767:
6757:
6490:
6304:
6149:
5376:
5247:
5168:
4974:
4925:
4876:
4812:
4784:
4688:
4662:
4612:
4007:
3896:
3861:
3819:
3590:
3448:
3381:
3314:
3180:
3052:
2981:
2914:
2521:
2453:
2010:
1584:
1580:
1552:
1229:
1208:
tank of about 40 m height and diameter, filled with 50,000 tons of
1205:
1186:
1062:
1003:
598:
470:
359:
5153:
5023:
4380:
4342:
4275:
4216:
4157:
4104:
3925:
3523:
3247:
3113:
2847:
2780:
2713:
2378:
2300:
884:
The main goal of the Pi-Zero Detector is a measurement of neutral
760:
Principle of operation of a scintillator in the T2K near detectors
6732:
5302:
Inside Japan's Big Physics | Part one: Super Kamiokande – YouTube
5281:
2042:
1814:
1693:
1596:
1548:
1146:
O) forces us to rely on cross-section models to disentangle the H
1097:
769:
1103:(CH) bars, that acts as the main CH target and particle tracker.
6925:
6707:
6667:
6652:
6586:
6526:
6500:
5747:
4860:"A fully-active fine-grained detector with three readout views"
4857:
1734:
1572:
1512:
1504:
1279:
756:
698:
694:
594:
582:
285:
159:, and thus the confirmation that the last unknown mixing angle
91:
3889:
3766:
Himmel, Alex; et al. (NOvA Collaboration) (2 July 2020).
1662:
1610:
Three main measures need to be taken to address these issues:
1599:) were lost, may be mis-reconstructed as CCQE and introduce a
1503:
The beam upgrade plan requires one year long shut down of the
61:
T2K was the first experiment which observed the appearance of
6727:
6632:
6627:
6510:
6505:
6480:
6329:
6218:
2030:
1353:
1209:
1073:
990:
709:
T2K is the first experiment in which the concept of off-axis
602:
339:. T2K provided the first and the strongest yet constraint on
289:
43:
4722:"J-PARC accelerator and neutrino beamline upgrade programme"
4571:
The 20th Lomonosov Conference on Elementary Particle Physics
4416:
Oyama, Yuichi (2006). "Results from K2K and status of T2K".
6426:
6421:
5579:
5072:"Supernova Neutrino Detection in Water Cherenkov Detectors"
4564:"Physics and status of SuperFGDdetector for T2K experiment"
4201:
4142:
1642:
1592:
1588:
1576:
1531:
1527:
1225:
1217:
1190:
1107:
885:
610:
606:
379:
293:
47:
4955:
4420:. NATO Security through Science Series. pp. 113–124.
1551:
capacity of the secondary beamline components such as the
1539:
the anti-neutrino mode beam) by around 5 - 10%.
1320:
spectra are determined, leading to the measurement of the
1707:
1345:
4958:"A 4π time-of-flight detector for the ND280/T2K upgrade"
1511:
in 2021, followed by a constant gradual increase of the
1068:
The WAGASCI-BabyMIND consists of several sub-detectors:
4715:
4713:
3634:
2215:"RE13/T2K : The long-baseline neutrino experiment"
1138:
Different target material between ND280 (80% CH + 20% H
358:
the excess of matter with respect to antimatter at the
195:
oscillations, which could be observed as a deficit of
90:
The intense beam of muon neutrinos is produced in the
5208:"The Hyper-Kamiokande project is officially approved"
4813:
The T2K ND280 Upgrade Working Group (June 19, 2020).
4710:
4260:
4038:
3996:
2255:"The status of T2K and Hyper-Kamiokande experiments"
1666:
TPC for the ND280 Upgrade of T2K experiment in Japan
1336:) experiment, which ran from 1999 till 2004. In the
1110:
planes intertwined with active scintillator planes.
1037:stopped in the calorimeter. SMRD can also act as a
169:
Precise measurement of the oscillation parameters Δ
4806:
4773:
4771:
4769:
4767:
4765:
3850:
3848:
3846:
3804:
3768:"New Oscillation Results from the NOvA Experiment"
3737:"Biggest cosmic mystery 'step closer' to solution"
2160:"T2K experiment official page – T2K collaboration"
2078:and study better matter-antimatter differences in
693:, forming a muon antineutrino beam. All remaining
4777:
4677:
4675:
4673:
4466:
3910:
3854:
3575:
3508:
3433:
3366:
3299:
3232:
3165:
3098:
3033:
2966:
2899:
2832:
2765:
2698:
2438:
2363:
2285:
6943:
5336:
5235:Progress of Theoretical and Experimental Physics
4600:Progress of Theoretical and Experimental Physics
4557:
4555:
4089:
4039:Ovsiannikova, T; et al. (5 February 2016).
4001:(NUPHYS2016-HALLSJO, FERMILAB-CONF-17-270-APC).
3578:Progress of Theoretical and Experimental Physics
2699:T2K Collaboration (2011). "The T2K Experiment".
2614:
2579:
522:
284:interactions, etc. on different targets such as
55:
6151:Neutrino detectors, experiments, and facilities
5297:Neutrino physics – The T2K experiment – YouTube
5004:
4762:
3843:
3628:
2502:
1282:produced in the CCQE interaction. In this way,
4670:
2085:
1022:
577:T2K uses a muon neutrino or muon antineutrino
481:. NOvA provided a less precise measurement of
6135:
5322:
4552:
5200:
5117:
5115:
4843:: CS1 maint: numeric names: authors list (
4798:: CS1 maint: numeric names: authors list (
4702:: CS1 maint: numeric names: authors list (
4535:"T2K experiment official page – T2K Run 10"
4519:: CS1 maint: numeric names: authors list (
4313:: CS1 maint: numeric names: authors list (
4246:: CS1 maint: numeric names: authors list (
4187:: CS1 maint: numeric names: authors list (
3992:
3990:
3988:
3986:
3984:
3982:
3980:
3978:
3976:
3974:
3963:: CS1 maint: numeric names: authors list (
3875:: CS1 maint: numeric names: authors list (
3620:: CS1 maint: numeric names: authors list (
3561:: CS1 maint: numeric names: authors list (
3494:: CS1 maint: numeric names: authors list (
3419:: CS1 maint: numeric names: authors list (
3352:: CS1 maint: numeric names: authors list (
3285:: CS1 maint: numeric names: authors list (
3218:: CS1 maint: numeric names: authors list (
3151:: CS1 maint: numeric names: authors list (
3084:: CS1 maint: numeric names: authors list (
3019:: CS1 maint: numeric names: authors list (
2952:: CS1 maint: numeric names: authors list (
2885:: CS1 maint: numeric names: authors list (
2818:: CS1 maint: numeric names: authors list (
2751:: CS1 maint: numeric names: authors list (
2483:: CS1 maint: numeric names: authors list (
2424:: CS1 maint: numeric names: authors list (
2359:
2357:
2346:: CS1 maint: numeric names: authors list (
2281:
2279:
2248:
2246:
2244:
2242:
2240:
1031:
976:
613:, which are then focused by a set of three
6911:BNO (Baksan or Baxan Neutrino Observatory)
6142:
6128:
5329:
5315:
4034:
4032:
4030:
4028:
4026:
4024:
4022:
4020:
4018:
3883:
2694:
2692:
2690:
2688:
2686:
2684:
2498:
2496:
2494:
2253:Vilela, Cristovao (September 5–10, 2021).
1332:T2K is a successor of the KEK to Kamioka (
16:Long-baseline neutrino experiment in Japan
5714:The Event Horizon Telescope Collaboration
5246:
5167:
5095:
5069:
5022:
4973:
4924:
4875:
4783:
4745:
4687:
4661:
4651:
4649:
4647:
4611:
4480:
4425:
4341:
4274:
4215:
4156:
4103:
4074:
4064:
4006:
3924:
3895:
3860:
3818:
3688:
3589:
3522:
3447:
3380:
3313:
3246:
3179:
3112:
3069:
3051:
2980:
2913:
2846:
2779:
2759:
2712:
2682:
2680:
2678:
2676:
2674:
2672:
2670:
2668:
2666:
2664:
2628:
2520:
2452:
2377:
2299:
2096:The successor of the T2K experiment, the
1013:
5112:
4327:
3971:
2354:
2276:
2237:
1661:
1562:
1180:
1052:
854:
755:
299:The first significant constraint on the
188:via muon neutrino disappearance studies.
5149:
5147:
4825:from the original on September 29, 2021
4561:
4015:
3904:
2491:
1989:by another nucleus, which goes into an
1645:. The cubes are woven with a series of
6944:
5214:from the original on 27 September 2020
4719:
4644:
3765:
3734:
2661:
2503:Abe, K.; et al. (15 April 2020).
2252:
1708:Impact on Neutrino Oscillation Physics
1092:One Proton Module, the same as in the
544:Bird's-eye view of the entire facility
6123:
5310:
5076:Journal of Physics: Conference Series
4726:Journal of Physics: Conference Series
4415:
4045:Journal of Physics: Conference Series
1726:
1154:O) and plastic (CH) with 3% accuracy.
5144:
4562:Kudenko, Yury (August 19–25, 2021).
4418:Nuclear Science and Safety in Europe
1469:– the parameter responsible for the
1236:quasielastic interactions (CCQE) of
1212:and instrumented with around 13,000
1093:
255:The most precise measurement of the
202:Measurements of various interaction
5123:"Super-Kamiokande Official Website"
4821:. CERN-SPSC-2020-008. SPSC-SR-267.
3703:
1170:
1124:
1048:
850:
843:producing 0.2 T uniform horizontal
827:Exploded view of the ND280 detector
13:
5070:Scholberg, Kate (10 August 2011).
4956:Korzenev, A.; et al. (2022).
3747:from the original on 18 April 2020
3716:from the original on 20 April 2020
3644:"Evidence for the 2π decay of the
3034:T2K Collaboration (19 June 2015).
2561:from the original on 16 April 2020
2225:from the original on 30 April 2020
2195:from the original on 22 April 2019
2016:The first loading of 13 tons of Gd
1344:of muon neutrinos was produced at
790:
350:proposed by the Russian physicist
109:
14:
6978:
6875:Long Baseline Neutrino Experiment
5292:Super-Kamiokande Realtime Monitor
5287:Super-Kamiokande Official Website
5275:
4907:Ambrosi, L.; et al. (2023).
4858:Blondel, A.; et al. (2018).
3786:from the original on 5 March 2021
1993:and during deexcitation produced
799:
751:
730:
42:. The experiment is conducted in
6952:Accelerator neutrino experiments
2185:"Recognized Experiments at CERN"
1558:
892:neutrino interactions on water:
820:
808:
704:
563:
549:
537:
528:
6957:Science and technology in Japan
5282:T2K Experiment Official Website
5226:
5133:from the original on 2021-10-07
5063:
4998:
4949:
4900:
4851:
4819:CERN Scientific Committee Paper
4591:
4580:from the original on 2021-09-29
4541:from the original on 2020-05-03
4527:
4460:
4409:
4374:
4321:
4254:
4195:
4136:
4083:
3798:
3759:
3728:
3697:
3569:
3502:
3427:
3360:
3293:
3226:
3159:
3092:
3027:
2960:
2893:
2826:
2608:
2265:from the original on 2021-09-29
2219:The CERN Experimental Programme
2189:The CERN Experimental Programme
2166:from the original on 2020-04-17
2131:
2003:produce electron-positron pairs
1498:
1408:
570:Neutrino beam production scheme
389:through the comparison between
306:parameter, responsible for the
56:the Hyper-Kamiokande experiment
5097:10.1088/1742-6596/309/1/012028
4984:10.1088/1748-0221/17/01/P01016
4886:10.1088/1748-0221/13/02/P02006
4747:10.1088/1742-6596/888/1/012042
4066:10.1088/1742-6596/675/1/012030
3735:Rincon, Paul (16 April 2020).
3466:10.1103/PhysRevLett.117.192501
2969:Journal of High Energy Physics
2617:Reports on Progress in Physics
2573:
2432:
2396:10.1103/PhysRevLett.112.181801
2318:10.1103/PhysRevLett.107.041801
2207:
2177:
2152:
1526:focusing secondary particles (
1:
6192:Lederman–Schwartz–Steinberger
4815:"NP07: ND280 Upgrade project"
4403:10.1016/S0168-9002(03)00425-X
4293:10.1088/1748-0221/8/10/P10019
3999:Prospects in Neutrino Physics
3704:Cho, Adrian (15 April 2020).
2145:
1817:is usually realised from the
310:in the neutrino oscillations.
6931:List of neutrino experiments
5622:Sudbury Neutrino Observatory
4720:Friend, M (September 2017).
2602:10.1016/0370-2693(86)91126-3
79:and a hint of a significant
7:
5546:Supernova Cosmology Project
4436:10.1007/978-1-4020-4965-1_9
3829:10.1103/PhysRevD.106.032004
3332:10.1103/PhysRevD.101.112001
2647:10.1088/0034-4885/70/11/R02
2112:
2086:Hyper-Kamiokande experiment
1630:
1023:Electromagnetic Calorimeter
784:Multi-pixel photon counters
518:
308:matter-antimatter asymmetry
81:matter-antimatter asymmetry
51:
10:
6983:
5186:10.1016/j.nima.2021.166248
5041:10.1103/RevModPhys.84.1307
4962:Journal of Instrumentation
4943:10.1016/j.nima.2023.168534
4864:Journal of Instrumentation
4499:10.1103/PhysRevD.74.072003
4360:10.1016/j.nima.2012.10.001
4263:Journal of Instrumentation
4234:10.1016/j.nima.2012.08.020
4175:10.1016/j.nima.2011.02.036
4122:10.1016/j.nima.2012.05.028
3943:10.1103/physrevd.87.012001
3690:10.1103/PhysRevLett.13.138
3541:10.1103/PhysRevD.90.072012
3399:10.1103/PhysRevD.95.012010
3265:10.1103/PhysRevD.92.112003
3198:10.1103/PhysRevD.93.112012
3131:10.1103/PhysRevD.87.092003
3071:10.1103/PhysRevD.91.112010
2932:10.1103/PhysRevD.99.071103
2865:10.1103/PhysRevD.91.051102
2798:10.1103/PhysRevD.88.032002
2731:10.1016/j.nima.2011.06.067
2463:10.1103/PhysRevD.91.072010
2104:, and possibly also a new
2089:
2047:remote supernova neutrinos
1327:
1174:
782:and detected by Hamamatsu
6903:
6857:
6781:
6600:
6544:
6519:
6461:
6440:
6384:
6353:
6275:
6260:
6157:
5785:
5438:
5345:
5127:www-sk.icrr.u-tokyo.ac.jp
5011:Reviews of Modern Physics
2539:10.1038/s41586-020-2177-0
2102:Hyper-Kamiokande detector
1429:
6967:Fixed-target experiments
2124:
1716:
1672:Time Projection Chambers
1657:
1096:detector, made of plain
1032:Side Muon Range Detector
983:Time Projection Chambers
977:Time projection chambers
859:Pi-Zero detector scheme.
815:ND280 under construction
766:Time Projection Chambers
34:experiment studying the
6040:Shankar Balasubramanian
5776:Alexander Zamolodchikov
5708:Peter van Nieuwenhuizen
3668:Physical Review Letters
3436:Physical Review Letters
2999:10.1007/JHEP10(2020)114
2288:Physical Review Letters
2040:gadolinium(III) sulfate
1402:Great Tohoku Earthquake
1356:) and sent towards the
6054:Clifford P. Brangwynne
5887:Emmanuelle Charpentier
3780:10.5281/zenodo.3959581
3642:; et al. (1964).
1687:
1667:
1568:
1534:, etc.) with a chosen
1198:
1058:
1014:Fine-grained detectors
860:
761:
362:, which forms now our
199:neutrino interactions.
5558:High-Z Supernova Team
4870:(02): P02006–P02006.
2259:PANIC 2021 Conference
2106:intermediate detector
1665:
1566:
1374:atmospheric neutrinos
1214:photomultiplier tubes
1184:
1056:
858:
759:
364:matter-built Universe
118:The discovery of the
40:accelerator neutrinos
6246:Neutrino oscillation
5997:Virginia Man-Yee Lee
5861:Alexander Varshavsky
5680:Jocelyn Bell Burnell
5578:and contributors to
5210:. 12 February 2020.
2080:accelerator neutrino
2001:from an atom and/or
1384:and oscillations of
1216:(PMT). It detects a
473:and far detector in
6916:Kamioka Observatory
5981:Jeffrey M. Friedman
5871:Charles David Allis
5556:and members of the
5544:and members of the
5265:10.1093/ptep/ptv061
5257:2015PTEP.2015e3C02A
5178:2022NIMPA102766248A
5088:2011JPhCS.309a2028S
5033:2012RvMP...84.1307F
4935:2023NIMPA105668534A
4738:2017JPhCS.888a2042F
4630:10.1093/ptep/ptv061
4622:2015PTEP.2015e3C02A
4491:2006PhRvD..74g2003A
4395:2003NIMPA.501..418F
4352:2013NIMPA.698..135A
4285:2013JInst...8P0019A
4226:2012NIMPA.696....1A
4167:2011NIMPA.637...25A
4114:2012NIMPA.686...48A
4057:2016JPhCS.675a2030O
3935:2013PhRvD..87a2001A
3681:1964PhRvL..13..138C
3608:10.1093/ptep/ptz070
3600:2019PTEP.2019i3C02A
3533:2014PhRvD..90g2012A
3458:2016PhRvL.117s2501A
3391:2017PhRvD..95a2010A
3324:2020PhRvD.101k2001A
3257:2015PhRvD..92k2003A
3190:2016PhRvD..93k2012A
3123:2013PhRvD..87i2003A
3062:2015PhRvD..91k2010A
2991:2020JHEP...10..114T
2924:2019PhRvD..99g1103A
2857:2015PhRvD..91e1102A
2790:2013PhRvD..88c2002A
2723:2011NIMPA.659..106A
2639:2007RPPh...70.1757M
2594:1986PhLB..174...45F
2531:2020Natur.580..339T
2388:2014PhRvL.112r1801A
2310:2011PhRvL.107d1801A
2119:Kamioka Observatory
1823:charge conservation
1422:far detector – the
1008:Bethe-Bloch formula
777:wavelength-shifting
320:takes values from -
6074:Masashi Yanagisawa
5985:Franz-Ulrich Hartl
5915:Stephen J. Elledge
5867:Alim Louis Benabid
5754:Charles H. Bennett
5704:Daniel Z. Freedman
5654:Charles L. Bennett
5618:Arthur B. McDonald
5606:Kōichirō Nishikawa
5536:John Henry Schwarz
5526:Alexander Polyakov
5504:Michel Della Negra
5423:Daniel A. Spielman
5338:Breakthrough Prize
5005:Formaggio, J. A.;
4573:. pp. 17–18.
1668:
1569:
1199:
1059:
861:
762:
601:target, producing
63:electron neutrinos
6939:
6938:
6673:Heidelberg-Moscow
6540:
6539:
6397:ICARUS (Fermilab)
6117:
6116:
6096:Fredrick Van Goor
5989:Arthur L. Horwich
5963:Adrian R. Krainer
5857:Richard P. Lifton
5815:Napoleone Ferrara
5795:Cornelia Bargmann
5644:Andrew Strominger
5640:Joseph Polchinski
5450:Nima Arkani-Hamed
5399:Vincent Lafforgue
5389:Christopher Hacon
4469:Physical Review D
4445:978-1-4020-4963-7
3913:Physical Review D
3807:Physical Review D
3511:Physical Review D
3369:Physical Review D
3302:Physical Review D
3235:Physical Review D
3168:Physical Review D
3101:Physical Review D
3040:Physical Review D
2902:Physical Review D
2835:Physical Review D
2768:Physical Review D
2623:(11): 1757–1867.
2582:Physics Letters B
2515:(7803): 339–344.
1999:scatter electrons
1142:O) and SK (pure H
6974:
6962:CERN experiments
6824:Neutrino Factory
6577:Hyper-Kamiokande
6340:Super-Kamiokande
6273:
6272:
6240:
6239:
6238:
6230:
6229:
6213:
6212:
6211:
6203:
6202:
6186:
6185:
6184:
6176:
6175:
6144:
6137:
6130:
6121:
6120:
6108:Andrew Singleton
6058:Anthony A. Hyman
6028:Jeffery W. Kelly
6023:
6015:Richard J. Youle
5959:C. Frank Bennett
5953:Don W. Cleveland
5927:Yoshinori Ohsumi
5853:Robert S. Langer
5841:James P. Allison
5803:Lewis C. Cantley
5744:Hidetoshi Katori
5724:Jens H. Gundlach
5634:Super-Kamiokande
5516:Joseph Incandela
5500:Fabiola Gianotti
5462:Maxim Kontsevich
5417:Takuro Mochizuki
5359:Maxim Kontsevich
5331:
5324:
5317:
5308:
5307:
5269:
5268:
5250:
5230:
5224:
5223:
5221:
5219:
5204:
5198:
5197:
5171:
5151:
5142:
5141:
5139:
5138:
5119:
5110:
5109:
5099:
5067:
5061:
5060:
5026:
5017:(3): 1307–1341.
5002:
4996:
4995:
4977:
4953:
4947:
4946:
4928:
4904:
4898:
4897:
4879:
4855:
4849:
4848:
4842:
4834:
4832:
4830:
4810:
4804:
4803:
4797:
4789:
4787:
4775:
4760:
4759:
4749:
4717:
4708:
4707:
4701:
4693:
4691:
4679:
4668:
4667:
4665:
4653:
4642:
4641:
4615:
4595:
4589:
4588:
4586:
4585:
4579:
4568:
4559:
4550:
4549:
4547:
4546:
4531:
4525:
4524:
4518:
4510:
4484:
4464:
4458:
4457:
4429:
4413:
4407:
4406:
4389:(2–3): 418–462.
4378:
4372:
4371:
4345:
4325:
4319:
4318:
4312:
4304:
4278:
4258:
4252:
4251:
4245:
4237:
4219:
4199:
4193:
4192:
4186:
4178:
4160:
4140:
4134:
4133:
4107:
4087:
4081:
4080:
4078:
4068:
4036:
4013:
4012:
4010:
3994:
3969:
3968:
3962:
3954:
3928:
3908:
3902:
3901:
3899:
3887:
3881:
3880:
3874:
3866:
3864:
3852:
3841:
3840:
3822:
3802:
3796:
3795:
3793:
3791:
3763:
3757:
3756:
3754:
3752:
3741:BBC News website
3732:
3726:
3725:
3723:
3721:
3701:
3695:
3694:
3692:
3662:
3661:
3660:
3652:
3651:
3632:
3626:
3625:
3619:
3611:
3593:
3573:
3567:
3566:
3560:
3552:
3526:
3506:
3500:
3499:
3493:
3485:
3451:
3431:
3425:
3424:
3418:
3410:
3384:
3364:
3358:
3357:
3351:
3343:
3317:
3297:
3291:
3290:
3284:
3276:
3250:
3230:
3224:
3223:
3217:
3209:
3183:
3163:
3157:
3156:
3150:
3142:
3116:
3096:
3090:
3089:
3083:
3075:
3073:
3055:
3031:
3025:
3024:
3018:
3010:
2984:
2964:
2958:
2957:
2951:
2943:
2917:
2897:
2891:
2890:
2884:
2876:
2850:
2830:
2824:
2823:
2817:
2809:
2783:
2763:
2757:
2756:
2750:
2742:
2716:
2696:
2659:
2658:
2632:
2612:
2606:
2605:
2577:
2571:
2570:
2568:
2566:
2524:
2500:
2489:
2488:
2482:
2474:
2456:
2436:
2430:
2429:
2423:
2415:
2381:
2361:
2352:
2351:
2345:
2337:
2303:
2283:
2274:
2273:
2271:
2270:
2250:
2235:
2234:
2232:
2230:
2211:
2205:
2204:
2202:
2200:
2181:
2175:
2174:
2172:
2171:
2156:
2139:
2135:
2098:Hyper-Kamiokande
2092:Hyper-Kamiokande
2069:
2068:
2067:
2060:
2057:
2056:
2037:
1976:
1975:
1974:
1967:
1966:
1958:
1957:
1956:
1949:
1948:
1940:
1939:
1938:
1931:
1930:
1922:
1921:
1920:
1913:
1910:
1909:
1900:
1899:
1898:
1891:
1890:
1882:
1881:
1880:
1873:
1872:
1864:
1863:
1862:
1855:
1854:
1846:
1845:
1844:
1836:
1835:
1812:
1811:
1810:
1803:
1800:
1799:
1791:
1790:
1789:
1782:
1781:
1773:
1772:
1771:
1763:
1762:
1754:
1753:
1752:
1745:
1744:
1727:Super-Kamiokande
1494:
1493:
1492:
1485:
1484:
1457:
1456:
1424:Hyper-Kamiokande
1358:Super-Kamiokande
1342:accelerator beam
1319:
1318:
1317:
1309:
1308:
1300:
1299:
1298:
1290:
1289:
1273:
1272:
1271:
1263:
1262:
1254:
1253:
1252:
1244:
1243:
1195:Super-Kamiokande
1177:Super-Kamiokande
1171:Super-Kamiokande
1049:WAGASCI-BabyMIND
971:
970:
969:
962:
961:
950:
949:
948:
941:
940:
932:
931:
930:
922:
921:
913:
912:
911:
903:
902:
880:
879:
878:
871:
870:
851:Pi-Zero detector
824:
812:
719:Super-Kamiokande
692:
691:
690:
683:
680:
679:
671:
670:
669:
662:
661:
653:
652:
651:
643:
642:
634:
633:
632:
625:
624:
581:produced at the
567:
553:
541:
523:Hyper-Kamiokande
502:
501:
468:
467:
466:
459:
456:
455:
447:
446:
445:
438:
435:
434:
426:
425:
424:
416:
415:
407:
406:
405:
397:
396:
267:sterile neutrino
251:
250:
249:
241:
240:
232:
231:
230:
222:
221:
193:sterile neutrino
180:
179:
155:
154:
153:
145:
144:
136:
135:
134:
126:
125:
96:Super-Kamiokande
85:matter-dominated
32:particle physics
6982:
6981:
6977:
6976:
6975:
6973:
6972:
6971:
6942:
6941:
6940:
6935:
6899:
6853:
6777:
6596:
6536:
6515:
6457:
6436:
6380:
6349:
6268:
6266:
6264:
6262:
6256:
6237:
6234:
6233:
6232:
6228:
6226:
6225:
6224:
6223:
6210:
6207:
6206:
6205:
6201:
6199:
6198:
6197:
6196:
6183:
6180:
6179:
6178:
6174:
6172:
6171:
6170:
6169:
6153:
6148:
6118:
6113:
6104:Ellen Sidransky
6084:Michel Sadelain
6070:Emmanuel Mignot
6044:David Klenerman
6017:
6007:Catherine Dulac
5919:Harry F. Noller
5897:Karl Deisseroth
5883:Jennifer Doudna
5849:Michael N. Hall
5835:Bert Vogelstein
5831:Shinya Yamanaka
5827:Robert Weinberg
5823:Charles Sawyers
5781:
5758:Gilles Brassard
5738:Steven Weinberg
5720:Eric Adelberger
5630:Yōichirō Suzuki
5542:Saul Perlmutter
5508:Tejinder Virdee
5492:Stephen Hawking
5441:
5434:
5355:Simon Donaldson
5341:
5335:
5278:
5273:
5272:
5231:
5227:
5217:
5215:
5206:
5205:
5201:
5152:
5145:
5136:
5134:
5121:
5120:
5113:
5068:
5064:
5003:
4999:
4954:
4950:
4905:
4901:
4856:
4852:
4836:
4835:
4828:
4826:
4811:
4807:
4791:
4790:
4776:
4763:
4718:
4711:
4695:
4694:
4680:
4671:
4654:
4645:
4596:
4592:
4583:
4581:
4577:
4566:
4560:
4553:
4544:
4542:
4533:
4532:
4528:
4512:
4511:
4465:
4461:
4446:
4414:
4410:
4379:
4375:
4326:
4322:
4306:
4305:
4259:
4255:
4239:
4238:
4200:
4196:
4180:
4179:
4141:
4137:
4088:
4084:
4037:
4016:
3995:
3972:
3956:
3955:
3909:
3905:
3888:
3884:
3868:
3867:
3853:
3844:
3803:
3799:
3789:
3787:
3764:
3760:
3750:
3748:
3733:
3729:
3719:
3717:
3702:
3698:
3659:
3656:
3655:
3654:
3650:
3648:
3647:
3646:
3645:
3633:
3629:
3613:
3612:
3574:
3570:
3554:
3553:
3507:
3503:
3487:
3486:
3432:
3428:
3412:
3411:
3365:
3361:
3345:
3344:
3298:
3294:
3278:
3277:
3231:
3227:
3211:
3210:
3164:
3160:
3144:
3143:
3097:
3093:
3077:
3076:
3032:
3028:
3012:
3011:
2965:
2961:
2945:
2944:
2898:
2894:
2878:
2877:
2831:
2827:
2811:
2810:
2764:
2760:
2744:
2743:
2697:
2662:
2613:
2609:
2578:
2574:
2564:
2562:
2501:
2492:
2476:
2475:
2437:
2433:
2417:
2416:
2366:Phys. Rev. Lett
2362:
2355:
2339:
2338:
2284:
2277:
2268:
2266:
2251:
2238:
2228:
2226:
2213:
2212:
2208:
2198:
2196:
2183:
2182:
2178:
2169:
2167:
2158:
2157:
2153:
2148:
2143:
2142:
2136:
2132:
2127:
2115:
2094:
2088:
2066:
2063:
2062:
2061:
2058:
2055:
2053:
2052:
2051:
2050:
2034:
2029:
2027:
2023:
2019:
1983:Cherenkov light
1973:
1971:
1970:
1969:
1965:
1963:
1962:
1961:
1960:
1955:
1953:
1952:
1951:
1947:
1945:
1944:
1943:
1942:
1937:
1935:
1934:
1933:
1929:
1927:
1926:
1925:
1924:
1919:
1916:
1915:
1914:
1911:
1908:
1906:
1905:
1904:
1903:
1897:
1895:
1894:
1893:
1889:
1887:
1886:
1885:
1884:
1879:
1877:
1876:
1875:
1871:
1869:
1868:
1867:
1866:
1861:
1859:
1858:
1857:
1853:
1851:
1850:
1849:
1848:
1843:
1840:
1839:
1838:
1834:
1832:
1831:
1830:
1829:
1809:
1806:
1805:
1804:
1801:
1798:
1796:
1795:
1794:
1793:
1788:
1786:
1785:
1784:
1780:
1778:
1777:
1776:
1775:
1770:
1767:
1766:
1765:
1761:
1759:
1758:
1757:
1756:
1755:is produced by
1751:
1749:
1748:
1747:
1743:
1741:
1740:
1739:
1738:
1719:
1710:
1690:
1670:The High Angle
1660:
1633:
1605:nuclear effects
1561:
1536:electric charge
1501:
1491:
1489:
1488:
1487:
1483:
1481:
1480:
1479:
1478:
1468:
1455:
1452:
1451:
1450:
1445:
1432:
1411:
1382:proton lifetime
1330:
1316:
1313:
1312:
1311:
1307:
1305:
1304:
1303:
1302:
1297:
1294:
1293:
1292:
1288:
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1285:
1284:
1283:
1270:
1267:
1266:
1265:
1261:
1259:
1258:
1257:
1256:
1251:
1248:
1247:
1246:
1242:
1240:
1239:
1238:
1237:
1234:charged current
1222:Cherenkov light
1203:stainless steel
1179:
1173:
1153:
1149:
1145:
1141:
1087:
1051:
1034:
1025:
1016:
979:
968:
966:
965:
964:
960:
958:
957:
956:
955:
947:
945:
944:
943:
939:
937:
936:
935:
934:
929:
926:
925:
924:
920:
918:
917:
916:
915:
910:
907:
906:
905:
901:
899:
898:
897:
896:
890:neutral current
877:
875:
874:
873:
869:
867:
866:
865:
864:
853:
832:
831:
830:
829:
828:
825:
817:
816:
813:
802:
793:
791:INGRID detector
764:Except for the
754:
733:
724:charged current
707:
689:
686:
685:
684:
681:
678:
676:
675:
674:
673:
668:
666:
665:
664:
660:
658:
657:
656:
655:
650:
647:
646:
645:
641:
639:
638:
637:
636:
631:
629:
628:
627:
623:
621:
620:
619:
618:
597:collide with a
575:
574:
573:
572:
571:
568:
559:
558:
557:
554:
546:
545:
542:
531:
516:
509:
500:
497:
496:
495:
487:
465:
462:
461:
460:
457:
454:
452:
451:
450:
449:
444:
441:
440:
439:
436:
433:
431:
430:
429:
428:
423:
420:
419:
418:
414:
412:
411:
410:
409:
404:
401:
400:
399:
395:
393:
392:
391:
390:
388:
354:, necessary to
352:Andrei Sakharov
345:
335:equal to 0 or ±
334:
319:
305:
282:neutral current
278:charged current
261:
248:
245:
244:
243:
239:
237:
236:
235:
234:
229:
226:
225:
224:
220:
218:
217:
216:
215:
197:neutral current
187:
178:
175:
174:
173:
165:
152:
149:
148:
147:
143:
141:
140:
139:
138:
133:
130:
129:
128:
124:
122:
121:
120:
119:
112:
110:Physics program
104:Gifu prefecture
78:
17:
12:
11:
5:
6980:
6970:
6969:
6964:
6959:
6954:
6937:
6936:
6934:
6933:
6928:
6923:
6918:
6913:
6907:
6905:
6901:
6900:
6898:
6897:
6892:
6887:
6885:NESTOR Project
6882:
6877:
6872:
6867:
6865:DUMAND Project
6861:
6859:
6855:
6854:
6852:
6851:
6846:
6841:
6836:
6831:
6826:
6821:
6816:
6811:
6806:
6801:
6796:
6791:
6785:
6783:
6779:
6778:
6776:
6775:
6770:
6765:
6760:
6755:
6750:
6745:
6740:
6735:
6730:
6725:
6720:
6715:
6710:
6705:
6700:
6695:
6690:
6685:
6680:
6675:
6670:
6665:
6660:
6655:
6650:
6645:
6640:
6635:
6630:
6625:
6620:
6615:
6610:
6604:
6602:
6598:
6597:
6595:
6594:
6589:
6584:
6579:
6574:
6569:
6564:
6559:
6554:
6548:
6546:
6542:
6541:
6538:
6537:
6535:
6534:
6529:
6523:
6521:
6517:
6516:
6514:
6513:
6508:
6503:
6498:
6493:
6488:
6483:
6478:
6473:
6467:
6465:
6459:
6458:
6456:
6455:
6450:
6444:
6442:
6438:
6437:
6435:
6434:
6429:
6424:
6419:
6414:
6409:
6404:
6399:
6394:
6388:
6386:
6382:
6381:
6379:
6378:
6373:
6368:
6363:
6357:
6355:
6351:
6350:
6348:
6347:
6342:
6337:
6332:
6327:
6322:
6317:
6312:
6307:
6302:
6297:
6292:
6287:
6281:
6279:
6270:
6258:
6257:
6255:
6254:
6253:neutrino burst
6248:
6243:
6235:
6227:
6216:
6208:
6200:
6189:
6181:
6173:
6161:
6159:
6155:
6154:
6147:
6146:
6139:
6132:
6124:
6115:
6114:
6112:
6111:
6092:Paul Negulescu
6077:
6062:Demis Hassabis
6051:
6032:Katalin Karikó
6025:
6000:
5978:
5971:Xiaowei Zhuang
5956:
5945:Kazutoshi Mori
5934:
5912:
5890:
5864:
5838:
5811:Titia de Lange
5799:David Botstein
5791:
5789:
5783:
5782:
5780:
5779:
5769:
5751:
5741:
5731:
5717:
5711:
5700:Sergio Ferrara
5693:
5683:
5673:
5666:Lyman Page Jr.
5662:Norman Jarosik
5651:
5637:
5626:Takaaki Kajita
5583:
5582:project (2016)
5561:
5539:
5529:
5523:
5485:
5474:Nathan Seiberg
5470:Juan Maldacena
5446:
5444:
5436:
5435:
5433:
5432:
5426:
5420:
5414:
5408:
5402:
5396:
5393:James McKernan
5386:
5380:
5374:
5371:Richard Taylor
5351:
5349:
5343:
5342:
5334:
5333:
5326:
5319:
5311:
5305:
5304:
5299:
5294:
5289:
5284:
5277:
5276:External links
5274:
5271:
5270:
5241:(5): 53C02–0.
5225:
5199:
5143:
5111:
5062:
4997:
4968:(01): P01016.
4948:
4899:
4850:
4805:
4761:
4709:
4669:
4643:
4606:(5): 53C02–0.
4590:
4551:
4526:
4482:hep-ex/0606032
4459:
4444:
4427:hep-ex/0512041
4408:
4373:
4320:
4269:(10): P10019.
4253:
4194:
4135:
4082:
4014:
3970:
3903:
3882:
3842:
3797:
3758:
3727:
3710:Science | AAAS
3696:
3675:(4): 138–140.
3657:
3649:
3627:
3568:
3501:
3442:(19): 192501.
3426:
3359:
3308:(11): 112001.
3292:
3241:(11): 112003.
3225:
3174:(11): 112012.
3158:
3091:
3046:(11): 112010.
3026:
2959:
2892:
2825:
2758:
2707:(1): 106–135.
2660:
2630:hep-ph/0510213
2607:
2572:
2490:
2431:
2372:(18): 181801.
2353:
2275:
2236:
2206:
2176:
2150:
2149:
2147:
2144:
2141:
2140:
2129:
2128:
2126:
2123:
2122:
2121:
2114:
2111:
2090:Main article:
2087:
2084:
2082:oscillations.
2074:explosions in
2064:
2054:
2032:
2025:
2021:
2017:
1979:
1978:
1972:
1964:
1954:
1946:
1936:
1928:
1917:
1907:
1901:
1896:
1888:
1878:
1870:
1860:
1852:
1841:
1833:
1807:
1797:
1787:
1779:
1768:
1760:
1750:
1742:
1718:
1715:
1709:
1706:
1701:time of flight
1689:
1686:
1659:
1656:
1647:optical fibres
1632:
1629:
1624:
1623:
1619:
1615:
1560:
1557:
1544:power supplies
1500:
1497:
1490:
1482:
1466:
1453:
1443:
1431:
1428:
1410:
1407:
1370:muon neutrinos
1338:K2K experiment
1329:
1326:
1314:
1306:
1295:
1287:
1268:
1260:
1249:
1241:
1175:Main article:
1172:
1169:
1168:
1167:
1159:
1155:
1151:
1147:
1143:
1139:
1125:Signal readout
1121:
1120:
1111:
1104:
1085:
1082:
1081:
1050:
1047:
1033:
1030:
1024:
1021:
1015:
1012:
978:
975:
967:
959:
952:
951:
946:
938:
927:
919:
908:
900:
888:production in
876:
868:
852:
849:
845:magnetic field
841:UA1 experiment
826:
819:
818:
814:
807:
806:
805:
804:
803:
801:
800:ND280 detector
798:
792:
789:
753:
752:Signal readout
750:
749:
748:
744:
741:
732:
731:Near detectors
729:
717:away from the
706:
703:
687:
677:
667:
659:
648:
640:
630:
622:
615:magnetic horns
569:
562:
561:
560:
555:
548:
547:
543:
536:
535:
534:
533:
532:
530:
527:
521:and 5σ in the
514:
507:
498:
485:
463:
453:
442:
432:
421:
413:
402:
394:
386:
360:early universe
343:
332:
317:
312:
311:
303:
297:
270:
263:
259:
253:
246:
238:
227:
219:
208:
207:
204:cross-sections
200:
189:
185:
176:
167:
163:
150:
142:
131:
123:
111:
108:
76:
15:
9:
6:
4:
3:
2:
6979:
6968:
6965:
6963:
6960:
6958:
6955:
6953:
6950:
6949:
6947:
6932:
6929:
6927:
6924:
6922:
6919:
6917:
6914:
6912:
6909:
6908:
6906:
6902:
6896:
6893:
6891:
6888:
6886:
6883:
6881:
6878:
6876:
6873:
6871:
6868:
6866:
6863:
6862:
6860:
6856:
6850:
6847:
6845:
6842:
6840:
6837:
6835:
6832:
6830:
6827:
6825:
6822:
6820:
6817:
6815:
6812:
6810:
6807:
6805:
6802:
6800:
6797:
6795:
6792:
6790:
6787:
6786:
6784:
6780:
6774:
6771:
6769:
6766:
6764:
6761:
6759:
6756:
6754:
6751:
6749:
6746:
6744:
6741:
6739:
6736:
6734:
6731:
6729:
6726:
6724:
6721:
6719:
6716:
6714:
6711:
6709:
6706:
6704:
6701:
6699:
6696:
6694:
6691:
6689:
6686:
6684:
6681:
6679:
6676:
6674:
6671:
6669:
6666:
6664:
6661:
6659:
6656:
6654:
6651:
6649:
6646:
6644:
6641:
6639:
6636:
6634:
6631:
6629:
6626:
6624:
6621:
6619:
6616:
6614:
6611:
6609:
6606:
6605:
6603:
6599:
6593:
6590:
6588:
6585:
6583:
6580:
6578:
6575:
6573:
6570:
6568:
6565:
6563:
6560:
6558:
6555:
6553:
6550:
6549:
6547:
6543:
6533:
6530:
6528:
6525:
6524:
6522:
6518:
6512:
6509:
6507:
6504:
6502:
6499:
6497:
6494:
6492:
6489:
6487:
6484:
6482:
6479:
6477:
6474:
6472:
6469:
6468:
6466:
6464:
6460:
6454:
6451:
6449:
6446:
6445:
6443:
6439:
6433:
6430:
6428:
6425:
6423:
6420:
6418:
6415:
6413:
6410:
6408:
6405:
6403:
6400:
6398:
6395:
6393:
6390:
6389:
6387:
6383:
6377:
6374:
6372:
6369:
6367:
6364:
6362:
6359:
6358:
6356:
6352:
6346:
6343:
6341:
6338:
6336:
6333:
6331:
6328:
6326:
6323:
6321:
6318:
6316:
6313:
6311:
6308:
6306:
6303:
6301:
6298:
6296:
6293:
6291:
6288:
6286:
6283:
6282:
6280:
6278:
6274:
6271:
6259:
6252:
6249:
6247:
6244:
6241:
6220:
6217:
6214:
6193:
6190:
6187:
6166:
6163:
6162:
6160:
6156:
6152:
6145:
6140:
6138:
6133:
6131:
6126:
6125:
6122:
6109:
6105:
6101:
6100:Thomas Gasser
6097:
6093:
6089:
6088:Sabine Hadida
6085:
6081:
6078:
6075:
6071:
6067:
6063:
6059:
6055:
6052:
6049:
6045:
6041:
6037:
6036:Drew Weissman
6033:
6029:
6026:
6021:
6016:
6012:
6008:
6004:
6001:
5998:
5994:
5990:
5986:
5982:
5979:
5976:
5972:
5968:
5967:Angelika Amon
5964:
5960:
5957:
5954:
5950:
5946:
5942:
5938:
5935:
5932:
5928:
5924:
5923:Roeland Nusse
5920:
5916:
5913:
5910:
5906:
5902:
5898:
5894:
5893:Edward Boyden
5891:
5888:
5884:
5880:
5876:
5875:Victor Ambros
5872:
5868:
5865:
5862:
5858:
5854:
5850:
5846:
5845:Mahlon DeLong
5842:
5839:
5836:
5832:
5828:
5824:
5820:
5816:
5812:
5808:
5804:
5800:
5796:
5793:
5792:
5790:
5788:
5787:Life sciences
5784:
5777:
5773:
5770:
5767:
5766:Peter W. Shor
5763:
5762:David Deutsch
5759:
5755:
5752:
5749:
5745:
5742:
5739:
5735:
5732:
5729:
5728:Blayne Heckel
5725:
5721:
5718:
5715:
5712:
5709:
5705:
5701:
5697:
5694:
5691:
5687:
5684:
5681:
5677:
5674:
5671:
5670:David Spergel
5667:
5663:
5659:
5655:
5652:
5649:
5645:
5641:
5638:
5635:
5631:
5627:
5623:
5619:
5615:
5611:
5607:
5603:
5599:
5598:Atsuto Suzuki
5595:
5594:Daya Bay team
5591:
5587:
5584:
5581:
5577:
5573:
5569:
5568:Ronald Drever
5565:
5562:
5559:
5555:
5551:
5550:Brian Schmidt
5547:
5543:
5540:
5537:
5533:
5532:Michael Green
5530:
5527:
5524:
5521:
5517:
5513:
5512:Guido Tonelli
5509:
5505:
5501:
5497:
5493:
5489:
5486:
5483:
5482:Edward Witten
5479:
5475:
5471:
5467:
5463:
5459:
5458:Alexei Kitaev
5455:
5451:
5448:
5447:
5445:
5443:
5437:
5430:
5429:Simon Brendle
5427:
5424:
5421:
5418:
5415:
5412:
5411:Martin Hairer
5409:
5406:
5403:
5400:
5397:
5394:
5390:
5387:
5384:
5383:Jean Bourgain
5381:
5378:
5375:
5372:
5368:
5364:
5360:
5356:
5353:
5352:
5350:
5348:
5344:
5339:
5332:
5327:
5325:
5320:
5318:
5313:
5312:
5309:
5303:
5300:
5298:
5295:
5293:
5290:
5288:
5285:
5283:
5280:
5279:
5266:
5262:
5258:
5254:
5249:
5244:
5240:
5236:
5229:
5213:
5209:
5203:
5195:
5191:
5187:
5183:
5179:
5175:
5170:
5165:
5161:
5157:
5150:
5148:
5132:
5128:
5124:
5118:
5116:
5107:
5103:
5098:
5093:
5089:
5085:
5082:(1): 012028.
5081:
5077:
5073:
5066:
5058:
5054:
5050:
5046:
5042:
5038:
5034:
5030:
5025:
5020:
5016:
5012:
5008:
5007:Zeller, G. P.
5001:
4993:
4989:
4985:
4981:
4976:
4971:
4967:
4963:
4959:
4952:
4944:
4940:
4936:
4932:
4927:
4922:
4918:
4914:
4910:
4903:
4895:
4891:
4887:
4883:
4878:
4873:
4869:
4865:
4861:
4854:
4846:
4840:
4829:September 29,
4824:
4820:
4816:
4809:
4801:
4795:
4786:
4781:
4774:
4772:
4770:
4768:
4766:
4757:
4753:
4748:
4743:
4739:
4735:
4732:(1): 012042.
4731:
4727:
4723:
4716:
4714:
4705:
4699:
4690:
4685:
4678:
4676:
4674:
4664:
4659:
4652:
4650:
4648:
4639:
4635:
4631:
4627:
4623:
4619:
4614:
4609:
4605:
4601:
4594:
4576:
4572:
4565:
4558:
4556:
4540:
4536:
4530:
4522:
4516:
4508:
4504:
4500:
4496:
4492:
4488:
4483:
4478:
4475:(7): 072003.
4474:
4470:
4463:
4455:
4451:
4447:
4441:
4437:
4433:
4428:
4423:
4419:
4412:
4404:
4400:
4396:
4392:
4388:
4384:
4377:
4369:
4365:
4361:
4357:
4353:
4349:
4344:
4339:
4335:
4331:
4324:
4316:
4310:
4302:
4298:
4294:
4290:
4286:
4282:
4277:
4272:
4268:
4264:
4257:
4249:
4243:
4235:
4231:
4227:
4223:
4218:
4213:
4209:
4205:
4198:
4190:
4184:
4176:
4172:
4168:
4164:
4159:
4154:
4150:
4146:
4139:
4131:
4127:
4123:
4119:
4115:
4111:
4106:
4101:
4097:
4093:
4086:
4077:
4072:
4067:
4062:
4058:
4054:
4051:(1): 012030.
4050:
4046:
4042:
4035:
4033:
4031:
4029:
4027:
4025:
4023:
4021:
4019:
4009:
4004:
4000:
3993:
3991:
3989:
3987:
3985:
3983:
3981:
3979:
3977:
3975:
3966:
3960:
3952:
3948:
3944:
3940:
3936:
3932:
3927:
3922:
3919:(1): 012001.
3918:
3914:
3907:
3898:
3893:
3886:
3878:
3872:
3863:
3858:
3851:
3849:
3847:
3838:
3834:
3830:
3826:
3821:
3816:
3813:(3): 032004.
3812:
3808:
3801:
3785:
3781:
3777:
3773:
3769:
3762:
3746:
3742:
3738:
3731:
3715:
3711:
3707:
3700:
3691:
3686:
3682:
3678:
3674:
3670:
3669:
3664:
3641:
3637:
3631:
3623:
3617:
3609:
3605:
3601:
3597:
3592:
3587:
3584:(9): 093C02.
3583:
3579:
3572:
3564:
3558:
3550:
3546:
3542:
3538:
3534:
3530:
3525:
3520:
3517:(7): 072012.
3516:
3512:
3505:
3497:
3491:
3483:
3479:
3475:
3471:
3467:
3463:
3459:
3455:
3450:
3445:
3441:
3437:
3430:
3422:
3416:
3408:
3404:
3400:
3396:
3392:
3388:
3383:
3378:
3375:(1): 012010.
3374:
3370:
3363:
3355:
3349:
3341:
3337:
3333:
3329:
3325:
3321:
3316:
3311:
3307:
3303:
3296:
3288:
3282:
3274:
3270:
3266:
3262:
3258:
3254:
3249:
3244:
3240:
3236:
3229:
3221:
3215:
3207:
3203:
3199:
3195:
3191:
3187:
3182:
3177:
3173:
3169:
3162:
3154:
3148:
3140:
3136:
3132:
3128:
3124:
3120:
3115:
3110:
3107:(9): 092003.
3106:
3102:
3095:
3087:
3081:
3072:
3067:
3063:
3059:
3054:
3049:
3045:
3041:
3037:
3030:
3022:
3016:
3008:
3004:
3000:
2996:
2992:
2988:
2983:
2978:
2974:
2970:
2963:
2955:
2949:
2941:
2937:
2933:
2929:
2925:
2921:
2916:
2911:
2908:(7): 071103.
2907:
2903:
2896:
2888:
2882:
2874:
2870:
2866:
2862:
2858:
2854:
2849:
2844:
2841:(5): 051102.
2840:
2836:
2829:
2821:
2815:
2807:
2803:
2799:
2795:
2791:
2787:
2782:
2777:
2774:(3): 032002.
2773:
2769:
2762:
2754:
2748:
2740:
2736:
2732:
2728:
2724:
2720:
2715:
2710:
2706:
2702:
2695:
2693:
2691:
2689:
2687:
2685:
2683:
2681:
2679:
2677:
2675:
2673:
2671:
2669:
2667:
2665:
2656:
2652:
2648:
2644:
2640:
2636:
2631:
2626:
2622:
2618:
2611:
2603:
2599:
2595:
2591:
2587:
2583:
2576:
2560:
2556:
2552:
2548:
2544:
2540:
2536:
2532:
2528:
2523:
2518:
2514:
2510:
2506:
2499:
2497:
2495:
2486:
2480:
2472:
2468:
2464:
2460:
2455:
2450:
2446:
2442:
2435:
2427:
2421:
2413:
2409:
2405:
2401:
2397:
2393:
2389:
2385:
2380:
2375:
2371:
2367:
2360:
2358:
2349:
2343:
2335:
2331:
2327:
2323:
2319:
2315:
2311:
2307:
2302:
2297:
2294:(4): 041801.
2293:
2289:
2282:
2280:
2264:
2260:
2256:
2249:
2247:
2245:
2243:
2241:
2224:
2220:
2216:
2210:
2194:
2190:
2186:
2180:
2165:
2161:
2155:
2151:
2134:
2130:
2120:
2117:
2116:
2110:
2107:
2103:
2099:
2093:
2083:
2081:
2077:
2073:
2048:
2044:
2041:
2036:
2014:
2012:
2008:
2004:
2000:
1996:
1992:
1991:excited state
1988:
1984:
1902:
1828:
1827:
1826:
1824:
1821:. Because of
1820:
1816:
1736:
1732:
1728:
1724:
1714:
1705:
1702:
1698:
1695:
1685:
1682:
1677:
1673:
1664:
1655:
1653:
1648:
1644:
1641:
1638:
1637:scintillating
1628:
1622:interactions.
1620:
1616:
1613:
1612:
1611:
1608:
1606:
1602:
1598:
1594:
1590:
1586:
1582:
1578:
1574:
1565:
1559:ND280 Upgrade
1556:
1554:
1550:
1545:
1540:
1537:
1533:
1529:
1525:
1519:
1517:
1514:
1510:
1506:
1496:
1476:
1472:
1465:
1461:
1449:
1442:
1438:
1427:
1425:
1421:
1416:
1406:
1403:
1397:
1395:
1391:
1387:
1383:
1377:
1375:
1371:
1367:
1366:disappearance
1363:
1359:
1355:
1351:
1347:
1343:
1339:
1335:
1325:
1323:
1281:
1277:
1235:
1231:
1227:
1223:
1219:
1215:
1211:
1207:
1204:
1196:
1192:
1188:
1185:Detection of
1183:
1178:
1165:
1160:
1156:
1137:
1136:
1135:
1133:
1128:
1126:
1117:
1112:
1109:
1105:
1102:
1099:
1095:
1091:
1090:
1089:
1079:
1075:
1071:
1070:
1069:
1066:
1064:
1055:
1046:
1044:
1040:
1029:
1020:
1011:
1009:
1005:
1001:
996:
992:
988:
984:
974:
895:
894:
893:
891:
887:
882:
863:The Pi-Zero (
857:
848:
846:
842:
836:
823:
811:
797:
788:
785:
781:
778:
774:
771:
767:
758:
745:
742:
739:
738:
737:
728:
725:
720:
716:
712:
711:neutrino beam
705:Off-axis beam
702:
700:
696:
616:
612:
608:
604:
600:
596:
593:(Main Ring).
592:
588:
584:
580:
566:
552:
540:
529:Neutrino beam
526:
524:
520:
513:
506:
494:
489:
484:
480:
476:
472:
385:
381:
376:
374:
369:
365:
361:
357:
353:
349:
342:
338:
331:
327:
323:
316:
309:
302:
298:
295:
291:
287:
283:
279:
275:
274:cross-section
271:
268:
264:
258:
254:
213:
212:
211:
205:
201:
198:
194:
190:
184:
172:
168:
162:
158:
117:
116:
115:
107:
105:
101:
97:
93:
88:
86:
82:
75:
71:
68:
67:muon neutrino
64:
59:
57:
53:
49:
45:
41:
37:
33:
29:
25:
21:
6880:NEMO Project
6638:Double Chooz
6545:Construction
6431:
6277:Astronomical
6165:Cowan–Reines
6048:Pascal Mayer
5993:David Julius
5975:Zhijian Chen
5941:Peter Walter
5937:Joanne Chory
5909:Svante Pääbo
5807:Hans Clevers
5733:
5695:
5686:Charles Kane
5675:
5658:Gary Hinshaw
5613:
5576:Rainer Weiss
5563:
5522:(LHC) (2013)
5487:
5466:Andrei Linde
5238:
5234:
5228:
5216:. Retrieved
5202:
5159:
5155:
5135:. Retrieved
5126:
5079:
5075:
5065:
5049:1721.1/75437
5014:
5010:
5000:
4965:
4961:
4951:
4916:
4912:
4902:
4867:
4863:
4853:
4839:cite journal
4827:. Retrieved
4818:
4808:
4729:
4725:
4603:
4599:
4593:
4582:. Retrieved
4570:
4543:. Retrieved
4529:
4515:cite journal
4472:
4468:
4462:
4417:
4411:
4386:
4382:
4376:
4333:
4329:
4323:
4309:cite journal
4266:
4262:
4256:
4242:cite journal
4207:
4203:
4197:
4183:cite journal
4151:(1): 25–46.
4148:
4144:
4138:
4095:
4091:
4085:
4048:
4044:
3998:
3959:cite journal
3916:
3912:
3906:
3885:
3810:
3806:
3800:
3790:30 September
3788:. Retrieved
3772:Neutrino2020
3771:
3761:
3749:. Retrieved
3740:
3730:
3718:. Retrieved
3709:
3699:
3672:
3666:
3636:J. W. Cronin
3630:
3616:cite journal
3581:
3577:
3571:
3557:cite journal
3514:
3510:
3504:
3490:cite journal
3439:
3435:
3429:
3415:cite journal
3372:
3368:
3362:
3348:cite journal
3305:
3301:
3295:
3281:cite journal
3238:
3234:
3228:
3214:cite journal
3171:
3167:
3161:
3147:cite journal
3104:
3100:
3094:
3080:cite journal
3043:
3039:
3029:
3015:cite journal
2972:
2968:
2962:
2948:cite journal
2905:
2901:
2895:
2881:cite journal
2838:
2834:
2828:
2814:cite journal
2771:
2767:
2761:
2747:cite journal
2704:
2700:
2620:
2616:
2610:
2588:(1): 45–47.
2585:
2581:
2575:
2563:. Retrieved
2512:
2508:
2479:cite journal
2444:
2440:
2434:
2420:cite journal
2369:
2365:
2342:cite journal
2291:
2287:
2267:. Retrieved
2258:
2227:. Retrieved
2218:
2209:
2197:. Retrieved
2188:
2179:
2168:. Retrieved
2154:
2133:
2095:
2049:, for which
2015:
1980:
1720:
1711:
1697:scintillator
1691:
1669:
1652:antineutrino
1634:
1625:
1618:information.
1609:
1570:
1541:
1520:
1502:
1499:Beam upgrade
1463:
1447:
1440:
1433:
1412:
1409:Future plans
1398:
1378:
1348:facility in
1331:
1232:produced in
1200:
1129:
1122:
1101:scintillator
1083:
1078:scintillator
1067:
1060:
1035:
1026:
1017:
980:
953:
883:
862:
837:
833:
794:
773:scintillator
763:
734:
708:
697:and charged
587:accelerators
576:
525:experiment.
511:
504:
492:
490:
482:
383:
377:
373:leptogenesis
368:CP violation
340:
336:
329:
325:
321:
314:
313:
300:
265:Limits on a
256:
209:
182:
170:
166:is not zero.
160:
157:oscillations
113:
89:
73:
60:
36:oscillations
19:
18:
6486:KamLAND-Zen
6385:Accelerator
6263:(divided by
6158:Discoveries
6066:John Jumper
6018: [
6003:David Baker
5949:Kim Nasmyth
5931:Huda Zoghbi
5905:Helen Hobbs
5879:Gary Ruvkun
5819:Eric Lander
5690:Eugene Mele
5648:Cumrun Vafa
5636:team (2016)
5590:Kam-Biu Luk
5586:Yifang Wang
5496:Peter Jenni
5440:Fundamental
5367:Terence Tao
5363:Jacob Lurie
5347:Mathematics
4336:: 135–146.
4076:2433/235156
3640:V. L. Fitch
2975:(10): 114.
2043:octahydrate
1640:polystyrene
1509:accelerator
1439:parameters
1437:oscillation
1396:neutrinos.
1394:accelerator
1386:atmospheric
1322:oscillation
1206:cylindrical
1164:Combination
1162:detectors.
1132:oscillation
1043:cosmic rays
591:synchrotron
191:Search for
6946:Categories
6703:Kamiokande
6658:Gargamelle
6562:Baikal-GVD
6417:NA61/SHINE
6402:MicroBooNE
5901:John Hardy
5772:John Cardy
5572:Kip Thorne
5554:Adam Riess
5518:(CMS) and
5478:Ashoke Sen
5405:Alex Eskin
5248:1502.05199
5169:2109.00360
5162:: 166248.
5137:2021-10-07
4975:2109.03078
4926:2303.04481
4919:: 168534.
4877:1707.01785
4794:cite arXiv
4785:1901.03750
4698:cite arXiv
4689:1908.05141
4663:1805.04163
4613:1502.05199
4584:2021-09-29
4545:2020-03-31
4008:1704.08079
3897:1805.04163
3871:cite arXiv
3862:1609.04111
3820:2108.08219
3591:1904.09611
3449:1604.04406
3382:1605.07964
3315:2002.09323
3181:1602.03652
3053:1503.08815
2982:2002.11986
2915:1902.06529
2522:1910.03887
2454:1502.01550
2447:: 072010.
2269:2021-09-29
2229:20 January
2170:2020-03-31
2146:References
2076:our galaxy
1995:gamma rays
1723:gadolinium
1676:MicroMegas
1507:Main Ring
1475:gadolinium
1415:gadolinium
987:MicroMegas
348:conditions
262:parameter.
87:Universe.
6858:Cancelled
6678:Homestake
6628:Cuoricino
6592:SuperNEMO
6412:MiniBooNE
6261:Operating
6080:Carl June
6011:Dennis Lo
5520:Lyn Evans
5502:(ATLAS),
5454:Alan Guth
5340:laureates
5194:237372721
5106:121098709
5024:1305.7513
4992:1748-0221
4894:1748-0221
4756:1742-6588
4638:2050-3911
4454:117059077
4368:119280423
4343:1206.3553
4276:1308.3445
4217:1204.3666
4158:1012.0865
4130:118606685
4105:1111.5030
4098:: 48–63.
3926:1211.0469
3837:237195004
3524:1403.3140
3340:211252681
3273:118125266
3248:1411.6264
3114:1302.4908
3007:211532582
2940:119331309
2848:1410.8811
2781:1304.0841
2714:1106.1238
2655:119092531
2555:203951445
2441:Phys. Rev
2379:1403.1532
2301:1106.2822
2138:detector.
2072:supernova
1725:into the
1681:resistive
1581:electrons
1477:to allow
1420:Cherenkov
1230:electrons
1187:electrons
605:, mainly
479:Minnesota
475:Ash River
58:in 2027.
6904:See also
6849:WATCHMAN
6799:JEM-EUSO
6782:Proposed
6768:Soudan 2
6758:SciBooNE
6491:MAJORANA
6441:Collider
6361:Daya Bay
6305:Borexino
6267:neutrino
5632:and the
5620:and the
5608:and the
5600:and the
5592:and the
5377:Ian Agol
5212:Archived
5131:Archived
5057:54087013
4823:Archived
4575:Archived
4539:Archived
4507:22053653
4301:55993395
4210:: 1–31.
3951:55114627
3784:Archived
3751:18 April
3745:Archived
3720:19 April
3714:Archived
3549:53641707
3482:27564132
3474:27858422
3407:16748058
3206:35063421
3139:54889936
2873:54629105
2806:53322828
2739:55962579
2565:16 April
2559:Archived
2547:32296192
2471:34184232
2412:11484010
2404:24856687
2334:16654679
2326:21866992
2263:Archived
2223:Archived
2221:. CERN.
2193:Archived
2191:. CERN.
2164:Archived
2113:See also
2011:hydrogen
1987:absorbed
1654:energy.
1631:SuperFGD
1597:nucleons
1585:neutrino
1553:graphite
1197:detector
1072:Two new
1063:neutrino
1004:momentum
599:graphite
471:Fermilab
272:Various
30:") is a
6829:Nucifer
6648:EXO-200
6601:Retired
6557:ARIANNA
6453:SND@LHC
6407:MINERνA
6366:KamLAND
6354:Reactor
6320:IceCube
6290:ANTARES
6269:source)
6265:primary
6251:SN 1987
5734:Special
5696:Special
5676:Special
5602:KamLAND
5564:Special
5488:Special
5442:physics
5253:Bibcode
5218:1 April
5174:Bibcode
5084:Bibcode
5029:Bibcode
4931:Bibcode
4734:Bibcode
4618:Bibcode
4487:Bibcode
4391:Bibcode
4348:Bibcode
4281:Bibcode
4222:Bibcode
4163:Bibcode
4110:Bibcode
4053:Bibcode
3931:Bibcode
3677:Bibcode
3596:Bibcode
3529:Bibcode
3454:Bibcode
3387:Bibcode
3320:Bibcode
3253:Bibcode
3186:Bibcode
3119:Bibcode
3058:Bibcode
2987:Bibcode
2920:Bibcode
2853:Bibcode
2786:Bibcode
2719:Bibcode
2635:Bibcode
2590:Bibcode
2527:Bibcode
2384:Bibcode
2306:Bibcode
2199:9 March
2007:thermal
1819:nucleus
1815:nucleon
1694:plastic
1573:leptons
1549:cooling
1368:of the
1350:Tsukuba
1328:History
1276:showers
1193:in the
1116:ferrite
1098:plastic
1039:trigger
933:+ N’ +
770:plastic
747:energy.
715:degrees
699:leptons
695:hadrons
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