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''''T2K''' ("[[Tōkai, Ibaraki|Tokai]] to [[Kamioka, Gifu|Kamioka]]") is a [[particle physics]] experiment studying the [[neutrino oscillations|oscillations]] of the [[accelerator neutrinos]]. The experiment is conducted in [[Japan]] by the international cooperation of about 500 physicists and engineers with over 60 research institutions from several countries from [[Europe]], [[Asia]] and [[North America]]<ref>{{cite web |title=T2K experiment official page - T2K collaboration |url=https://t2k-experiment.org/t2k/collaboration/}}</ref> and it is a recognized [[CERN]] experiment (RE13).<ref>{{cite web |url=https://greybook.cern.ch/greybook/experiment/recognized |title=Recognized Experiments at CERN |website=The CERN Experimental Programme |publisher=CERN |access-date=9 March 2021}}</ref><ref>{{cite web |url=https://greybook.cern.ch/greybook/experiment/detail?id=RE13 |title=RE13/T2K : The long-baseline neutrino experiment |website=The CERN Experimental Programme |publisher=CERN |access-date=20 January 2020}}</ref> T2K was the first experiment which observed the appearance of [[electron neutrino]]s in [[muon neutrino]] [[particle beam|beam]],<ref name="1106.2822">{{Cite journal|arxiv=1106.2822 |author1=T2K Collaboration |title=Indication of Electron Neutrino Appearance from an Accelerator-produced Off-axis Muon Neutrino Beam |journal=Physical Review Letters |volume=107 |issue=4 |pages=041801 |year=2011 |doi=10.1103/PhysRevLett.107.041801 |pmid=21866992 |bibcode = 2011PhRvL.107d1801A }}</ref> it also provided the world best measurement of oscillation parameter ''θ''<sub>23</sub><ref name="1403.1532">{{Cite journal|arxiv=1403.1532 |author1=T2K Collaboration | title=Precise Measurement of the Neutrino Mixing Parameter \theta_{23} from Muon Neutrino Disappearance in an Off-Axis Beam | journal=Phys. Rev. Lett. |volume=112 | pages=181801 |year=2014 |issue=18 | doi=10.1103/PhysRevLett.112.181801 |pmid=24856687 }}</ref> and a hint of a significant [[CP violation|matter-antimatter asymmetry]] in neutrino oscillations.<ref>{{Cite journal|arxiv=1502.01550 |author1=T2K Collaboration | title=Measurements of neutrino oscillation in appearance and disappearance channels by the T2K experiment with 6.6E20 protons on target | journal=Phys. Rev. |volume=D91 | pages=072010 |year=2015 | doi=10.1103/PhysRevD.91.072010 }}</ref><ref name="cpnature">{{cite journal |title=Constraint on the matter–antimatter symmetry-violating phase in neutrino oscillations |journal=Nature |date=15 April 2020 |volume=580 |pages=339–344 |doi=10.1038/s41586-020-2177-0 |url=https://www.nature.com/articles/s41586-020-2177-0 |arxiv=1910.03887}}</ref> The measurement of the neutrino-antineutrino oscillation asymmetry may bring us closer to the explanation of the existence of our [[Baryon asymmetry|matter-dominated]] Universe.<ref>{{cite journal |last1=Fukugita |first1=M. |last2=Yanagida |first2=T. |title=Barygenesis without grand unification |journal=Physics Letters B |date=June 1986 |volume=174 |issue=1 |pages=45–47 |doi=10.1016/0370-2693(86)91126-3|bibcode=1986PhLB..174...45F }}</ref><ref>{{cite journal|last1=Mohapatra |first1=R N|last2=Antusch|first2=S|display-authors=1 |title=Theory of neutrinos: a white paper |journal=Reports on Progress in Physics |date=1 November 2007 |volume=70 |issue=11 |pages=1757–1867 |doi=10.1088/0034-4885/70/11/R02|arxiv=hep-ph/0510213|bibcode=2007RPPh...70.1757M}}</ref> The intense beam of muon neutrinos is produced in the [[J-PARC]] facility (Japan Proton Accelerator Research Complex) in [[Tōkai, Ibaraki|Tokai]] on the east coast of Japan. The beam is directed towards the [[Super-Kamiokande]] far detector located 295&nbsp;km away in the city of [[Hida, Gifu|Hida]], [[Gifu prefecture]]. The properties and composition of the neutrino flux are first measured by a system of near detectors located 280 m 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.<ref name="t2knim">{{Cite journal|author=T2K Collaboration |year=2011 |title=The T2K Experiment |journal=Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment |volume=659 |issue=1 |pages=106–135 |arxiv=1106.1238 |doi=10.1016/j.nima.2011.06.067 |bibcode = 2011NIMPA.659..106A }}</ref> ==Physics program== T2K experiment was proposed in 2003 with the following measurement goals:<ref name="t2knim"/> * The discovery of the {{SubatomicParticle|Muon neutrino}} → {{SubatomicParticle|Electron neutrino}} [[neutrino oscillation|oscillations]], and thus the confirmation that the last unknown mixing angle ''θ''<sub>13</sub> is not zero. * Precise measurement of the oscillation parameters Δ''m''{{su|b=23|p=2}} and ''θ''<sub>23</sub> via muon neutrino disappearance studies. * Search for [[sterile neutrino]] oscillations, which could be observed as a deficit of [[neutral current]] neutrino interactions. * Measurements of various interaction [[Cross section (physics)|cross-sections]] for different types of neutrinos and targets in an energy range of few GeV. Since the start of the data taking in 2010, the T2K experiment succeeded to provide a list of world-class results: * The confirmation of electron neutrino appearance in the muon neutrino beam ({{SubatomicParticle|Muon neutrino}}→{{SubatomicParticle|Electron neutrino}}), which was the first time when neutrinos produced in one flavour was explicitly observed in another flavour.<ref name="1106.2822" /><ref name="1304.0841">{{cite journal |author=T2K Collaboration |title=Evidence of electron neutrino appearance in a muon neutrino beam |journal=Physical Review D |date=5 August 2013 |volume=88 |issue=3 |pages=032002 |doi=10.1103/PhysRevD.88.032002|arxiv=1304.0841|bibcode=2013PhRvD..88c2002A }}</ref> * The most precise measurement of the ''θ''<sub>23</sub> parameter.<ref name="1403.1532" /> * The first significant constraint on the ''δ''<sub>CP</sub> parameter, responsible for the [[CP violation|matter-antimatter asymmetry]] in the neutrino sector.<ref name="cpnature" /> * Limits on a [[sterile neutrino]] oscillation parameters based on studies in the near ND280<ref>{{cite journal |author=T2K Collaboration |title=Search for short baseline nue disappearance with the T2K near detector |journal=Physical Review D |date=16 March 2015 |volume=91 |issue=5 |pages=051102 |doi=10.1103/PhysRevD.91.051102 |arxiv=1410.8811|bibcode=2015PhRvD..91e1102A }}</ref> and far Super-Kamiokande<ref>{{cite journal |author=T2K Collaboration |title=Search for light sterile neutrinos with the T2K far detector Super-Kamiokande at a baseline of 295 km |journal=Physical Review D |date=30 April 2019 |volume=99 |issue=7 |pages=071103 |doi=10.1103/PhysRevD.99.071103 |arxiv=1902.06529|bibcode=2019PhRvD..99g1103A}}</ref> detectors. * Various [[Cross section (physics)|cross-section]] measurements of electron<ref>{{cite arxiv | author=T2K Collaboration |title=Measurement of the charged-current electron (anti-)neutrino inclusive cross-sections at the T2K off-axis near detector ND280 |date=27 February 2020 |class=hep-ex | eprint=2002.11986}}</ref><ref>{{cite journal |author=T2K Collaboration |title=Measurement of the electron neutrino charged-current interaction rate on water with the T2K ND280 pi0 detector |journal=Physical Review D |date=19 June 2015 |volume=91 |issue=11 |pages=112010 |doi=10.1103/PhysRevD.91.112010|bibcode=2015PhRvD..91k2010A |doi-access=free }}</ref> and muon neutrino and antineutrino, including inclusive [[charged current]] (CC) interactions,<ref>{{cite journal | author=T2K Collaboration |title=Measurement of the inclusive numu charged current cross section on carbon in the near detector of the T2K experiment |journal=Physical Review D |date=7 May 2013 |volume=87 |issue=9 |doi=10.1103/PhysRevD.87.092003|arxiv=1302.4908}}</ref> CC interactions without pions<ref>{{cite journal | author=T2K Collaboration |title=Measurement of double-differential muon neutrino charged-current interactions on C8H8 without pions in the final state using the T2K off-axis beam |journal=Physical Review D |date=21 June 2016 |volume=93 |issue=11 |pages=112012 |doi=10.1103/PhysRevD.93.112012|arxiv=1602.03652|bibcode=2016PhRvD..93k2012A }}</ref><ref>{{cite journal |author=T2K Collaboration|title=Measurement of the numu charged-current quasielastic cross section on carbon with the ND280 detector at T2K |journal=Physical Review D |date=11 December 2015 |volume=92 |issue=11 |doi=10.1103/PhysRevD.92.112003|arxiv=1411.6264}}</ref><ref>{{cite arxiv |author=T2K Collaboration |title=First combined measurement of the muon neutrino and antineutrino charged-current cross section without pions in the final state at T2K |date=21 February 2020 |class=hep-ex |eprint=2002.09323}}</ref> and with single pion in the final state,<ref>{{cite journal |author=T2K Collaboration |title=First measurement of the muon neutrino charged current single pion production cross section on water with the T2K near detector |journal=Physical Review D |date=26 January 2017 |volume=95 |issue=1 |pages=012010 |doi=10.1103/PhysRevD.95.012010|arxiv=1605.07964|bibcode=2017PhRvD..95a2010A }}</ref> coherent pion production,<ref>{{cite journal |author=T2K Collaboration |title=Measurement of Coherent pi+ Production in Low Energy Neutrino-Carbon Scattering |journal=Physical Review Letters |date=4 November 2016 |volume=117 |issue=19 |pages=192501 |doi=10.1103/PhysRevLett.117.192501|pmid=27858422 |arxiv=1604.04406|bibcode=2016PhRvL.117s2501A }}</ref> [[neutral current]] interactions,<ref>{{cite journal |author=T2K Collaboration |title=Measurement of the neutrino-oxygen neutral-current interaction cross section by observing nuclear deexcitation gamma rays |journal=Physical Review D |date=31 October 2014 |volume=90 |issue=7 |pages=072012 |doi=10.1103/PhysRevD.90.072012|arxiv=1403.3140|bibcode=2014PhRvD..90g2012A }}</ref> etc. on different targets such as [[carbon]], [[water]] and [[iron]].<ref>{{cite journal |author=T2K Collaboration |title=Measurement of the muon neutrino charged-current cross sections on water, hydrocarbon and iron, and their ratios, with the T2K on-axis detectors |journal=Progress of Theoretical and Experimental Physics |date=September 2019 |volume=2019 |issue=9 |pages=093C02 |doi=10.1093/ptep/ptz070|arxiv=1904.09611 |bibcode=2019PTEP.2019i3C02A }}</ref> Future upgrades of T2K is expected to provide further constrain on the ''δ''<sub>CP</sub> phase by comparing oscillations of neutrinos to those of antineutrinos, as well as more precise measurements of Δ''m''{{su|b=23|p=2}} and ''θ''<sub>23</sub> parameters, and cross-section measurements which will extend our understanding of neutrino interactions and thus improve theoretical models used in neutrino generators.<ref name="upgradeproposal">{{cite arxiv |author=T2K Collaboration |title=Proposal for an Extended Run of T2K to 20E21 POT |date=13 September 2016 |class=hep-ex |eprint=1609.04111}}</ref><ref name="1805.04163">{{cite arxiv |author=Hyper-Kamiokande Collaboration |title=Hyper-Kamiokande Design Report |date=28 November 2018 |class=physics.ins-det |eprint=1805.04163}}</ref> ==Neutrino beam== {{multiple image | align = right | perrow = 2 / 1 | total_width = 415 | image1 = The entire view of J-PARC.jpg | caption1 = Bird's-eye view of the entire facility. | image2 = Superconducting Magnets J-PARC.jpg | caption2 = Superconducting magnets under construction in 2008 to veer the proton beam towards Kamioka. | image3 = Neutrino beam production.svg | caption3 = Neutrino beam production scheme. }} T2K uses a muon neutrino or muon antineutrino [[accelerator neutrino|beam]] produced at the [[J-PARC]] facility using a proton beam gradually accelerated to 30 GeV by a system of three [[particle accelerator|accelerators]]: 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 [[synchrotron]] (Main Ring). [[Proton]]s collide with a [[graphite]] target, producing [[meson]]s, mainly [[pion]]s and [[kaon]]s, which are then focused by a set of three [[magnetic horn]]s 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 {{SubatomicParticle|Muon+}} and {{SubatomicParticle|Muon neutrino}}, forming a muon neutrino beam, while negative pions and kaons decay mainly into {{SubatomicParticle|Muon-}} and {{SubatomicParticle|Muon antineutrino}}, forming a muon antineutrino beam. All remaining [[hadron]]s and charged [[lepton]]s 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.<ref name="t2knim"/> ===Off-axis beam=== T2K is the first experiment in which the concept of off-axis [[accelerator neutrino|neutrino beam]] was realized. The neutrino beam at J-PARC is designed so that it can be directed 2 to 3 [[degree (angle)|degrees]] away from the [[Super-Kamiokande]] 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&nbsp;km is maximal for around 600&nbsp;MeV neutrinos. In this neutrino energy range, the dominant type of neutrino interactions are [[charged current]] 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 with meson production, which are background in the oscillation analysis in the T2K experiment.<ref name="t2knim"/><ref name="t2kflux">{{cite journal |author=T2K Collaboration |title=T2K neutrino flux prediction |journal=Physical Review D |date=2 January 2013 |volume=87 |issue=1 |pages=012001 |doi=10.1103/physrevd.87.012001|arxiv=1211.0469|bibcode=2013PhRvD..87a2001A }}</ref> ==Near detectors== The near detector complex<ref name="t2knim"/> is located at a distance of 280 meters 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: * INGRID detector (Interactive Neutrino GRID) located on the axis of the neutrino beam, * ND280 detector located 2.5° away from the beam axis, i.e. at the same angle as the far detector. * 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 energy.<ref name="babymind">{{cite journal|display-authors=1 |last1=Antonova |first1=M. |last2=Asfandiyarov |first2=R. |title=Baby MIND: A magnetised spectrometer for the WAGASCI experiment |arxiv=1704.08079 |year=2017}}</ref><ref name="wagasci">{{cite journal|display-authors=1 |last1=Ovsiannikova |first1=T |last2=Antonova |first2=M |title=The new experiment WAGASCI for water to hydrocarbon neutrino cross section measurement using the J-PARC beam |journal=Journal of Physics: Conference Series |date=5 February 2016 |volume=675 |issue=1 |pages=012030 |doi=10.1088/1742-6596/675/1/012030|doi-access=free }}</ref> ===Signal readout=== [[File:Scintillator.svg|300px|thumb|Principle of operation of a scintillator in the T2K near detectors.]] Except for the [[Time Projection Chamber]]s in ND280, the entire active material (enabling particle tracking) of the near detectors is [[plastic]] [[scintillator]]. The light produced by traversing particles in the plastic scintillator bars and planes is collected by [[wavelength shifter|wavelength-shifting]] [[optical fiber|fibres]] and detected by Hamamatsu [[Silicon photomultiplier|Multi-pixel photon counters]] 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 traversing particles.<ref name="t2knim"/> ===INGRID detector=== 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 modules outside the cross. Height and width of the arms are 10 meters. 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.<ref name="t2knim"/> ===ND280 detector=== {{multiple image | align = right | total_width = 400 | image1 = J-PARC T2K ND280 Pit.jpg | caption1 = ND280 under construction. | image2 = ND280 detector scheme.png | caption2 = Exploded view of the ND280 detector. }} 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 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.<ref name="t2knim"/> 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 [[UA1 experiment]] producing 0.2 T uniform horizontal field and instrumented with scintillator planes constituting the Side Muon Range Detector.<ref name="t2knim"/> ====Pi-Zero detector==== [[File:Nd280 p0d layers structure.png|180px|thumb|Pi-Zero detector scheme.]] The Pi-Zero ({{SubatomicParticle|Pion0}}) Detector (P0D) contains 40 plastic scintillator module planes, which in the central part are interleaved with 2.8&nbsp;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. The main goal of the Pi-Zero Detector is measurement neutral [[pion]]s production in [[neutral current]] neutrino interactions on water: : {{SubatomicParticle|Muon neutrino}} + N → {{SubatomicParticle|Muon neutrino}} + N’ + {{SubatomicParticle|Pion0}} This reaction can mimic electron neutrino interactions because photons from {{SubatomicParticle|Pion0}} 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.<ref name="t2knim"/><ref>{{cite journal |first1=S|last1=Assylbekov|first2=B E|last2=Berger|display-authors=1 |title=The T2K ND280 off-axis pi–zero detector |journal=Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment |date=September 2012 |volume=686 |pages=48–63 |doi=10.1016/j.nima.2012.05.028|arxiv=1111.5030|bibcode=2012NIMPA.686...48A}}</ref> ====Time projection chambers==== Three [[time projection chamber]]s (TPCs) are gas-tight rectangular boxes, with a cathode plane in the centre and readout [[MicroMegas detector|MicroMegas]] modules at both sides parallel to the cathode. TPCs are filled with [[argon]]-based drift gas under atmospheric pressure. Charged particles crossing TPC [[ionisation|ionise]] 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 MicroMegas modules, and X coordinate is based on the electrons drift time. In the magnetic field, the curvature of this path allows to determine [[electric charge|charge]] and [[momentum]] of the particle, and the amount of the ionisation electrons per unit distance is used to identify particles based on the [[Bethe formula|Bethe-Bloch formula]].<ref name="t2knim"/><ref>{{cite journal |author=T2K ND280 TPC collaboration |title=Time projection chambers for the T2K near detectors |journal=Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment |date=May 2011 |volume=637 |issue=1 |pages=25–46 |doi=10.1016/j.nima.2011.02.036|arxiv=1012.0865|bibcode=2011NIMPA.637...25A }}</ref> ====Fine-grained detectors==== 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 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 detector at Super-Kamiokande is water-based. Cross sections on carbon and on the water can be determined from a comparison of neutrino interactions in the two FGDs.<ref name="t2knim"/><ref>{{cite journal |author=T2K ND280 FGD Collaboration |title=The T2K fine-grained detectors |journal=Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment |date=December 2012 |volume=696 |pages=1–31 |doi=10.1016/j.nima.2012.08.020 |arxiv=1204.3666|bibcode=2012NIMPA.696....1A }}</ref> ====Electromagnetic Calorimeter==== 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 providing additional information relevant for their identification.<ref name="t2knim"/><ref>{{cite journal |author=T2K UK Collaboration |title=The electromagnetic calorimeter for the T2K near detector ND280 |journal=Journal of Instrumentation |date=17 October 2013 |volume=8 |issue=10 |pages=P10019 |doi=10.1088/1748-0221/8/10/P10019 |arxiv=1308.3445|bibcode=2013JInst...8P0019A }}</ref> ====Side Muon Range Detector==== 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 stopped in the calorimeter. SMRD can also act as a [[trigger (particle physics)|trigger]] for [[cosmic rays]]. Finally, it can help identify beam interactions in the surrounding walls and in the magnet itself.<ref name="t2knim"/><ref>{{cite journal |first1=S|last1=Aoki|first2=G|last2=Barr|display-authors=1|title=The T2K Side Muon Range Detector (SMRD) |journal=Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment |date=January 2013 |volume=698 |pages=135–146 |doi=10.1016/j.nima.2012.10.001|arxiv=1206.3553|bibcode=2013NIMPA.698..135A}}</ref> ===WAGASCI-Baby MIND=== [[File:Wagasci and ND280 neutrino flux.png|200px|thumb|right|The predicted T2K neutrino flux at the site of the WAGASCI-Baby MIND (red line) and of the ND280 (black line) detectors.]] WAGASCI-Baby MIND is a new detector located next to the INGRID and ND280 detectors, devoted to [[neutrino]] interaction studies. It provided the first neutrino beam data using a full detector setup during the 2019/2020 winter run.<ref name="babymind"/><ref name="wagasci"/> The WAGASCI-Baby MIND consists of several sub-detectors: * Two new [[water]]-[[scintillator]] 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. Thanks to such a structure, a high water to scintillator mass ratio was obtained (80% H<sub>2</sub>O + 20% CH) and the acceptance is high and approximately constant in all directions.<ref name="babymind"/><ref name="wagasci"/> * One Proton Module, the same as in the [[T2K experiment#INGRID detector|INGRID]] detector, made of plain [[plastic]] [[scintillator]] (CH) bars, that acts as the main CH target and particle tracker.<ref name="babymind"/><ref name="wagasci"/> * Two WallMRD (Wall Muon Range Detector) that are non-magnetized muon spectrometers to detect side going muons. They are made of passive [[iron]] planes intertwined with active scintillator planes.<ref name="babymind"/><ref name="wagasci"/> * One Baby MIND (prototype Magnetized Iron Neutrino Detector) that is a magnetized muon spectrometer to detect forward-going muons. Baby MIND sports an original configuration of scintillation modules intertwined with magnetized [[ferrite (iron)|ferrite]] 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 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.<ref name="babymind"/> All the active material in the detectors is made up of plastic scintillator and is read as explained in section [[T2K experiment#Signal readout|Signal readout]].<ref name="babymind"/><ref name="wagasci"/> The main goal of the WAGASCI-Baby MIND detector is a reduction of the systematic error in the T2K [[neutrino oscillation|oscillation]] analysis, which will be achieved thanks to its complementarity with respect to the ND280 detector: * Different target material between ND280 (80% CH + 20% H<sub>2</sub>O) and SK (pure H<sub>2</sub>O) forces us to rely on cross-section models to disentangle the H<sub>2</sub>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<sub>2</sub>O) and plastic (CH) with 3% accuracy.<ref name="babymind"/><ref name="wagasci"/> * 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 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.<ref name="babymind"/><ref name="wagasci"/> * 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 detectors. [[linear combination|Combination]] of measurements from these detectors will provide an improved constraint on the neutrino cross-sections as a function of their energy.<ref name="babymind"/><ref name="wagasci"/> ==Super-Kamiokande== {{main|Super-Kamiokande}} [[File:Superkamiokande electron muon discriminator.png|thumb|Detection of [[electron]]s and [[muon]]s in the [[Super-Kamiokande]] detector.]] 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 [[stainless steel]] [[cylinder|cylindrical]] tank of about 40 m height and diameter, filled with 50,000 tons of [[water]] and instrumented with around 13,000 [[photomultiplier tube]]s (PMT). It detects a [[cone]] of [[Cherenkov radiation|Cherenkov light]] emitted by charged particles moving in water faster than light in this medium. Its goal is to measure [[muon]]s and [[electron]]s produced in [[charged current]] quasielastic interactions (CCQE) of {{SubatomicParticle|Muon neutrino}} and {{SubatomicParticle|Electron neutrino}}, 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 [[particle shower|showers]], observed by PMTs as a ring with fuzzy edges. Neutrino energy is calculated based on the direction and energy of a charged [[lepton]] produced in the CCQE interaction. In this way, {{SubatomicParticle|Muon neutrino}} and {{SubatomicParticle|Electron neutrino}} spectra are determined, leading to the measurement of the [[neutrino oscillation|oscillation]] parameters relevant for muon neutrino disappearance and electron neutrino appearance.<ref name="t2knim"/><ref>{{cite journal |author=The Super-Kamiokande Collaboration |title=The Super-Kamiokande detector |journal=Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment |date=April 2003 |volume=501 |issue=2–3 |pages=418–462 |doi=10.1016/S0168-9002(03)00425-X|bibcode=2003NIMPA.501..418F }}</ref> ==History== T2K is a successor of the KEK to Kamioka ([[K2K experiment|K2K]]) experiment, which ran from 1999 till 2004. In the [[K2K experiment]], an [[accelerator neutrino|accelerator beam]] of muon neutrinos was produced at [[KEK]] facility in [[Tsukuba, Ibaraki|Tsukuba]] ([[Japan]]) and sent towards the [[Super-Kamiokande]] detector, located 250&nbsp;km away. The K2K experiment results confirmed at the confidence level of 99.9985% (4.3 [[Standard deviation|σ]]) the [[neutrino oscillation|disappearance]] of the [[muon neutrino]]s and were consistent with the previous measurements of oscillation parameters measured by the Super-Kamiokande detector for [[Neutrino#Atmospheric|atmospheric neutrino]]s.<ref>{{cite book |last1=Oyama |first1=Yuichi |title=Nuclear Science and Safety in Europe |chapter=Results from K2K and status of T2K |series=NATO Security through Science Series |year=2006 |pages=113–124 |doi=10.1007/978-1-4020-4965-1_9 |arxiv=hep-ex/0512041|isbn=978-1-4020-4963-7 }}</ref><ref>{{cite journal |author=K2K Collaboration |title=Measurement of neutrino oscillation by the K2K experiment |journal=Physical Review D |date=12 October 2006 |volume=74 |issue=7 |pages=072003 |doi=10.1103/PhysRevD.74.072003|arxiv=hep-ex/0606032|bibcode=2006PhRvD..74g2003A }}</ref> 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 installed in the fall of 2010. T2K far detector is the large Super-Kamiokande detector, which has been running since 1996 and studying [[proton lifetime]] and oscillations of [[Neutrino#Atmospheric|atmospheric]], [[solar neutrino|solar]] and [[accelerator neutrino|accelerator]] neutrinos.<ref name="t2knim"/> 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 [[Great Tohoku Earthquake]] in March 2011. The proton beam power, and thus the neutrino beam intensity, was constantly growing, reaching by February 2020 the power of 515&nbsp;kW and a total number of accumulated protons on target of 3.64×10<sup>21</sup> protons<ref>{{cite web |title=T2K experiment official page - T2K Run 10 |url=https://t2k-experiment.org/2020/02/t2k-run-10-ended-with-record-beam-power/}}</ref> with 55% of data in neutrino-mode and 45% in antineutrino-mode. In April 2020, T2K collaboration published results strongly constraining the ''δ''<sub>CP</sub> phase. The results reject at 95% confidence the hypothesis of no CP violation (including the possibility of ''δ''<sub>CP</sub> equal to ''π'').<ref name="cpnature"/><ref>{{cite news |last1=Cho |first1=Adrian |title=Skewed neutrino behavior could help explain matter’s dominion over antimatter |url=https://www.sciencemag.org/news/2020/04/skewed-neutrino-behavior-could-help-explain-matter-s-dominion-over-antimatter |access-date=19 April 2020 |work=Science {{!}} AAAS |date=15 April 2020 |language=en}}</ref> The results also reject at the 3σ (99.7%) significance level almost half of the possible values of this parameter and give a strong hint that CP violation may be large in the neutrino sector.<ref name="cpnature"/><ref>{{cite web |url=https://www.bbc.com/news/science-environment-52297058 |title=Biggest cosmic mystery 'step closer' to solution |last=Rincon |first=Paul |date=16 April 2020 |website=BBC News website}}</ref> ==Future plans== The T2K experiment operated in the current form until 2020. In 2021 the first data run with Gadollinium loaded into the Super-Kamiokande far detector was taken.<ref name="panik2021">{{cite web |last1=Vilela |first1=Cristovao |title=The status of T2K and Hyper-Kamiokande experiments |url=https://indico.lip.pt/event/592/contributions/3550/ |website=PANIC 2021 Conference |date=September 5-10, 2021}}</ref>{{rp|12}} 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).<ref name="lomonosov2021">{{cite web |last1=Kudenko |first1=Yury |title=Physics and status of SuperFGDdetector for T2K experiment |url=https://lomcon.ru/files/20LomCon/presentations/Presenteations/19/lomonosov2021_kudenko.pdf |website=The 20th Lomonosov Conference on Elementary Particle Physics |date=August 19-25, 2021 |page=17-18}}</ref><ref name="upgradeproposal"/> In 2027, the successor of the T2K experiment will be launched, the Hyper-Kamiokande (HK) experiment, with the new, 250,000-ton water [[Cherenkov radiation|Cherenkov]] far detector - the [[Hyper-Kamiokande]] detector.<ref name="panik2021"/>{{rp|20}}<ref>{{cite journal |author=Hyper-Kamiokande Proto-Collaboraion |title=Physics Potential of a Long Baseline Neutrino Oscillation Experiment Using J-PARC Neutrino Beam and Hyper-Kamiokande |journal=Progress of Theoretical and Experimental Physics |date=19 May 2015 |volume=2015 |issue=5 |pages=53C02–0 |doi=10.1093/ptep/ptv061 |arxiv=1502.05199 |bibcode=2015PTEP.2015e3C02A |issn=2050-3911}}</ref><ref name="hyperk">{{cite arxiv |author=Hyper-Kamiokande Proto-Collaboration |title=Hyper-Kamiokande Design Report |date=28 November 2018 |class=physics.ins-det |eprint=1805.04163}}</ref> The building of an additional Intermediate Water Cherenkov detector at a distance of around 2&nbsp;km is also considered for the HK experiment.<ref name="hyperk"/> ===T2K-II=== The 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 [[neutrino oscillation|oscillation]] parameters ''θ''<sub>23</sub> and Δ''m''{{su|b=23|p=2}} with a precision of 1.7° and 1%, respectively, as well as a confirmation at the level of 3 [[Standard deviation|σ]] or more of the matter-antimatter asymmetry in the neutrino sector in a wide range of possible true values of ''δ''<sub>CP</sub> - the parameter responsible for the [[CP violation|CP]] (matter-antimatter) asymmetry. Achievement of these goals requires reduction of the statistical and systematic errors, and thus a significant upgrade of the beamline and the ND280 detector, as well as improvements in the software and analysis methods.<ref name="upgradeproposal"/> ====Beam upgrade==== The beam upgrade plan requires one year long shut down of the [[J-PARC]] Main Ring [[particle accelerator|accelerator]] in 2021, followed by a constant gradual increase of the [[proton]] [[particle beam|beam]] power until the start of the HK experiment. The beam power should reach 750&nbsp;kW in 2022 and then grow to 1.3 MW by 2029.<ref name="beamupgradetdr">{{cite arxiv |author=T2K Collaboration and J-PARC Neutrino Facility Group |title=J-PARC Neutrino Beamline Upgrade Technical Design Report |date=14 August 2019 |class=physics.ins-det |eprint=1908.05141}}</ref> In February 2020, the proton beam power reached 515&nbsp;kW with 2.7x10<sup>14</sup> protons per pulse and with 2.48 seconds between pulses (so-called repetition cycle). To reach 750&nbsp;kW, the repetition cycle will be reduced to 1.32 s with 2.0x10<sup>14</sup> protons per pulse, while for 1.3 MW the repetition cycle has to be further decreased to 1.16 s and the number of protons per pulse has to increase to 3.2x10<sup>14</sup>. In addition to increasing the primary proton beam power, the current in the [[magnetic horn|horns]] focusing secondary particles ([[pion]]s, [[kaon]]s, etc.) with a chosen [[electric charge]] 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 the anti-neutrino mode beam) by around 5-10%.<ref name="beamupgradetdr"/><ref name="beamupgradeprogramme">{{cite journal |last1=Friend |first1=M |title=J-PARC accelerator and neutrino beamline upgrade programme |journal=Journal of Physics: Conference Series |date=September 2017 |volume=888 |issue=1 |pages=012042 |doi=10.1088/1742-6596/888/1/012042 |bibcode=2017JPhCS.888a2042F |language=en |issn=1742-6588|doi-access=free }}</ref> Reduction of the repetition cycle will require a series of hardware upgrades, including a major upgrade of the Main Ring [[power supply|power supplies]] 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 [[cooling]] capacity of the secondary beamline components such as the [[graphite]] target, the magnetic horns and the beam dump, as well as disposal of a larger amount of irradiated cooling water.<ref name="beamupgradetdr"/><ref name="beamupgradeprogramme"/> ====ND280 Upgrade==== [[File:Nd280upgrade scheme.png|thumb|Scheme of the inner part of the ND280 detector after planned upgrade.]] The current design of the ND280 detector is optimized for the detection and reconstruction of forward-going [[lepton]]s ([[muon]]s and [[electron]]s), but it also has a number of limitations, like low reconstruction efficiency of particles produced almost perpendicular and backward w.r.t. the direction of the interacting [[neutrino]], 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 ([[pion]]s, [[kaon]]s, [[nucleon]]s) were lost, may be mis-reconstructed as CCQE and introduce a [[Bias (statistics)|bias]] in the reconstructed neutrino energy spectrum. Thus, it is essential to optimize the detector to be sensitive to additional particles and [[Nuclear structure|nuclear effects]]. Three main measures need to be taken to address these issues: * The detector needs to efficiently detect the nucleons in the final state of neutrino interactions. For this, the detection thresholds need to be lowered. * 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 information. * 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 interactions. 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 maintain their sandwiched structure and continue to detect forward going leptons and high momentum hardons. 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.<ref name="nd280upgradetdr">{{cite arxiv |author=T2K Collaboration|title=T2K ND280 Upgrade - Technical Design Report |date=11 January 2019 |class=physics.ins-det |eprint=1901.03750}}</ref> The installation of the new sub-detectors into ND280 will be done in 2022.<ref name="lomonosov2021"/><ref name="nd280upgradetdradd">{{cite journal |author=The T2K ND280 Upgrade Working Group|title=NP07: ND280 Upgrade project |date=June 19, 2020 |url=http://cds.cern.ch/record/2713578 |journal=CERN Scientific Committee Paper |volume=CERN-SPSC-2020-008. SPSC-SR-267}}</ref>{{rp|18}} =====SuperFGD===== The SuperFGD is a 2m x 2m x 0.5m detector consisting of approximately 2 million 1&nbsp;cm<sup>3</sup> [[scintillator|scintillating]] [[polystyrene]] [[cube]]s. The cubes are woven with a series of [[optical fiber|optical fibres]] 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 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 [[antineutrino]] energy.<ref name="nd280upgradetdr"/> =====HATPC===== The High Angle [[Time Projection Chamber]]s (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 [[MicroMegas detector|MicroMegas]] 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 [[Electrical resistance and conductance|resistive]] 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.<ref name="nd280upgradetdr"/> =====TOF===== The six Time-of-Flight (TOF) detectors surrounding the HATPCs and SuperFGD are a series of [[plastic]] [[scintillator]] layers designed to identify the particle direction sense through the measurement of the [[time of flight]] for each crossing track with a timing resolution of the order of 600 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.<ref name="nd280upgradetdr"/> =====Impact on Neutrino Oscillation Physics===== 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 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.<ref name="nd280upgradetdr"/> ===Hyper-Kamiokande experiment=== {{main|Hyper-Kamiokande}} The successor of the T2K experiment, the [[Hyper-Kamiokande]] (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 Hyper-Kamiokande detector, and possibly also a new intermediate detector 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.<ref name="panik2021"/>{{rp|20}}<ref name="hyperk"/><ref name="hyperkstart">{{cite news|url=http://www.j-parc.jp/c/en/topics/2020/02/12000416.html|title=The Hyper-Kamiokande project is officially approved.|date=12 February 2020}}</ref><ref>{{cite journal |author=Hyper-Kamiokande Proto-Collaboraion |title=Physics potential of a long-baseline neutrino oscillation experiment using a J-PARC neutrino beam and Hyper-Kamiokande |journal=Progress of Theoretical and Experimental Physics |date=19 May 2015 |volume=2015 |issue=5 |pages=53C02–0 |doi=10.1093/ptep/ptv061 |arxiv=1502.05199|bibcode=2015PTEP.2015e3C02A }}</ref> ====Hyper-Kamiokande detector==== The Hyper-Kamiokande detector will be a [[water]] [[Cherenkov radiation|Cherenkov]] detector, 5 times larger (258 kton of water) than the [[Super-Kamiokande]] detector. It will be a [[cylinder]] of 74 meters diameter and 60 meter height with 40000 [[photomultiplier]] tubes of 50&nbsp;cm diameter and 6700 photomultiplier tubes of 20&nbsp;cm diameter. It will be located 8&nbsp;km south from the Super-Kamiokande detector in the Tochibora mine, 650 meters under the peak of Nijuugo mountain, at the same off-axis angle (2.5°) to the neutrino beam centre and in the same distance (295&nbsp;km) from the beam production place at [[J-PARC]]. The HK detector construction began in 2020 and the start of data collection is expected in 2027.<ref name="panik2021"/>{{rp|24}}<ref name="hyperk"/><ref name="hyperkstart"/> ====Intermediate Water Cherenkov==== The Intermediate Water Cherenkov Detector (IWCD) will be located at a distance of 0.7–2&nbsp;km from the neutrino production place. It would be a cylinder filled with water of 10 m diameter and 50 m height with a 10 m tall structure instrumented with around 3000 photomultiplier tubes of a 20&nbsp;cm diameter. The structure will be moved in a vertical direction by a crane system, providing measurements of neutrino interactions at different off-axis angles, spanning from 1° to 4°, and thus for different energy spectra. Combining the results from different off-axis angles it is possible to extract the results for nearly monochromatic neutrino spectrum without relying on theoretical models of neutrino interactions to reconstruct neutrino energy. Usage of the same type of detector as the far detector with almost the same angular and momentum acceptance allows comparing results from these two detectors without relying on detectors response simulations. These two facts, independence from the neutrino interaction and detector response models, will enable to minimise systematic error in the oscillation analysis. Additional advantages of such a design of the detector is a possibility to search for [[sterile neutrino|sterile]] [[neutrino oscillation|oscillation]] pattern for different off-axis angles and to obtain a cleaner sample of [[electron neutrino]] interaction, whose fraction is larger for the larger off-axis angle.<ref name="hyperk"/>{{rp|47–50}}<ref>{{cite arxiv |author=nuPRISM Collaboration |title=Letter of Intent to Construct a nuPRISM Detector in the J-PARC Neutrino Beamline |date=13 December 2014 |class=physics.ins-det |eprint=1412.3086}}</ref><ref>{{cite web |author=nuPRISM Collaboration |title=Proposal for the NuPRISM Experiment in the J-PARC Neutrino Beamline |url=https://j-parc.jp/researcher/Hadron/en/pac_1607/pdf/P61_2016-17.pdf |date=7 July 2016}}</ref> It is planned that the IWCD will be finalised in 2024 and will start to take data from 2025, yet before launching the HK experiment.<ref>{{cite web |last1=Yoshida |first1=Tomoyo |title=J-PARC E61 experiment |url=https://indico.cern.ch/event/531125/contributions/2858586/attachments/1604730/2545546/4_J-PARC_E61_experiment.pdf |publisher=Lake Louise Winter Institute |date=21 February 2018}}</ref> ==See also== * [[Kamioka Observatory]] ==Notes== {{reflist}} ==External links== {{Commons|T2K}} * [http://www.t2k-experiment.org/ T2K Experiment Official Website] * [http://www-sk.icrr.u-tokyo.ac.jp/sk/index-e.html Super-Kamiokande Official Website] * [http://www-sk.icrr.u-tokyo.ac.jp/realtimemonitor/ Super-Kamiokande Realtime Monitor] * [https://www.youtube.com/watch?v=tBrFrdSneZg Neutrino physics - The T2K experiment - YouTube] * [https://www.youtube.com/watch?v=cs02i8TIphs Inside Japan's Big Physics | Part one: Super Kamiokande - YouTube] {{Breakthrough Prize laureates}} {{Neutrino detectors}} [[Category:Accelerator neutrino experiments]] [[Category:Science and technology in Japan]] [[Category:CERN experiments]] [[Category:Fixed-target experiments]]'
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''''T2K''' ("[[Tōkai, Ibaraki|Tokai]] to [[Kamioka, Gifu|Kamioka]]") is a [[particle physics]] experiment studying the [[neutrino oscillations|oscillations]] of the [[accelerator neutrinos]]. The experiment is conducted in [[Japan]] by the international cooperation of about 500 physicists and engineers with over 60 research institutions from several countries from [[Europe]], [[Asia]] and [[North America]]<ref>{{cite web |title=T2K experiment official page - T2K collaboration |url=https://t2k-experiment.org/t2k/collaboration/}}</ref> and it is a recognized [[CERN]] experiment (RE13).<ref>{{cite web |url=https://greybook.cern.ch/greybook/experiment/recognized |title=Recognized Experiments at CERN |website=The CERN Experimental Programme |publisher=CERN |access-date=9 March 2021}}</ref><ref>{{cite web |url=https://greybook.cern.ch/greybook/experiment/detail?id=RE13 |title=RE13/T2K : The long-baseline neutrino experiment |website=The CERN Experimental Programme |publisher=CERN |access-date=20 January 2020}}</ref> T2K was the first experiment which observed the appearance of [[electron neutrino]]s in [[muon neutrino]] [[particle beam|beam]],<ref name="1106.2822">{{Cite journal|arxiv=1106.2822 |author1=T2K Collaboration |title=Indication of Electron Neutrino Appearance from an Accelerator-produced Off-axis Muon Neutrino Beam |journal=Physical Review Letters |volume=107 |issue=4 |pages=041801 |year=2011 |doi=10.1103/PhysRevLett.107.041801 |pmid=21866992 |bibcode = 2011PhRvL.107d1801A }}</ref> it also provided the world best measurement of oscillation parameter ''θ''<sub>23</sub><ref name="1403.1532">{{Cite journal|arxiv=1403.1532 |author1=T2K Collaboration | title=Precise Measurement of the Neutrino Mixing Parameter \theta_{23} from Muon Neutrino Disappearance in an Off-Axis Beam | journal=Phys. Rev. Lett. |volume=112 | pages=181801 |year=2014 |issue=18 | doi=10.1103/PhysRevLett.112.181801 |pmid=24856687 }}</ref> and a hint of a significant [[CP violation|matter-antimatter asymmetry]] in neutrino oscillations.<ref>{{Cite journal|arxiv=1502.01550 |author1=T2K Collaboration | title=Measurements of neutrino oscillation in appearance and disappearance channels by the T2K experiment with 6.6E20 protons on target | journal=Phys. Rev. |volume=D91 | pages=072010 |year=2015 | doi=10.1103/PhysRevD.91.072010 }}</ref><ref name="cpnature">{{cite journal |title=Constraint on the matter–antimatter symmetry-violating phase in neutrino oscillations |journal=Nature |date=15 April 2020 |volume=580 |pages=339–344 |doi=10.1038/s41586-020-2177-0 |url=https://www.nature.com/articles/s41586-020-2177-0 |arxiv=1910.03887}}</ref> The measurement of the neutrino-antineutrino oscillation asymmetry may bring us closer to the explanation of the existence of our [[Baryon asymmetry|matter-dominated]] Universe.<ref>{{cite journal |last1=Fukugita |first1=M. |last2=Yanagida |first2=T. |title=Barygenesis without grand unification |journal=Physics Letters B |date=June 1986 |volume=174 |issue=1 |pages=45–47 |doi=10.1016/0370-2693(86)91126-3|bibcode=1986PhLB..174...45F }}</ref><ref>{{cite journal|last1=Mohapatra |first1=R N|last2=Antusch|first2=S|display-authors=1 |title=Theory of neutrinos: a white paper |journal=Reports on Progress in Physics |date=1 November 2007 |volume=70 |issue=11 |pages=1757–1867 |doi=10.1088/0034-4885/70/11/R02|arxiv=hep-ph/0510213|bibcode=2007RPPh...70.1757M}}</ref> The intense beam of muon neutrinos is produced in the [[J-PARC]] facility (Japan Proton Accelerator Research Complex) in [[Tōkai, Ibaraki|Tokai]] on the east coast of Japan. The beam is directed towards the [[Super-Kamiokande]] far detector located 295&nbsp;km away in the city of [[Hida, Gifu|Hida]], [[Gifu prefecture]]. The properties and composition of the neutrino flux are first measured by a system of near detectors located 280 m 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.<ref name="t2knim">{{Cite journal|author=T2K Collaboration |year=2011 |title=The T2K Experiment |journal=Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment |volume=659 |issue=1 |pages=106–135 |arxiv=1106.1238 |doi=10.1016/j.nima.2011.06.067 |bibcode = 2011NIMPA.659..106A }}</ref> ==Physics program== T2K experiment was proposed in 2003 with the following measurement goals:<ref name="t2knim"/> * The discovery of the {{SubatomicParticle|Muon neutrino}} → {{SubatomicParticle|Electron neutrino}} [[neutrino oscillation|oscillations]], and thus the confirmation that the last unknown mixing angle ''θ''<sub>13</sub> is not zero. * Precise measurement of the oscillation parameters Δ''m''{{su|b=23|p=2}} and ''θ''<sub>23</sub> via muon neutrino disappearance studies. * Search for [[sterile neutrino]] oscillations, which could be observed as a deficit of [[neutral current]] neutrino interactions. * Measurements of various interaction [[Cross section (physics)|cross-sections]] for different types of neutrinos and targets in an energy range of few GeV. Since the start of the data taking in 2010, the T2K experiment succeeded to provide a list of world-class results: * The confirmation of electron neutrino appearance in the muon neutrino beam ({{SubatomicParticle|Muon neutrino}}→{{SubatomicParticle|Electron neutrino}}), which was the first time when neutrinos produced in one flavour was explicitly observed in another flavour.<ref name="1106.2822" /><ref name="1304.0841">{{cite journal |author=T2K Collaboration |title=Evidence of electron neutrino appearance in a muon neutrino beam |journal=Physical Review D |date=5 August 2013 |volume=88 |issue=3 |pages=032002 |doi=10.1103/PhysRevD.88.032002|arxiv=1304.0841|bibcode=2013PhRvD..88c2002A }}</ref> * The most precise measurement of the ''θ''<sub>23</sub> parameter.<ref name="1403.1532" /> * The first significant constraint on the ''δ''<sub>CP</sub> parameter, responsible for the [[CP violation|matter-antimatter asymmetry]] in the neutrino sector.<ref name="cpnature" /> * Limits on a [[sterile neutrino]] oscillation parameters based on studies in the near ND280<ref>{{cite journal |author=T2K Collaboration |title=Search for short baseline nue disappearance with the T2K near detector |journal=Physical Review D |date=16 March 2015 |volume=91 |issue=5 |pages=051102 |doi=10.1103/PhysRevD.91.051102 |arxiv=1410.8811|bibcode=2015PhRvD..91e1102A }}</ref> and far Super-Kamiokande<ref>{{cite journal |author=T2K Collaboration |title=Search for light sterile neutrinos with the T2K far detector Super-Kamiokande at a baseline of 295 km |journal=Physical Review D |date=30 April 2019 |volume=99 |issue=7 |pages=071103 |doi=10.1103/PhysRevD.99.071103 |arxiv=1902.06529|bibcode=2019PhRvD..99g1103A}}</ref> detectors. * Various [[Cross section (physics)|cross-section]] measurements of electron<ref>{{cite arxiv | author=T2K Collaboration |title=Measurement of the charged-current electron (anti-)neutrino inclusive cross-sections at the T2K off-axis near detector ND280 |date=27 February 2020 |class=hep-ex | eprint=2002.11986}}</ref><ref>{{cite journal |author=T2K Collaboration |title=Measurement of the electron neutrino charged-current interaction rate on water with the T2K ND280 pi0 detector |journal=Physical Review D |date=19 June 2015 |volume=91 |issue=11 |pages=112010 |doi=10.1103/PhysRevD.91.112010|bibcode=2015PhRvD..91k2010A |doi-access=free }}</ref> and muon neutrino and antineutrino, including inclusive [[charged current]] (CC) interactions,<ref>{{cite journal | author=T2K Collaboration |title=Measurement of the inclusive numu charged current cross section on carbon in the near detector of the T2K experiment |journal=Physical Review D |date=7 May 2013 |volume=87 |issue=9 |doi=10.1103/PhysRevD.87.092003|arxiv=1302.4908}}</ref> CC interactions without pions<ref>{{cite journal | author=T2K Collaboration |title=Measurement of double-differential muon neutrino charged-current interactions on C8H8 without pions in the final state using the T2K off-axis beam |journal=Physical Review D |date=21 June 2016 |volume=93 |issue=11 |pages=112012 |doi=10.1103/PhysRevD.93.112012|arxiv=1602.03652|bibcode=2016PhRvD..93k2012A }}</ref><ref>{{cite journal |author=T2K Collaboration|title=Measurement of the numu charged-current quasielastic cross section on carbon with the ND280 detector at T2K |journal=Physical Review D |date=11 December 2015 |volume=92 |issue=11 |doi=10.1103/PhysRevD.92.112003|arxiv=1411.6264}}</ref><ref>{{cite arxiv |author=T2K Collaboration |title=First combined measurement of the muon neutrino and antineutrino charged-current cross section without pions in the final state at T2K |date=21 February 2020 |class=hep-ex |eprint=2002.09323}}</ref> and with single pion in the final state,<ref>{{cite journal |author=T2K Collaboration |title=First measurement of the muon neutrino charged current single pion production cross section on water with the T2K near detector |journal=Physical Review D |date=26 January 2017 |volume=95 |issue=1 |pages=012010 |doi=10.1103/PhysRevD.95.012010|arxiv=1605.07964|bibcode=2017PhRvD..95a2010A }}</ref> coherent pion production,<ref>{{cite journal |author=T2K Collaboration |title=Measurement of Coherent pi+ Production in Low Energy Neutrino-Carbon Scattering |journal=Physical Review Letters |date=4 November 2016 |volume=117 |issue=19 |pages=192501 |doi=10.1103/PhysRevLett.117.192501|pmid=27858422 |arxiv=1604.04406|bibcode=2016PhRvL.117s2501A }}</ref> [[neutral current]] interactions,<ref>{{cite journal |author=T2K Collaboration |title=Measurement of the neutrino-oxygen neutral-current interaction cross section by observing nuclear deexcitation gamma rays |journal=Physical Review D |date=31 October 2014 |volume=90 |issue=7 |pages=072012 |doi=10.1103/PhysRevD.90.072012|arxiv=1403.3140|bibcode=2014PhRvD..90g2012A }}</ref> etc. on different targets such as [[carbon]], [[water]] and [[iron]].<ref>{{cite journal |author=T2K Collaboration |title=Measurement of the muon neutrino charged-current cross sections on water, hydrocarbon and iron, and their ratios, with the T2K on-axis detectors |journal=Progress of Theoretical and Experimental Physics |date=September 2019 |volume=2019 |issue=9 |pages=093C02 |doi=10.1093/ptep/ptz070|arxiv=1904.09611 |bibcode=2019PTEP.2019i3C02A }}</ref> Future upgrades of T2K is expected to provide further constrain on the ''δ''<sub>CP</sub> phase by comparing oscillations of neutrinos to those of antineutrinos, as well as more precise measurements of Δ''m''{{su|b=23|p=2}} and ''θ''<sub>23</sub> parameters, and cross-section measurements which will extend our understanding of neutrino interactions and thus improve theoretical models used in neutrino generators.<ref name="upgradeproposal">{{cite arxiv |author=T2K Collaboration |title=Proposal for an Extended Run of T2K to 20E21 POT |date=13 September 2016 |class=hep-ex |eprint=1609.04111}}</ref><ref name="1805.04163">{{cite arxiv |author=Hyper-Kamiokande Collaboration |title=Hyper-Kamiokande Design Report |date=28 November 2018 |class=physics.ins-det |eprint=1805.04163}}</ref> ==Neutrino beam== {{multiple image | align = right | perrow = 2 / 1 | total_width = 415 | image1 = The entire view of J-PARC.jpg | caption1 = Bird's-eye view of the entire facility. | image2 = Superconducting Magnets J-PARC.jpg | caption2 = Superconducting magnets under construction in 2008 to veer the proton beam towards Kamioka. | image3 = Neutrino beam production.svg | caption3 = Neutrino beam production scheme. }} T2K uses a muon neutrino or muon antineutrino [[accelerator neutrino|beam]] produced at the [[J-PARC]] facility using a proton beam gradually accelerated to 30 GeV by a system of three [[particle accelerator|accelerators]]: 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 [[synchrotron]] (Main Ring). [[Proton]]s collide with a [[graphite]] target, producing [[meson]]s, mainly [[pion]]s and [[kaon]]s, which are then focused by a set of three [[magnetic horn]]s 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 {{SubatomicParticle|Muon+}} and {{SubatomicParticle|Muon neutrino}}, forming a muon neutrino beam, while negative pions and kaons decay mainly into {{SubatomicParticle|Muon-}} and {{SubatomicParticle|Muon antineutrino}}, forming a muon antineutrino beam. All remaining [[hadron]]s and charged [[lepton]]s 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.<ref name="t2knim"/> ===Off-axis beam=== T2K is the first experiment in which the concept of off-axis [[accelerator neutrino|neutrino beam]] was realized. The neutrino beam at J-PARC is designed so that it can be directed 2 to 3 [[degree (angle)|degrees]] away from the [[Super-Kamiokande]] 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&nbsp;km is maximal for around 600&nbsp;MeV neutrinos. In this neutrino energy range, the dominant type of neutrino interactions are [[charged current]] 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 with meson production, which are background in the oscillation analysis in the T2K experiment.<ref name="t2knim"/><ref name="t2kflux">{{cite journal |author=T2K Collaboration |title=T2K neutrino flux prediction |journal=Physical Review D |date=2 January 2013 |volume=87 |issue=1 |pages=012001 |doi=10.1103/physrevd.87.012001|arxiv=1211.0469|bibcode=2013PhRvD..87a2001A }}</ref> ==Near detectors== The near detector complex<ref name="t2knim"/> is located at a distance of 280 meters 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: * INGRID detector (Interactive Neutrino GRID) located on the axis of the neutrino beam, * ND280 detector located 2.5° away from the beam axis, i.e. at the same angle as the far detector. * 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 energy.<ref name="babymind">{{cite journal|display-authors=1 |last1=Antonova |first1=M. |last2=Asfandiyarov |first2=R. |title=Baby MIND: A magnetised spectrometer for the WAGASCI experiment |arxiv=1704.08079 |year=2017}}</ref><ref name="wagasci">{{cite journal|display-authors=1 |last1=Ovsiannikova |first1=T |last2=Antonova |first2=M |title=The new experiment WAGASCI for water to hydrocarbon neutrino cross section measurement using the J-PARC beam |journal=Journal of Physics: Conference Series |date=5 February 2016 |volume=675 |issue=1 |pages=012030 |doi=10.1088/1742-6596/675/1/012030|doi-access=free }}</ref> ===Signal readout=== [[File:Scintillator.svg|300px|thumb|Principle of operation of a scintillator in the T2K near detectors.]] Except for the [[Time Projection Chamber]]s in ND280, the entire active material (enabling particle tracking) of the near detectors is [[plastic]] [[scintillator]]. The light produced by traversing particles in the plastic scintillator bars and planes is collected by [[wavelength shifter|wavelength-shifting]] [[optical fiber|fibres]] and detected by Hamamatsu [[Silicon photomultiplier|Multi-pixel photon counters]] 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 traversing particles.<ref name="t2knim"/> ===INGRID detector=== 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 modules outside the cross. Height and width of the arms are 10 meters. 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. Veto is a part of a detector where no activity should be registered to accept an event. Such requirement allows to constrain amount of background events in a selected sample; here the background from particles produced outside of the detector. 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.<ref name="t2knim"/> ===ND280 detector=== {{multiple image | align = right | total_width = 400 | image1 = J-PARC T2K ND280 Pit.jpg | caption1 = ND280 under construction. | image2 = ND280 detector scheme.png | caption2 = Exploded view of the ND280 detector. }} 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 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.<ref name="t2knim"/> 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 [[UA1 experiment]] producing 0.2 T uniform horizontal field and instrumented with scintillator planes constituting the Side Muon Range Detector.<ref name="t2knim"/> ====Pi-Zero detector==== [[File:Nd280 p0d layers structure.png|180px|thumb|Pi-Zero detector scheme.]] The Pi-Zero ({{SubatomicParticle|Pion0}}) Detector (P0D) contains 40 plastic scintillator module planes, which in the central part are interleaved with 2.8&nbsp;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. The main goal of the Pi-Zero Detector is measurement neutral [[pion]]s production in [[neutral current]] neutrino interactions on water: : {{SubatomicParticle|Muon neutrino}} + N → {{SubatomicParticle|Muon neutrino}} + N’ + {{SubatomicParticle|Pion0}} This reaction can mimic electron neutrino interactions because photons from {{SubatomicParticle|Pion0}} 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.<ref name="t2knim"/><ref>{{cite journal |first1=S|last1=Assylbekov|first2=B E|last2=Berger|display-authors=1 |title=The T2K ND280 off-axis pi–zero detector |journal=Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment |date=September 2012 |volume=686 |pages=48–63 |doi=10.1016/j.nima.2012.05.028|arxiv=1111.5030|bibcode=2012NIMPA.686...48A}}</ref> ====Time projection chambers==== Three [[time projection chamber]]s (TPCs) are gas-tight rectangular boxes, with a cathode plane in the centre and readout [[MicroMegas detector|MicroMegas]] modules at both sides parallel to the cathode. TPCs are filled with [[argon]]-based drift gas under atmospheric pressure. Charged particles crossing TPC [[ionisation|ionise]] 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 MicroMegas modules, and X coordinate is based on the electrons drift time. In the magnetic field, the curvature of this path allows to determine [[electric charge|charge]] and [[momentum]] of the particle, and the amount of the ionisation electrons per unit distance is used to identify particles based on the [[Bethe formula|Bethe-Bloch formula]].<ref name="t2knim"/><ref>{{cite journal |author=T2K ND280 TPC collaboration |title=Time projection chambers for the T2K near detectors |journal=Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment |date=May 2011 |volume=637 |issue=1 |pages=25–46 |doi=10.1016/j.nima.2011.02.036|arxiv=1012.0865|bibcode=2011NIMPA.637...25A }}</ref> ====Fine-grained detectors==== 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 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 detector at Super-Kamiokande is water-based. Cross sections on carbon and on the water can be determined from a comparison of neutrino interactions in the two FGDs.<ref name="t2knim"/><ref>{{cite journal |author=T2K ND280 FGD Collaboration |title=The T2K fine-grained detectors |journal=Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment |date=December 2012 |volume=696 |pages=1–31 |doi=10.1016/j.nima.2012.08.020 |arxiv=1204.3666|bibcode=2012NIMPA.696....1A }}</ref> ====Electromagnetic Calorimeter==== 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 providing additional information relevant for their identification.<ref name="t2knim"/><ref>{{cite journal |author=T2K UK Collaboration |title=The electromagnetic calorimeter for the T2K near detector ND280 |journal=Journal of Instrumentation |date=17 October 2013 |volume=8 |issue=10 |pages=P10019 |doi=10.1088/1748-0221/8/10/P10019 |arxiv=1308.3445|bibcode=2013JInst...8P0019A }}</ref> ====Side Muon Range Detector==== 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 stopped in the calorimeter. SMRD can also act as a [[trigger (particle physics)|trigger]] for [[cosmic rays]]. Finally, it can help identify beam interactions in the surrounding walls and in the magnet itself.<ref name="t2knim"/><ref>{{cite journal |first1=S|last1=Aoki|first2=G|last2=Barr|display-authors=1|title=The T2K Side Muon Range Detector (SMRD) |journal=Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment |date=January 2013 |volume=698 |pages=135–146 |doi=10.1016/j.nima.2012.10.001|arxiv=1206.3553|bibcode=2013NIMPA.698..135A}}</ref> ===WAGASCI-Baby MIND=== [[File:Wagasci and ND280 neutrino flux.png|200px|thumb|right|The predicted T2K neutrino flux at the site of the WAGASCI-Baby MIND (red line) and of the ND280 (black line) detectors.]] WAGASCI-Baby MIND is a new detector located next to the INGRID and ND280 detectors, devoted to [[neutrino]] interaction studies. It provided the first neutrino beam data using a full detector setup during the 2019/2020 winter run.<ref name="babymind"/><ref name="wagasci"/> The WAGASCI-Baby MIND consists of several sub-detectors: * Two new [[water]]-[[scintillator]] 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. Thanks to such a structure, a high water to scintillator mass ratio was obtained (80% H<sub>2</sub>O + 20% CH) and the acceptance is high and approximately constant in all directions.<ref name="babymind"/><ref name="wagasci"/> * One Proton Module, the same as in the [[T2K experiment#INGRID detector|INGRID]] detector, made of plain [[plastic]] [[scintillator]] (CH) bars, that acts as the main CH target and particle tracker.<ref name="babymind"/><ref name="wagasci"/> * Two WallMRD (Wall Muon Range Detector) that are non-magnetized muon spectrometers to detect side going muons. They are made of passive [[iron]] planes intertwined with active scintillator planes.<ref name="babymind"/><ref name="wagasci"/> * One Baby MIND (prototype Magnetized Iron Neutrino Detector) that is a magnetized muon spectrometer to detect forward-going muons. Baby MIND sports an original configuration of scintillation modules intertwined with magnetized [[ferrite (iron)|ferrite]] 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 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.<ref name="babymind"/> All the active material in the detectors is made up of plastic scintillator and is read as explained in section [[T2K experiment#Signal readout|Signal readout]].<ref name="babymind"/><ref name="wagasci"/> The main goal of the WAGASCI-Baby MIND detector is a reduction of the systematic error in the T2K [[neutrino oscillation|oscillation]] analysis, which will be achieved thanks to its complementarity with respect to the ND280 detector: * Different target material between ND280 (80% CH + 20% H<sub>2</sub>O) and SK (pure H<sub>2</sub>O) forces us to rely on cross-section models to disentangle the H<sub>2</sub>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<sub>2</sub>O) and plastic (CH) with 3% accuracy.<ref name="babymind"/><ref name="wagasci"/> * 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 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.<ref name="babymind"/><ref name="wagasci"/> * 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 detectors. [[linear combination|Combination]] of measurements from these detectors will provide an improved constraint on the neutrino cross-sections as a function of their energy.<ref name="babymind"/><ref name="wagasci"/> ==Super-Kamiokande== {{main|Super-Kamiokande}} [[File:Superkamiokande electron muon discriminator.png|thumb|Detection of [[electron]]s and [[muon]]s in the [[Super-Kamiokande]] detector.]] 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 [[stainless steel]] [[cylinder|cylindrical]] tank of about 40 m height and diameter, filled with 50,000 tons of [[water]] and instrumented with around 13,000 [[photomultiplier tube]]s (PMT). It detects a [[cone]] of [[Cherenkov radiation|Cherenkov light]] emitted by charged particles moving in water faster than light in this medium. Its goal is to measure [[muon]]s and [[electron]]s produced in [[charged current]] quasielastic interactions (CCQE) of {{SubatomicParticle|Muon neutrino}} and {{SubatomicParticle|Electron neutrino}}, 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 [[particle shower|showers]], observed by PMTs as a ring with fuzzy edges. Neutrino energy is calculated based on the direction and energy of a charged [[lepton]] produced in the CCQE interaction. In this way, {{SubatomicParticle|Muon neutrino}} and {{SubatomicParticle|Electron neutrino}} spectra are determined, leading to the measurement of the [[neutrino oscillation|oscillation]] parameters relevant for muon neutrino disappearance and electron neutrino appearance.<ref name="t2knim"/><ref>{{cite journal |author=The Super-Kamiokande Collaboration |title=The Super-Kamiokande detector |journal=Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment |date=April 2003 |volume=501 |issue=2–3 |pages=418–462 |doi=10.1016/S0168-9002(03)00425-X|bibcode=2003NIMPA.501..418F }}</ref> ==History== T2K is a successor of the KEK to Kamioka ([[K2K experiment|K2K]]) experiment, which ran from 1999 till 2004. In the [[K2K experiment]], an [[accelerator neutrino|accelerator beam]] of muon neutrinos was produced at [[KEK]] facility in [[Tsukuba, Ibaraki|Tsukuba]] ([[Japan]]) and sent towards the [[Super-Kamiokande]] detector, located 250&nbsp;km away. The K2K experiment results confirmed at the confidence level of 99.9985% (4.3 [[Standard deviation|σ]]) the [[neutrino oscillation|disappearance]] of the [[muon neutrino]]s and were consistent with the previous measurements of oscillation parameters measured by the Super-Kamiokande detector for [[Neutrino#Atmospheric|atmospheric neutrino]]s.<ref>{{cite book |last1=Oyama |first1=Yuichi |title=Nuclear Science and Safety in Europe |chapter=Results from K2K and status of T2K |series=NATO Security through Science Series |year=2006 |pages=113–124 |doi=10.1007/978-1-4020-4965-1_9 |arxiv=hep-ex/0512041|isbn=978-1-4020-4963-7 }}</ref><ref>{{cite journal |author=K2K Collaboration |title=Measurement of neutrino oscillation by the K2K experiment |journal=Physical Review D |date=12 October 2006 |volume=74 |issue=7 |pages=072003 |doi=10.1103/PhysRevD.74.072003|arxiv=hep-ex/0606032|bibcode=2006PhRvD..74g2003A }}</ref> 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 installed in the fall of 2010. T2K far detector is the large Super-Kamiokande detector, which has been running since 1996 and studying [[proton lifetime]] and oscillations of [[Neutrino#Atmospheric|atmospheric]], [[solar neutrino|solar]] and [[accelerator neutrino|accelerator]] neutrinos.<ref name="t2knim"/> 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 [[Great Tohoku Earthquake]] in March 2011. The proton beam power, and thus the neutrino beam intensity, was constantly growing, reaching by February 2020 the power of 515&nbsp;kW and a total number of accumulated protons on target of 3.64×10<sup>21</sup> protons<ref>{{cite web |title=T2K experiment official page - T2K Run 10 |url=https://t2k-experiment.org/2020/02/t2k-run-10-ended-with-record-beam-power/}}</ref> with 55% of data in neutrino-mode and 45% in antineutrino-mode. In April 2020, T2K collaboration published results strongly constraining the ''δ''<sub>CP</sub> phase. The results reject at 95% confidence the hypothesis of no CP violation (including the possibility of ''δ''<sub>CP</sub> equal to ''π'').<ref name="cpnature"/><ref>{{cite news |last1=Cho |first1=Adrian |title=Skewed neutrino behavior could help explain matter’s dominion over antimatter |url=https://www.sciencemag.org/news/2020/04/skewed-neutrino-behavior-could-help-explain-matter-s-dominion-over-antimatter |access-date=19 April 2020 |work=Science {{!}} AAAS |date=15 April 2020 |language=en}}</ref> The results also reject at the 3σ (99.7%) significance level almost half of the possible values of this parameter and give a strong hint that CP violation may be large in the neutrino sector.<ref name="cpnature"/><ref>{{cite web |url=https://www.bbc.com/news/science-environment-52297058 |title=Biggest cosmic mystery 'step closer' to solution |last=Rincon |first=Paul |date=16 April 2020 |website=BBC News website}}</ref> ==Future plans== The T2K experiment operated in the current form until 2020. In 2021 the first data run with Gadollinium loaded into the Super-Kamiokande far detector was taken.<ref name="panik2021">{{cite web |last1=Vilela |first1=Cristovao |title=The status of T2K and Hyper-Kamiokande experiments |url=https://indico.lip.pt/event/592/contributions/3550/ |website=PANIC 2021 Conference |date=September 5-10, 2021}}</ref>{{rp|12}} 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).<ref name="lomonosov2021">{{cite web |last1=Kudenko |first1=Yury |title=Physics and status of SuperFGDdetector for T2K experiment |url=https://lomcon.ru/files/20LomCon/presentations/Presenteations/19/lomonosov2021_kudenko.pdf |website=The 20th Lomonosov Conference on Elementary Particle Physics |date=August 19-25, 2021 |page=17-18}}</ref><ref name="upgradeproposal"/> In 2027, the successor of the T2K experiment will be launched, the Hyper-Kamiokande (HK) experiment, with the new, 250,000-ton water [[Cherenkov radiation|Cherenkov]] far detector - the [[Hyper-Kamiokande]] detector.<ref name="panik2021"/>{{rp|20}}<ref>{{cite journal |author=Hyper-Kamiokande Proto-Collaboraion |title=Physics Potential of a Long Baseline Neutrino Oscillation Experiment Using J-PARC Neutrino Beam and Hyper-Kamiokande |journal=Progress of Theoretical and Experimental Physics |date=19 May 2015 |volume=2015 |issue=5 |pages=53C02–0 |doi=10.1093/ptep/ptv061 |arxiv=1502.05199 |bibcode=2015PTEP.2015e3C02A |issn=2050-3911}}</ref><ref name="hyperk">{{cite arxiv |author=Hyper-Kamiokande Proto-Collaboration |title=Hyper-Kamiokande Design Report |date=28 November 2018 |class=physics.ins-det |eprint=1805.04163}}</ref> The building of an additional Intermediate Water Cherenkov detector at a distance of around 2&nbsp;km is also considered for the HK experiment.<ref name="hyperk"/> ===T2K-II=== The 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 [[neutrino oscillation|oscillation]] parameters ''θ''<sub>23</sub> and Δ''m''{{su|b=23|p=2}} with a precision of 1.7° and 1%, respectively, as well as a confirmation at the level of 3 [[Standard deviation|σ]] or more of the matter-antimatter asymmetry in the neutrino sector in a wide range of possible true values of ''δ''<sub>CP</sub> - the parameter responsible for the [[CP violation|CP]] (matter-antimatter) asymmetry. Achievement of these goals requires reduction of the statistical and systematic errors, and thus a significant upgrade of the beamline and the ND280 detector, as well as improvements in the software and analysis methods.<ref name="upgradeproposal"/> ====Beam upgrade==== The beam upgrade plan requires one year long shut down of the [[J-PARC]] Main Ring [[particle accelerator|accelerator]] in 2021, followed by a constant gradual increase of the [[proton]] [[particle beam|beam]] power until the start of the HK experiment. The beam power should reach 750&nbsp;kW in 2022 and then grow to 1.3 MW by 2029.<ref name="beamupgradetdr">{{cite arxiv |author=T2K Collaboration and J-PARC Neutrino Facility Group |title=J-PARC Neutrino Beamline Upgrade Technical Design Report |date=14 August 2019 |class=physics.ins-det |eprint=1908.05141}}</ref> In February 2020, the proton beam power reached 515&nbsp;kW with 2.7x10<sup>14</sup> protons per pulse and with 2.48 seconds between pulses (so-called repetition cycle). To reach 750&nbsp;kW, the repetition cycle will be reduced to 1.32 s with 2.0x10<sup>14</sup> protons per pulse, while for 1.3 MW the repetition cycle has to be further decreased to 1.16 s and the number of protons per pulse has to increase to 3.2x10<sup>14</sup>. In addition to increasing the primary proton beam power, the current in the [[magnetic horn|horns]] focusing secondary particles ([[pion]]s, [[kaon]]s, etc.) with a chosen [[electric charge]] 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 the anti-neutrino mode beam) by around 5-10%.<ref name="beamupgradetdr"/><ref name="beamupgradeprogramme">{{cite journal |last1=Friend |first1=M |title=J-PARC accelerator and neutrino beamline upgrade programme |journal=Journal of Physics: Conference Series |date=September 2017 |volume=888 |issue=1 |pages=012042 |doi=10.1088/1742-6596/888/1/012042 |bibcode=2017JPhCS.888a2042F |language=en |issn=1742-6588|doi-access=free }}</ref> Reduction of the repetition cycle will require a series of hardware upgrades, including a major upgrade of the Main Ring [[power supply|power supplies]] 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 [[cooling]] capacity of the secondary beamline components such as the [[graphite]] target, the magnetic horns and the beam dump, as well as disposal of a larger amount of irradiated cooling water.<ref name="beamupgradetdr"/><ref name="beamupgradeprogramme"/> ====ND280 Upgrade==== [[File:Nd280upgrade scheme.png|thumb|Scheme of the inner part of the ND280 detector after planned upgrade.]] The current design of the ND280 detector is optimized for the detection and reconstruction of forward-going [[lepton]]s ([[muon]]s and [[electron]]s), but it also has a number of limitations, like low reconstruction efficiency of particles produced almost perpendicular and backward w.r.t. the direction of the interacting [[neutrino]], 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 ([[pion]]s, [[kaon]]s, [[nucleon]]s) were lost, may be mis-reconstructed as CCQE and introduce a [[Bias (statistics)|bias]] in the reconstructed neutrino energy spectrum. Thus, it is essential to optimize the detector to be sensitive to additional particles and [[Nuclear structure|nuclear effects]]. Three main measures need to be taken to address these issues: * The detector needs to efficiently detect the nucleons in the final state of neutrino interactions. For this, the detection thresholds need to be lowered. * 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 information. * 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 interactions. 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 maintain their sandwiched structure and continue to detect forward going leptons and high momentum hardons. 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.<ref name="nd280upgradetdr">{{cite arxiv |author=T2K Collaboration|title=T2K ND280 Upgrade - Technical Design Report |date=11 January 2019 |class=physics.ins-det |eprint=1901.03750}}</ref> The installation of the new sub-detectors into ND280 will be done in 2022.<ref name="lomonosov2021"/><ref name="nd280upgradetdradd">{{cite journal |author=The T2K ND280 Upgrade Working Group|title=NP07: ND280 Upgrade project |date=June 19, 2020 |url=http://cds.cern.ch/record/2713578 |journal=CERN Scientific Committee Paper |volume=CERN-SPSC-2020-008. SPSC-SR-267}}</ref>{{rp|18}} =====SuperFGD===== The SuperFGD is a 2m x 2m x 0.5m detector consisting of approximately 2 million 1&nbsp;cm<sup>3</sup> [[scintillator|scintillating]] [[polystyrene]] [[cube]]s. The cubes are woven with a series of [[optical fiber|optical fibres]] 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 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 [[antineutrino]] energy.<ref name="nd280upgradetdr"/> =====HATPC===== The High Angle [[Time Projection Chamber]]s (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 [[MicroMegas detector|MicroMegas]] 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 [[Electrical resistance and conductance|resistive]] 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.<ref name="nd280upgradetdr"/> =====TOF===== The six Time-of-Flight (TOF) detectors surrounding the HATPCs and SuperFGD are a series of [[plastic]] [[scintillator]] layers designed to identify the particle direction sense through the measurement of the [[time of flight]] for each crossing track with a timing resolution of the order of 600 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.<ref name="nd280upgradetdr"/> =====Impact on Neutrino Oscillation Physics===== 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 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.<ref name="nd280upgradetdr"/> ===Hyper-Kamiokande experiment=== {{main|Hyper-Kamiokande}} The successor of the T2K experiment, the [[Hyper-Kamiokande]] (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 Hyper-Kamiokande detector, and possibly also a new intermediate detector 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.<ref name="panik2021"/>{{rp|20}}<ref name="hyperk"/><ref name="hyperkstart">{{cite news|url=http://www.j-parc.jp/c/en/topics/2020/02/12000416.html|title=The Hyper-Kamiokande project is officially approved.|date=12 February 2020}}</ref><ref>{{cite journal |author=Hyper-Kamiokande Proto-Collaboraion |title=Physics potential of a long-baseline neutrino oscillation experiment using a J-PARC neutrino beam and Hyper-Kamiokande |journal=Progress of Theoretical and Experimental Physics |date=19 May 2015 |volume=2015 |issue=5 |pages=53C02–0 |doi=10.1093/ptep/ptv061 |arxiv=1502.05199|bibcode=2015PTEP.2015e3C02A }}</ref> ====Hyper-Kamiokande detector==== The Hyper-Kamiokande detector will be a [[water]] [[Cherenkov radiation|Cherenkov]] detector, 5 times larger (258 kton of water) than the [[Super-Kamiokande]] detector. It will be a [[cylinder]] of 74 meters diameter and 60 meter height with 40000 [[photomultiplier]] tubes of 50&nbsp;cm diameter and 6700 photomultiplier tubes of 20&nbsp;cm diameter. It will be located 8&nbsp;km south from the Super-Kamiokande detector in the Tochibora mine, 650 meters under the peak of Nijuugo mountain, at the same off-axis angle (2.5°) to the neutrino beam centre and in the same distance (295&nbsp;km) from the beam production place at [[J-PARC]]. The HK detector construction began in 2020 and the start of data collection is expected in 2027.<ref name="panik2021"/>{{rp|24}}<ref name="hyperk"/><ref name="hyperkstart"/> ====Intermediate Water Cherenkov==== The Intermediate Water Cherenkov Detector (IWCD) will be located at a distance of 0.7–2&nbsp;km from the neutrino production place. It would be a cylinder filled with water of 10 m diameter and 50 m height with a 10 m tall structure instrumented with around 3000 photomultiplier tubes of a 20&nbsp;cm diameter. The structure will be moved in a vertical direction by a crane system, providing measurements of neutrino interactions at different off-axis angles, spanning from 1° to 4°, and thus for different energy spectra. Combining the results from different off-axis angles it is possible to extract the results for nearly monochromatic neutrino spectrum without relying on theoretical models of neutrino interactions to reconstruct neutrino energy. Usage of the same type of detector as the far detector with almost the same angular and momentum acceptance allows comparing results from these two detectors without relying on detectors response simulations. These two facts, independence from the neutrino interaction and detector response models, will enable to minimise systematic error in the oscillation analysis. Additional advantages of such a design of the detector is a possibility to search for [[sterile neutrino|sterile]] [[neutrino oscillation|oscillation]] pattern for different off-axis angles and to obtain a cleaner sample of [[electron neutrino]] interaction, whose fraction is larger for the larger off-axis angle.<ref name="hyperk"/>{{rp|47–50}}<ref>{{cite arxiv |author=nuPRISM Collaboration |title=Letter of Intent to Construct a nuPRISM Detector in the J-PARC Neutrino Beamline |date=13 December 2014 |class=physics.ins-det |eprint=1412.3086}}</ref><ref>{{cite web |author=nuPRISM Collaboration |title=Proposal for the NuPRISM Experiment in the J-PARC Neutrino Beamline |url=https://j-parc.jp/researcher/Hadron/en/pac_1607/pdf/P61_2016-17.pdf |date=7 July 2016}}</ref> It is planned that the IWCD will be finalised in 2024 and will start to take data from 2025, yet before launching the HK experiment.<ref>{{cite web |last1=Yoshida |first1=Tomoyo |title=J-PARC E61 experiment |url=https://indico.cern.ch/event/531125/contributions/2858586/attachments/1604730/2545546/4_J-PARC_E61_experiment.pdf |publisher=Lake Louise Winter Institute |date=21 February 2018}}</ref> ==See also== * [[Kamioka Observatory]] ==Notes== {{reflist}} ==External links== {{Commons|T2K}} * [http://www.t2k-experiment.org/ T2K Experiment Official Website] * [http://www-sk.icrr.u-tokyo.ac.jp/sk/index-e.html Super-Kamiokande Official Website] * [http://www-sk.icrr.u-tokyo.ac.jp/realtimemonitor/ Super-Kamiokande Realtime Monitor] * [https://www.youtube.com/watch?v=tBrFrdSneZg Neutrino physics - The T2K experiment - YouTube] * [https://www.youtube.com/watch?v=cs02i8TIphs Inside Japan's Big Physics | Part one: Super Kamiokande - YouTube] {{Breakthrough Prize laureates}} {{Neutrino detectors}} [[Category:Accelerator neutrino experiments]] [[Category:Science and technology in Japan]] [[Category:CERN experiments]] [[Category:Fixed-target experiments]]'
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'@@ -55,5 +55,5 @@ ===INGRID detector=== -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 modules outside the cross. Height and width of the arms are 10 meters. 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.<ref name="t2knim"/> +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 modules outside the cross. Height and width of the arms are 10 meters. 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. Veto is a part of a detector where no activity should be registered to accept an event. Such requirement allows to constrain amount of background events in a selected sample; here the background from particles produced outside of the detector. 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.<ref name="t2knim"/> ===ND280 detector=== '
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[ 0 => '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 modules outside the cross. Height and width of the arms are 10 meters. 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. Veto is a part of a detector where no activity should be registered to accept an event. Such requirement allows to constrain amount of background events in a selected sample; here the background from particles produced outside of the detector. 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.<ref name="t2knim"/>' ]
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[ 0 => '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 modules outside the cross. Height and width of the arms are 10 meters. 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.<ref name="t2knim"/>' ]
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