status of the nova experiment - osaka university · 2016-11-09 · beam performance dbd16 -osaka,...
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StatusoftheNOvAExperimentERIKACATAÑO-MUR (������� �� )
IOWA STATEUN IVERS ITY
FORTHENOVA COLLABORATION
DBD16 , NOVEMBER 9 , 2 016
NOvAoverview
2DBD16- OSAKA,JAPAN
§ NOvA isalong-baselineneutrinooscillationexperiment
§ StudyneutrinosfromNuMI beamatFermilab
§ 14mrad offthebeamaxis§ Twofunctionallyidenticalliquidscintillatordetectors:
§ FarDetector(FD)14kton;onthesurface
§ NearDetector(ND)0.3kton;undergroundMN WI
IL
MI
Near Detector
Far Detector
DBD16- OSAKA,JAPAN E.CATANO-MUR [ISU]– STATUSOFTHENOVAEXPERIMENT 3
20m
70m
Amonumentalexperiment…
ToweroftheSun
DBD16- OSAKA,JAPAN E.CATANO-MUR [ISU]– STATUSOFTHENOVAEXPERIMENT 4
NOvA FD
(rotated)
NOvA ND
(rotated)
NOvA
collaborator
60m
15.6m
Amonumentalexperiment…
810km
NOvA’s physicsprogramOscillationchannels
!" → !$ !" → !$ “appearance”!" → !" !" → !" “disappearance”
DBD16- OSAKA,JAPAN E.CATANO-MUR [ISU]– STATUSOFTHENOVAEXPERIMENT 5
§ Neutrino masshierarchy?§ %&' octant?§ Allowedrangeof()*?§ Precisionmeasurementsofsin. 2%&'
andΔ1'&& Otheranalyses:
§ Sterileneutrinos§ Crosssections§ Supernovae,
monopoles,etc.
§ 2015!$ analysisresults:PRL.116.151806§ 2015!" analysisresults:Phys.Rev.D93.051104§ 2016results:tobepublished
NuMI muonneutrinobeam
§ NuMI: neutrinosfromtheMainInjector
§ PartofFermilab’s acceleratorcomplex
DBD16- OSAKA,JAPAN 6
Maininjector(MI)
LinacBooster
NuMI
Neutrino
Beam
§ Linac: H- ions,400MeV
§ Booster:
protons,8GeV§ MainInjector:
protons,120GeV
§ TheseprotonsareusedtomaketheNuMI
beam
NuMI target
NuMI off-axis
DBD16- OSAKA,JAPAN E.CATANO-MUR [ISU]– STATUSOFTHENOVAEXPERIMENT 7
§ MIprotonbeamissteeredontoanarrowgraphitetarget approx.1minlength
§ Producedhadronsarefocusedinandcharge-sign-selectedbytwomagnetichorns
§ 675mdecaypipe§ Predominantlypions andkaons,decaymodes34 → 54 + !" ,74 → 54 + !" ⟹ 9: beam
§ Smallcontamination:!$ , !
[GeV]νE0 5 10 15
CC
/ 6E2
0 PO
T / k
ton
/ 0.1
GeV
µν 0
5
10
15
On-Axis
7 mrad Off-Axis
A)ν14.6 mrad Off-Axis (NO
21 mrad Off-Axis
FLUKA11
A SimulationνNO
At14.6mrad off-axis,NOvA observesanarrowbandbeampeakedat2GeV§ Optimalfor!" → !$
BeamPerformance
DBD16- OSAKA,JAPAN E.CATANO-MUR [ISU]– STATUSOFTHENOVAEXPERIMENT 8
§ Accumulatedexposure:6.05x1020 POTin14kton equivalentdetector§ Morethandoubleexposureof2015analysis§ ByJuly2016:runningat560kW(before3monthshutdown)§ Achieved700kWdesigngoalintestsonJune13!§ HighintensitybeamreturnsthisFriday
07/02/14 12/31/14 07/02/15 01/01/16 07/01/16
Bea
m P
ower
per
cal
enda
r hou
r (kW
)
0
100
200
300
400
500
600
700
Tota
l Pro
tons
(E20
)
0
2
4
6
8
10
12
14
DetectorCommissioning(ReducedMass)
FirstAnalysis2.74x1020 POT-equiv.
TotalExposure6.05x1020 POT-equiv.
POT=ProtonsOnTarget
NOvADetectors
DBD16- OSAKA,JAPAN 9
§ PVC+LiquidScintillator§ MineralOil§ 5%pseudocumene
§ ReadoutviawavelengthshiftingfibertoAPD
§ Layeredplanesoforthogonalviews
§ ND:214layers,18000channels§ FD:896layers,344000channels
Findingneutrinoevents
DBD16- OSAKA,JAPAN 10 E.CATANO-MUR [ISU]– STATUSOFTHENOVAEXPERIMENT
§ Detectorsarefine-grained,low-Z,highly-activetrackingcalorimeters
§ Orthogonallayersà topandsideviewsforeachevent
§ Timeanddirectionhelptoidentifybeamevents
Findingneutrinoevents
Slicing:Coarseevent-leveltime-spaceclustering
Allhitsrecordedin550μsec(beam:~10μsec)
Selectedslicewithbeamcandidate
Vertexing:Findlinesofenergydepositions(CCevents:11cmresolution)
Clustering:Findclustersinangularspacearoundvertex.MergeviewsviatopologyandprongdE/dx
Tracking:Traceparticletrajectories
DBD16- OSAKA,JAPAN 11E.CATANO-MUR [ISU]– STATUSOFTHENOVAEXPERIMENT
q (ADC)10 102 310
q (ADC)10 102 310
q (ADC)10 102 310
νμ
eνe
p
μ
p
1m
1m
ν
νµ CC
νe CC
NC
Long,straighttrack
Shorter,wider,fuzzyshower
Hadronicactivityfromnuclearrecoilsystem
Eventtopologies
DBD16- OSAKA,JAPAN E.CATANO-MUR [ISU]– STATUSOFTHENOVAEXPERIMENT 12
CC=chargedcurrent;NC=neutralcurrent
Eventselection(particleID)
DBD16- OSAKA,JAPAN E.CATANO-MUR [ISU]– STATUSOFTHENOVAEXPERIMENT 13
§ !" selection:kNN basedonmuon tracklength,scattering,planefraction,dE/dx.RemovesmostNCbackgroundevents
§ !$ selection:featuresanewtechniquebasedonideasfromcomputervisionanddeeplearning
o “ConvolutionalVisualNetwork”(CVN)
o Input:Calibratedhitmapso Imageprocessing
transformationsà abstractfeatures
o Networkdecidesimportantfeatures+correlations
o Output: eventclassifier
A. Aurisano etal.,2016JINST11P09001
FEATURE MAPS
::
FEATURE MAPS
::
Muonneutrinodisappearance
1. Identifycontained!" CCeventsineachdetector
2. MeasureNearandFarenergyspectra
3. Extractoscillationinformationfromdifferencesbetweenbothenergyspectra
DBD16- OSAKA,JAPAN 14
(simulated!5 CCevent)Ehad
Ltrack
!5 selectedeventsintheND
DBD16- OSAKA,JAPAN E.CATANO-MUR [ISU]– STATUSOFTHENOVAEXPERIMENT 15
§ Reconstructed!5 energyisE! =E5 +Ehad
Hadronic energy (GeV)0 0.5 1 1.5 2 2.5 3
Eve
nts
310
0
100
200
300 Simulated selected eventsSimulated backgroundData
syst. rangeσShape-only 1- POT20 10×ND area norm., 3.72
NOvA Preliminary
Reconstructed muon energy (GeV)0 1 2 3 4 5
Eve
nts
310
0
20
40
60
80
100 Simulated selected eventsSimulated backgroundData
syst. rangeσShape-only 1- POT20 10×ND area norm., 3.72
NOvA Preliminary
Reconstructed neutrino energy (GeV)0 1 2 3 4 5
Eve
nts
310
0
100
200
300 Simulated selected eventsSimulated backgroundData
syst. rangeσShape-only 1- POT20 10×ND area norm., 3.72
NOvA Preliminary
§ UseNDdatatoimprovetheFDprediction:Unfoldthereconstructedneutrinoenergy+usethetrueFar/Nearratiofromthesimulation
Hadronic systemEvisible� Ehad
Reconstructedmuon tracklength� E5
!5 selectedeventsintheFD
DBD16- OSAKA,JAPAN E.CATANO-MUR [ISU]– STATUSOFTHENOVAEXPERIMENT 16
§ PredictionusingNDdata:473±30withnooscillation
§ 78eventsobservedinFD
Reconstructed neutrino energy (GeV)0 1 2 3 4 5
Ratio
with
uno
sc. (
bkg
subt
ract
ed)
0
0.5
1
1.5 POT-equiv.2010×NOvA 6.05
Data
Best fit prediction
NOvA Preliminary
Reconstructed neutrino energy (GeV)0 1 2 3 4 5
Even
ts /
0.25
GeV
0
20
40
60
80
100
120 POT-equiv.2010×A 6.05νNO
Best fit prediction
Unoscillated prediction
Data
NOvA Preliminary
§ 82eventsatbestoscillationfit§ 3.7beambkgd.+2.9cosmic
Disappearanceresults
DBD16- OSAKA,JAPAN E.CATANO-MUR [ISU]– STATUSOFTHENOVAEXPERIMENT 17
BestFit(inNH):
23θ2sin0.3 0.4 0.5 0.6 0.7
)2 e
V-3
(10
322m
∆
2
2.5
3
3.5
NOvA Preliminary
Normal Hierarchy POT-equiv.2010×NOvA 6.05
90% C.L. NOvA 2016
90% C.L. NOvA 2015
���m232
�� = 2.67± 0.12⇥ 10�3eV2
sin2 ✓23 = 0.40+0.03�0.02(0.63
+0.02�0.03)
Comparedto lastyearNOvA’s results
NoFeldman-CousinsCorrection
§ FitforΔm2 andsin2θ23§ Using2DGaussianC.L.(FCcorrected:tobepublished)
§ Maximalmixingexcludedat2.5σ
§ Dominantsystematiceffectsincludedinfit:§ Normalization§ NCbackground§ Flux§ Muon andhadronicenergyscales§ Crosssection§ Detectorresponseandnoise
Loweroctant Upperoctant
23θ2sin0.3 0.4 0.5 0.6 0.7
)2 e
V-3
(10
322m
∆
2
2.5
3
3.5
NOvA PreliminaryNormal Hierarchy, 90% CL
NOvA 2016
T2K 2014MINOS 2014
Disappearanceresults
DBD16- OSAKA,JAPAN E.CATANO-MUR [ISU]– STATUSOFTHENOVAEXPERIMENT 18
BestFit(inNH):���m232
�� = 2.67± 0.12⇥ 10�3eV2
sin2 ✓23 = 0.40+0.03�0.02(0.63
+0.02�0.03)
Comparedtootherexperiments
NoFeldman-CousinsCorrection
§ FitforΔm2 andsin2θ23§ Using2DGaussianC.L.(FCcorrected:tobepublished)
§ Maximalmixingexcludedat2.5σ
§ Dominantsystematiceffectsincludedinfit:§ Normalization§ NCbackground§ Flux§ Muon andhadronicenergyscales§ Crosssection§ Detectorresponseandnoise
Electronneutrinoappearance
DBD16- OSAKA,JAPAN 19
1. Identifycontained!$ (!")CCcandidatesineachdetector.
2. Usedatatoimprovethepredictionfromthesimulation:
• ND!" candidatesà !$ signalintheFD• ND!$ candidatesà FDbeambackgrounds
• FDdataoutsideofthebeamtimewindowàFDcosmicraybackground
3. InterpretanyFDdataexcessoverpredictedbackgroundsas!$ appearance
(simulated!e CCevent)
!eselectedeventsintheND
DBD16- OSAKA,JAPAN
E.CATANO-MUR [ISU]– STATUSOFTHENOVAEXPERIMENT 20
§ ND:select3components:beam!$CC,!"CC,NC
§ Correspondto3FDbackgrounds§ Beam!$CC:intrinsic!$ componentin
thebeam.IntheFD,!$ → !$ isabackgroundto!" → !$.Actual!$ eventsà scorehighonclassifier
§ !"CC,NC:eventsthataremisidentifiedas!$CCineitherdetector
§ TranslateNDdatatoaFDbkgd.expectation inenergyxPIDbinsusingFar/Nearratiosfromsimulation
§ ~10%excessofdataoverMC.Howtodivideamongcomponents?
classifiereνCVN 0.75 0.80 0.85 0.90 0.95 1.00
PO
T20
10
×Ev
ents
/ 3.
72
200
400
600
800
1000 ND dataTotal MCFlux Uncert.NC
CCeνBeam CCµν
NOvA Preliminary
Mostsignallike
Reconstructed neutrino energy (GeV)
PO
T20
10×Ev
ents
/ 3.
72
0
1000
2000
3000
NOvA Preliminary0.75 < CVN < 0.87 0.87 < CVN < 0.95 0.95 < CVN < 1
0 1 2 3 4 0 1 2 3 4 0 1 2 3 4 5
Data
eνMC Beam
CCµνMC
MC NC
(Sameevents)
Data-drivenbackground(I)
DBD16- OSAKA,JAPAN E.CATANO-MUR [ISU]– STATUSOFTHENOVAEXPERIMENT 21
§ Recall:dominantdecaymodes–NuMI beam:34 → 54 + !"74 → 54 + !"
§ Small!$ contamination“beam!$”54 → <4 + !$ + !"74 → <4 + !$
§ Wecanuse!"-selectedsamples(morestatistics,fewbackgrounds)tocorrectthenumbersofpionandkaon ancestors,andthusconstrainthebeam!$ CC
§ Usingdata:wefindcorrections~-2%forpions,+17%forkaons
True Neutrino Energy (GeV)0 5 10 15 20
Even
ts /
Bin
/ 6E2
0 PO
T
0
5
10
15
20
310×
All AncestorsOther Ancestor
Ancestor0LK Ancestor+K Ancestor+π
True!$ intheND
True Neutrino Energy (GeV)0 5 10 15 20
Even
ts /
Bin
/ 6E2
0 PO
T
0
1
2
3
4
610×
All AncestorsOther Ancestor
Ancestor0LK Ancestor+K Ancestor+π
True!" intheND
34
74
Data-drivenbackground(II)
DBD16- OSAKA,JAPAN E.CATANO-MUR [ISU]– STATUSOFTHENOVAEXPERIMENT 22
Number of Michels0 1 2+
PO
T20
10×Ev
ents
/ 3.
72
0
5000
10000
15000
NOvA Preliminary
Data CCµνMC
MC NC
eνMC Beam
§ !"CC backgrounds:CCeventsthatdocontainamuon,butitstrackisnotclearlydefinedandit’smistakenfora!$ event
§ Containedevent:themuon decaysinsidethedetector.Dominantmodeis5= → <= + !$ + !"“Michel”electron
§ LookingforMichel-likeactivity,wecangetahandleonthe!"CC
§ Combiningthebeam!$ resultsandafittothenumberofMichels indataà all3componentsarecorrected
Averagecorrections:beam!$ upby4%,NCupby10%,!"CCupby17%
Reconstructed neutrino energy (GeV)
PO
T20
10×Ev
ents
/ 3.
72
0
1000
2000
3000
NOvA Preliminary0.75 < CVN < 0.87 0.87 < CVN < 0.95 0.95 < CVN < 1
0 1 2 3 4 0 1 2 3 4 0 1 2 3 4 5
Data
eνBeam CCµν
NCUncorrected MC
ElectronneutrinoFDprediction
DBD16- OSAKA,JAPAN E.CATANO-MUR [ISU]– STATUSOFTHENOVAEXPERIMENT 23
TotalBG NC Beamνe νµ CC ντ CC Cosmics
8.2 3.7 3.1 0.7 0.1 0.5
NH,3π/2, IH,π/2,
28.2 11.2
Signalevents(±5%systematicuncertainty):
Backgroundbycomponent(±10%systematicuncertainty):
§ FDbeambkgd.estimatedusingNDdata
§ FDsignalexpectationispinnedtotheND-selected!"CCspectrum
§ FDcosmicbkgd. estimatedusingν? selectedFDdataoutsideofthebeamtimewindow
§ Expectedeventcountsdependonoscillationparameters
CPδ
Tota
l eve
nts
expe
cted
0
10
20
30
40
50
02π π
2π3 π2
POT equiv.2010×6.05NOvA FD =0.4-0.623θ2sin
NHIH
NOvA Simulation
ElectronneutrinoFDdata
DBD16- OSAKA,JAPAN E.CATANO-MUR [ISU]– STATUSOFTHENOVAEXPERIMENT 24
NOvA - FNAL E929Run: 22242 / 18Event: 232856 / --UTC Mon Feb 15, 201604:36:13.437062336 sec)µt (
218 220 222 224 226 228
hits
110
210
q (ADC)10 210 310
hits
110
210
5000 5200 5400 5600 5800 6000
x (c
m)
500
600
700
z (cm)5000 5200 5400 5600 5800 6000
y (c
m)
600−
500−
400−
NOvA - FNAL E929Run: 22242 / 18Event: 232856 / --UTC Mon Feb 15, 201604:36:13.437062336 sec)µt (
218 220 222 224 226 228
hits
110
210
q (ADC)10 210 310
hits
110
210
5000 5200 5400 5600 5800 6000
x (c
m)
500
600
700
z (cm)5000 5200 5400 5600 5800 6000
y (c
m)
600−
500−
400−
NOvA - FNAL E929Run: 22242 / 18Event: 232856 / --UTC Mon Feb 15, 201604:36:13.437062336 sec)µt (
218 220 222 224 226 228
hits
110
210
q (ADC)10 210 310
hits
110
210
5000 5200 5400 5600 5800 6000
x (c
m)
500
600
700
z (cm)5000 5200 5400 5600 5800 6000
y (c
m)
600−
500−
400−
NOvA - FNAL E929Run: 22242 / 18Event: 232856 / --UTC Mon Feb 15, 201604:36:13.437062336 sec)µt (
218 220 222 224 226 228
hits
110
210
q (ADC)10 210 310
hits
110
210
5000 5200 5400 5600 5800 6000
x (c
m)
500
600
700
z (cm)5000 5200 5400 5600 5800 6000
y (c
m)
600−
500−
400−
NOvA - FNAL E929Run: 22242 / 18Event: 232856 / --UTC Mon Feb 15, 201604:36:13.437062336 sec)µt (
218 220 222 224 226 228
hits
110
210
q (ADC)10 210 310
hits
110
210
5000 5200 5400 5600 5800 6000
x (c
m)
500
600
700
z (cm)5000 5200 5400 5600 5800 6000
y (c
m)
600−
500−
400−
NOvA - FNAL E929Run: 22242 / 18Event: 232856 / --UTC Mon Feb 15, 201604:36:13.437062336 sec)µt (
218 220 222 224 226 228
hits
110
210
q (ADC)10 210 310
hits
110
210
5000 5200 5400 5600 5800 6000
x (c
m)
500
600
700
z (cm)5000 5200 5400 5600 5800 6000
y (c
m)
600−
500−
400−
NOvA - FNAL E929Run: 22242 / 18Event: 232856 / --UTC Mon Feb 15, 201604:36:13.437062336 sec)µt (
218 220 222 224 226 228
hits
110
210
q (ADC)10 210 310
hits
110
210
5000 5200 5400 5600 5800 6000
x (c
m)
500
600
700
z (cm)5000 5200 5400 5600 5800 6000
y (c
m)
600−
500−
400−
NOvA - FNAL E929Run: 22242 / 18Event: 232856 / --UTC Mon Feb 15, 201604:36:13.437062336 sec)µt (
218 220 222 224 226 228
hits
110
210
q (ADC)10 210 310
hits
110
210
5000 5200 5400 5600 5800 6000
x (c
m)
500
600
700
z (cm)5000 5200 5400 5600 5800 6000
y (c
m)
600−
500−
400−
Observe33eventsinFD§ background8.2±0.8§ >8@ significanceof
appearance
CVN=0.991E=1.63GeV
Reconstructed neutrino energy (GeV)
Even
ts /
0.5
GeV
Bin
0
5
10
15
20
1 2 3 1 2 3 1 2 3
0.75 < CVN < 0.87 0.87 < CVN < 0.95 0.95 < CVN < 1NH
NOvA Preliminary
FD DataBest Fit Prediction Total BackgroundCosmic Background
POT equiv.2010×6.05
Appearanceresults
DBD16- OSAKA,JAPAN E.CATANO-MUR [ISU]– STATUSOFTHENOVAEXPERIMENT 25
Fitforhierarchy,ACP,sin2θ23§ Using2DGaussianC.L.
(FCcorrected:tobepublished)§ Reactorconstraint(PDG2015)
sin2(2θ13)=0.085±0.05§ Δm2constraint(PDG2015)Δm2=2.44±0.06x10-3 eV2(-2.49±0.06x10-3 eV2, IH)
§ Systematiceffectsincludedasnuisanceparameters§ Normalization§ Flux§ Calibration§ Crosssection§ Detectorresponse
CPδ
23θ2sin
0
0.2
0.4
0.6
0.8
1
02π π
2π3 π2
NOvA Preliminary
σ1 σ2 σ3 NH
CPδ
23θ2sin
0
0.2
0.4
0.6
0.8
1
02π π
2π3 π2
NOvA Preliminary
σ1 σ2 σ3 IH
NoFeldman-CousinsCorrection
Appearanceresults
DBD16- OSAKA,JAPAN E.CATANO-MUR [ISU]– STATUSOFTHENOVAEXPERIMENT 26
Fitforhierarchy,ACP,sin2θ23§ Reactorconstraint(PDG2015)
sin2(2θ13)=0.085±0.05§ ConstrainΔm2andsin2θ23with
NOvAdisappearanceresults*Notafulljoint fit,systematicsandotheroscillationparametersnotcorrelated
GlobalbestfitNormalHierarchy
§ 3σ exclusioninIH,loweroctantaroundACP=π/2
§ bestfitIH-NH,ΔB2=0.47§ bothoctantsandhierarchies
allowedat1σ CPδ
23θ2sin
0.2
0.3
0.4
0.5
0.6
0.7
02π π
2π3 π2
NOvA Preliminary
σ1 σ2 σ3 IH
CPδ
23θ2sin
0.2
0.3
0.4
0.5
0.6
0.7
02π π
2π3 π2
NOvA Preliminary
σ1 σ2 σ3 NH
�CP = 1.49⇡sin2(✓23) = 0.40
NoFeldman-CousinsCorrection
Anti-neutrinorunningà helpremovedegeneracies
Outlook
DBD16- OSAKA,JAPAN 27
§ Below:sensitivitiesvstime,assumingfavoredoscillationparametersandmodestimprovementsintheanalysis
§ Startanti-neutrinorunningin2017;run50%neutrino50%anti-neutrinoafter2018
§ Inthenearterm(2018-19)expecttorejectWronghierarchyat>95%CLWrongoctantat>95%CLMax-mixingat>3sigma
Year2016 2018 2020 2022 2024
)σ
Sign
ifican
ce (
0
1
2
3
4
5
=0.02213θ2, sin2eV-310×=2.5322m∆
=0.40323θ2/2, sinπ=3CPδNormal
systematic uncertainty improvements2016 analysis techniques with projected
µν+eνNOvA joint Max. mixingHierarchyOctantCPV
NOvA Simulation
NH33/2Loweroctant
Year2016 2018 2020 2022 2024
)σ
Sign
ifican
ce (
0
1
2
3
4
5
=0.02213θ2, sin2eV-310×=2.5322m∆
=0.62523θ2/2, sinπ=3CPδNormal
systematic uncertainty improvements2016 analysis techniques with projected
µν+eνNOvA joint Max. mixingHierarchyOctantCPV
NOvA Simulation
NH33/2Upperoctant
Summary
DBD16- OSAKA,JAPAN 28
§ With6.05x1020 POT,NOvA finds:§ Muonneutrinosdisappear:Bestfitisnon-maximal
§ Electronneutrinosappear:DataprefersNHatlowsignificance
§ Excellentdetectorandbeamperformance§ Lookingforwardtomoreneutrinodata+antineutrinorunningstartinginspring2017!§ %&' non-maximal?Octant?§ Masshierarchy?
§ Broadphysicsprogram!Sterileneutrinos,cross-sectionmeasurements,exoticsearches...
Reconstructed neutrino energy (GeV)
Even
ts /
0.5
GeV
Bin
0
5
10
15
20
1 2 3 1 2 3 1 2 3
0.75 < CVN < 0.87 0.87 < CVN < 0.95 0.95 < CVN < 1NH
NOvA Preliminary
FD DataBest Fit Prediction Total BackgroundCosmic Background
POT equiv.2010×6.05
Reconstructed neutrino energy (GeV)0 1 2 3 4 5
Even
ts /
0.25
GeV
0
20
40
60
80
100
120 POT-equiv.2010×A 6.05νNO
Best fit prediction
Unoscillated prediction
Data
NOvA Preliminary
Thankyou!
DBD16- OSAKA,JAPAN E.CATANO-MUR [ISU]– STATUSOFTHENOVAEXPERIMENT 29
Argonne,Atlantico,BanarasHinduUniversity,Caltech,Cochin,InstituteofPhysicsandComputerscienceoftheCzechAcademyofSciences,CharlesUniversity,Cincinnati,ColoradoState,CzechTechnicalUniversity,Delhi,JINR,Fermilab,Goiás,IITGuwahati,Harvard,IITHyderabad,U.Hyderabad,Indiana,IowaState,Jammu,Lebedev,MichiganState,Minnesota-TwinCities,Minnesota-Duluth, INRMoscow,Panjab,South Carolina,SDSchoolofMines,SMU,Stanford,Sussex,Tennessee,Texas-Austin,Tufts,UCL,Virginia,WichitaState,WilliamandMary,WinonaState