recent neutrino oscillation results from t2k
TRANSCRIPT
Son V. Cao -‐ Kyoto University(On behalf of the T2K collaboration )
Recent neutrino oscillation results from T2K
7/14/16 PASCOS 2016, Quy Nhon, VN
² Introduction to 𝜈 oscillations
² Introduction to T2K experiment
² T2K latest results
² Summary
Brief neutrino history
7/14/16 PASCOS 2016, Quy Nhon, VN 2
Credit to APS
² 1930: On-‐paper appearance as “desperate” remedy by W. Pauli² 1956: first experimentally discovered by Reines and Cowan² 1962: existence confirmed by Lederman et al. ² 1998: Atmospheric neutrino oscillations discovered by Super-‐K² 2000: first evidence reported by DONUT experiment² 2001: Solar neutrino oscillations detected by SNO (KamLAND 2002)² 2011: transitions observed by OPERA² 2011-‐13: by T2K, deficit observed by Daya Bay(2012) ² 2015: Nobel prizes for 𝜈 oscillations, Breakthrough prize (2016)
⌫̄e
⌫µ
⌫⌧
⌫µ ! ⌫⌧⌫µ ! ⌫e ⌫̄e ! ⌫̄e
2015
T2K observe 𝜈𝜇à𝜈eappearance
Nobel & Breakthroughfor 𝜈 oscillations
Standard Model & neutrino oscillations
37/14/16 PASCOS 2016, Quy Nhon, VN
Source: AAAS
0
@⌫e⌫µ⌫⌧
1
A =
0
@1 0 00 c23 s230 �s23 c23
1
A
0
@c12 s12 0�s12 c12 00 0 1
1
A
0
@c13 0 s13e�i�CP
0 1 0�s13ei�CP 0 c13
1
A
0
@⌫1⌫2⌫3
1
APontecorvo(1957)
Maki,NakagawaSakata(1962)
Majorana(1937)
Standard Model:² Neutrinos interact through the weak
interaction
² Lepton flavor is strictly conserved
² Neutrinos have zero mass
Neutrino oscillations:
² Indicate massive neutrinos
² Mix flavor and mass eigenstates
² Beyond Standard Model
Flavor eigenstates Mass eigenstates
Standard Model & neutrino oscillationsStandard Model:² Neutrinos interact through the weak
interaction
² Lepton flavor is strictly conserved
² Neutrinos have zero mass
Neutrino oscillations:
² Indicate massive neutrinos
² Mix flavor and mass eigenstates
² Beyond Standard Model
47/14/16 PASCOS 2016, Quy Nhon, VN
Reactors / acceleratorSolar / reactors
0
@⌫e⌫µ⌫⌧
1
A =
0
@1 0 00 c23 s230 �s23 c23
1
A
0
@c12 s12 0�s12 c12 00 0 1
1
A
0
@c13 0 s13e�i�CP
0 1 0�s13ei�CP 0 c13
1
A
0
@⌫1⌫2⌫3
1
A
Source: AAAS
cij = cos ✓ij , sij = sin ✓ij
Atmospherics / Accelerators
Present neutrino oscillation landscape
7/14/16 PASCOS 2016, Quy Nhon, VN 5
Gonzalez-‐Garcia et al., arXiv:1512.06856 ⌫e ⌫µ ⌫⌧
Normal hierarchy Inverted hierarchy
m2lightest m2
lightest
0
@⌫e⌫µ⌫⌧
1
A =
0
@1 0 00 c23 s230 �s23 c23
1
A
0
@c12 s12 0�s12 c12 00 0 1
1
A
0
@c13 0 s13e�i�CP
0 1 0�s13ei�CP 0 c13
1
A
0
@⌫1⌫2⌫3
1
A
sign(�m232) = ?
✓23 is maximal ?
�CP = ?
mlightest = ?
�m232
�m231
�m221
�m221
⌫1
⌫2
⌫3
⌫1
⌫2
⌫3
�m221 = 7.50+0.19
�0.17 ⇥ 10�5eV2
�m231 = 2.457+0.047
�0.047 ⇥ 10�3eV2
✓13 = 8.50+0.20�0.21(
�)
✓12 = 33.48+0.78�0.75(
�)
✓23 = 42.3+3.0�1.6(
�)
�m2ij = m2
⌫i�m2
⌫j
Global fit – Normal hierarchy
T2K experiment
7/14/16 6PASCOS 2016, Quy Nhon, VN
² Long-‐baseline neutrino experiment, located in Japan² Large collaboration: ~400 physicists from 61 institutes/ 11 nations² Rich programs: standard neutrino oscillations (this talk), non-‐standard
physics search (Phillip’s talk), neutrino interactions (David’s talk)
J-‐PARC neutrino beam line
7/14/16
² High intensity, almost pure muon (anti) neutrino beam from J-‐PARC
7PASCOS 2016, Quy Nhon, VN
² 30 GeV p extracted from J-‐PARC main ring, impinge on 90-‐cm, graphite target ² Induced 𝜋+ (𝜋-‐) focused by three horns, pass through a 96-‐m decay pile² Beam dump to stop all particles except neutrinos and high-‐energy muons² Muon monitor, downstream of beam dump, to monitor beam intensity and direction by
measuring induced muon profile.
1.9⇥ �int
Beam power and data accumulation
7/14/16 PASCOS 2016, Quy Nhon, VN 8
!-mode POT: 7.57×1020 (50.14%) !-mode POT: 7.53×1020 (49.86%)
27 May 2016POT total: 1.510×1021
2011 2012 2013 2014 2015 2016
² Beam power steadily increased to 420 kW² 1.5x1021 Protons-‐on-‐target (POT) accumulated. Data sample for
results presented today:² Neutrino-‐mode: 6.91x1020 POT² Antineutrino-‐mode: 7.53x1020 POT (approx. 2 x 1st T2K antineutrino results)
Neutrino flux inference
7/14/16
² High intensity, almost pure muon (anti) neutrino beam from J-‐PARC
9PASCOS 2016, Quy Nhon, VN
² To infer neutrino flux, knowledge of hadron production at target needed
² Constrained by external data from NA61/SHINE
Flux uncertainty ~ 10%
Neutrino mode Antineutrino mode< 1%(⌫e/⌫e) < 1%(⌫e/⌫e)
T2K Far Detector T2K Far Detector
T2K Far Detector T2K Far Detector
(Beam modes changed by switching horn polarity)
Near Detectors
7/14/16 PASCOS 2016, Quy Nhon, VN 10
² Near Detector complex is 280m downstream of target
On-‐axis (called INGRID)Measure 𝜈 beam intensity & profile: 16 scintillator-‐steel interleaved modules (7.1 tons/each)
Off-‐axis (called ND280)Understand unoscillated 𝜈 beam: further constrain flux and cross-‐section parameters
Near Detectors measurements
11
Day
[eve
nts/
1e14
POT
]
0.40.60.8
11.21.41.61.8
Event rateHorn250kAHorn205kAHorn-250kA
[mra
d]
1−
0.5−
0
0.5Horizontal beam direction INGRID
MUMON
Day
[mra
d]
1−
0.5−
0
0.5
1Vertical beam direction INGRID
MUMON
T2K Run1Jan.2010-Jun.2010
T2K Run2Nov.2010-Mar.2011
T2K Run3Mar.2012-Jun.2012
T2K Run4Oct.2012-May.2013
T2K Run5May.2014-Jun.2014
T2K Run6Oct.2014-June.2015
T2K Run7Feb.2016-May.2016
7/14/16 PASCOS 2016, Quy Nhon, VN
Operating stably
Beam intensity/profile
Constrain flux
& 𝜈-‐int. model
Prefit = No ND280 dataPostfit = ND280 data included
Cross-‐section parameters
Off-‐axis neutrino energy strongly depend on beamdirection (1mrad ~ 2% shift of peak energy)
Data used as much as possibleto constrain 𝜈-‐int. model
Far Detector, Super-‐Kamiokande
7/14/16 PASCOS 2016, Quy Nhon, VN 12
(GeV)νE0 1 2 3
(A.U
.)29
5km
µν
Φ
0
0.5
1 °OA 0.0°OA 2.0°OA 2.5
0 1 2 3
) eν →µν
P(
0.05
0.1 = 0CPδNH, = 0CPδIH,
/2π = CPδNH, /2π = CPδIH,
0 1 2 3
)µν
→µν
P(
0.5
1
= 1.023θ22sin = 0.113θ22sin
2 eV-3 10× = 2.4 322m∆
Partice ID parameter-10 -8 -6 -4 -2 0 2 4 6 8 100
50
100
150
200
250
300
350
Super Kamiokande IV 2166.5 days : Monitoring
e-like muon-like
Num
ber o
f eve
nts
² Muon and electron are well-‐separatedà identify 𝜈𝜇/𝜈$ with high purity
² Super-‐K is 2.50 off the beam’s axis to achieve narrow band beam peaked at oscillation maximum (0.6 GeV)
(atmospheric 𝜈 data)
Super-‐Kamiokande(41.4 m tall x 39.3m diameter)22.5 ktons fiducial volume
1000m underground
⌫µ + n ! µ� + p
⌫e + n ! e� + p
Oscillation parameters extracted from T2K data
7/14/16 PASCOS 2016, Quy Nhon, VN 13
NH: Normal 𝜈 mass hierarchyIH: Inverted 𝜈 mass hierarchy
*Reactor constraint used as prior if is appliedsin2 2✓13 = 0.085± 0.005
Disappearance channel, sensitive to 𝜃23 & ∆𝑚()
)Appearance channel, sensitive to 𝜃13 & 𝛿CP
⌫µ candiate ⌫µ candiate
⌫e candiate
⌫e candiate
7/14/16 PASCOS 2016, Quy Nhon, VN 14
*Reactor constraint used as prior if is appliedsin2 2✓13 = 0.085± 0.005
Disappearance channel, sensitive to 𝜃23 & ∆𝑚()
)Appearance channel, sensitive to 𝜃13 & 𝛿CP
⌫µ candiate ⌫µ candiate
⌫e candiate
⌫e candiate
² Today result: All 𝜈/�̅� samples are combined to extract oscillation parameters. The 𝜈 and �̅� are treated identically.
² Different approaches for statistical treatment:o Frequentist and Bayesiano Fit on reconstructed E𝜈 or momentum/angle
of induced leptons² They agree with each other
Oscillation parameters extracted from T2K data
Results: 𝜃23 & ∆𝑚())
7/14/16 PASCOS 2016, Quy Nhon, VN
² Since 2014, mainly taking data in �̅� mode (run 5-‐7)
² 𝜈𝜇 disappearance behaves consistently w/ 𝜈, disappearance
² Result consistent with maximal mixing, the world’s highest precision 𝜃23 measurement
² Slightly favor normal mass hierarchy
15
Normal MH(𝛥𝝌2
best-‐fit=0.0)InvertedMH
(𝛥𝝌2best-‐fit=2.66)
sin2𝜃23 0.53245.56575.588 0.53445.5:;75.58<
∆𝑚())
/104((eV2) 2.54545.5?)75.5?8 2.51045.5?(75.5?)
𝜈: 6.91x1020 POT + �̅�: 7.53x1020 POT
T2K Run1-‐7b preliminary
T2K Run1-‐7b preliminary
Results: 𝜃13 & 𝛿CP
7/14/16 PASCOS 2016, Quy Nhon, VN 16
T2K data only
T2K data + reactor
² Shows for two cases: (i) T2K data only & (ii) T2K data w/ reactor constraint
²Mass hierarchy is fixed, either normal or inverted and compute independently
²Measured 𝜃13 w/ T2K data only (top plot) agrees with reactor measurement
² With reactor constraint, data exclude positive value of 𝛿CP at ~90% C.L.
Results: 𝛿CP
7/14/16 PASCOS 2016, Quy Nhon, VN 17
T2K + reactorObservation
Sensitivity
² Slightly favor 𝛿CP = -‐𝜋/2² Measured 𝛥𝝌2 is marginally different than
the expected one² It is due to difference btw/ observed data
and expectation, specifically² 𝜈$ appearance is larger than expected² 𝜈$B “appearance” is smaller than expected
Summary
7/14/16 PASCOS 2016, Quy Nhon, VN
² Results with 𝜈/�̅� combined data showno Consistent with 𝜃23 maximal mixing o Slightly prefer normal mass hierarchyo Slightly favor 𝛿CP = -‐𝜋/2
𝛿CP = [-‐3.02, -‐0.49] (NH), [-‐1.87, -‐0.98] (IH) at 90% C.L.
àMore statistics are needed
² J-‐PARC beam power has steadily increased up to 420 kW
² Accumulated exposure of 1.5x1021 POT (~20% of T2K total approved running)
Stay tuned for upcoming results from T2K
18
7/14/16 PASCOS 2016, Quy Nhon, VN 19
Thank you!(Cảm ơn)
T2K Phase 2 proposal
7/14/16 PASCOS 2016, Quy Nhon, VN
² Approved T2K statistics, 7.8 x1021POT, can be accumulated by JFY2020
² Hyper-‐K and DUNE are expected to start around 2026
² T2K Phase 2, if extended to JFY2026, collects ~ 20x1021 POT
² Neutrino beamlineupgrade & analysis improvements (SK fiducialvolume, add new event sample) à Effectively add 50% statistics
² Reduction of systematic uncertainties to enhance CPV sensitivity
20
Number of events expected at T2K far detector with full proposed T2K Phase 2 exposure
J-‐PARC Main Ring expected beam power& T2K Phase 2 accumulation scenario
T2K Phase 2 sensitivity to CPV
7/14/16 PASCOS 2016, Quy Nhon, VN 21
)21Protons-on-Target (x100 5 10 15 20
=0C
Pδ
to e
xclu
de s
in2 χ
∆
0
5
10
15 =0.4323θ2True sin
=0.5023θ2True sin
=0.6023θ2True sin
90% C.L.
99% C.L.
C.L.σ 3
w/ eff. stat. improvements (no sys. errors)
w/ eff. stat. & sys. improvements
Work in Progress
)°(CPδTrue 200− 100− 0 100 200
=0C
Pδ
to e
xclu
de s
in2 χ
∆
0
5
10
15
20
=0.4323θ2True sin=0.5023θ2True sin=0.6023θ2True sin
90% C.L.
99% C.L.
C.L.σ 3
POT w/ eff. stat. & sys. improvements2120x10 POT w/ 2016 sys. errs.217.8x10
Work in Progress
�CP = �⇡
2
² > 3𝜎 significance sensitivity to CP violation if 𝛿CP= -‐ 𝜋/2
² 99% C.L. significance for more than 45% of the possible true values of 𝛿CP
² 1% precision of 𝛥m223, 0.5o -‐ 1.7o
precision of 𝜃23 depending on its true value, ~3𝜎 significance for resolving 𝜃23 octant if sin2 𝜃23 >0.6 or sin2 𝜃23 <0.43
23θ2sin0.4 0.5 0.6
322 m
∆
2.2
2.4
2.6
2.8
33−10×
Current POT , 90% C.L
POT, 90% C.L217.8x10
POT w/improvement, 90% C.L2120x10
Stat. onlySystematics
Work in Progress
True sin2 ✓23 = 0.6
Bayesian posterior probability
7/14/16 22
�NSK/NSK
NH IH Sum
sin2θ23≤0.5 21.8% 7.2% 29.0%
sin2θ23>0.5 53.9% 18.1% 71.0%
Sum 74.7% 25.3% 100%Bayesian w/ MCMC
(Erec)
(Plep/𝜃lep)
² Prefer normal mass hierarchy and higher octant
Bayesian w/ likelihood fit(Erec)
PASCOS 2016, Quy Nhon, VN
Frequentist(Erec for 𝜈𝜇/𝜈, )(Erec/ 𝜃lep for 𝜈$/𝜈$B )
Backup: Data fit vs sensitivity
7/14/16 PASCOS 2016, Quy Nhon, VN 23
10k toys 10k toys
² Toy experiments at true values of 𝛿CP & MH generated to understand data fit outcomes
² Probability to exclude 𝛿CP = (0, 𝜋) is evaluated
² Data agree w/ 𝛿CP = -‐1.76 (~-‐𝜋/2), normal MH at 2𝜎 level and probability to exclude 𝛿CP =0 is non-‐negligible (>8%)
True: 𝛿CP = -‐1.76, normal MHTrue: 𝛿CP = 0, normal MH
Prop. (%)to exclude
True para.𝛿CP = -‐1.76, NH
True para.𝛿CP = 0, NH
90% CL 2𝝈 90% CL 2𝝈𝛿CP =0, NH 18.7 8.9 10.2 4.7
𝛿CP =𝜋, NH 16.3 6.8 13.4 6.5
Systematic error table
7/14/16 PASCOS 2016, Quy Nhon, VN 24
𝜈-‐mode (%) 𝝂B-‐mode (%)𝜇-‐like e-‐like 𝜇-‐like e-‐like
Flux 3.59 3.67 3.68 3.78𝜈 int. 4.10 5.20 5.43 3.78SK det. 4.15 3.50 3.94 3.97Osc. par. 0.03 4.16 0.03 4.00Pre fit 11.9 12.6 12.7 14.3Post fit 5.13 6.80 5.12 7.41
�NSK/NSK
90% range of 𝛿CP
7/14/16 PASCOS 2016, Quy Nhon, VN 25
�NSK/NSK
Fit with DataSensitivity
Data fit vs sensitivity
7/14/16 PASCOS 2016, Quy Nhon, VN 26
Results: 𝜃13 & 𝛿CP
7/14/16 PASCOS 2016, Quy Nhon, VN 27
T2K + reactor
Sensitivity
T2K data only
Observation
²Agree w/ reactor
²Marginally differ from expectation (next slides)
�CP = �1.601,
sin2 ✓13 = 0.0217,
sin2 ✓23 = 0.528,
�m232 = 2.509⇥ 10�3eV 2/c4
Assume (PDG 2015):
BANFF: flux RHC
7/14/16 PASCOS 2016, Quy Nhon, VN
² 15% increase
28
(GeV)νE-110 1 10
Flux
Par
amet
er V
alue
0.6
0.7
0.8
0.9
1
1.1
1.2
1.3
1.4
Prior to ND280 Constraint
After ND280 Constraint
beam modeν, eνND280
(GeV)νE-110 1 10
Flux
Par
amet
er V
alue
0.6
0.7
0.8
0.9
1
1.1
1.2
1.3
1.4
Prior to ND280 Constraint
After ND280 Constraint
beam modeν, eνND280
(GeV)νE-110 1 10
Flux
Par
amet
er V
alue
0.6
0.7
0.8
0.9
1
1.1
1.2
1.3
1.4
Prior to ND280 Constraint
After ND280 Constraint
beam modeν, µνND280
(GeV)νE-110 1 10
Flux
Par
amet
er V
alue
0.6
0.7
0.8
0.9
1
1.1
1.2
1.3
1.4
Prior to ND280 Constraint
After ND280 Constraint
beam modeν, µνND280
Neutrino oscillations² Now well-‐understood phenomenon² Quantum mechanical mixing between mass and flavor eigenstates
|⌫↵(0)i = U↵i|⌫i(0)i↵ = e, µ, ⌧ i = 1, 2, 3
|⌫�(t)i = U�j |⌫j(t)i� = e, µ, ⌧ j = 1, 2, 3
|⌫↵(0)i |⌫�(t)i
U⇤↵i U�j
e�mit
Credit to Boris K.
297/14/16 PASCOS 2016, Quy Nhon, VN
Neutrino oscillationsProbability (in vacuum):
* Abbreviated after Pontecorvo, Maki, Nakagawa, Sakata
UPMNS =
0
@1 0 00 c23 s230 �s23 c23
1
A
0
@c13 0 s13e�i�CP
0 1 0�s13ei�CP 0 c13
1
A
0
@c12 s12 0�s12 c12 00 0 1
1
A
Atmospherics / Accelerators Reactors / accelerator Solar neutrino / reactors
307/14/16 PASCOS 2016, Quy Nhon, VN
P⌫↵!⌫� (t) =|h⌫� |⌫↵(t)i|2
=�↵� � 4X
i>j
<(U⇤↵iU�iU↵jU
⇤�j) sin
2(�m2
ijL
4E)
+ 2X
i>j
=(U⇤↵iU�iU↵jU
⇤�j) sin(
�m2ijL
4E),
Non-‐zero
T2K off-‐axis detector: ND280
7/14/16 PASCOS 2016, Quy Nhon, VN
Aim to understand unoscillated 𝜈 beam: constrains flux and cross-‐section parameters ² Tracker, composed of Fine-‐Grained Detector (FGD)
and Time Projection Chamber (TPC), is central parto Two FGDs: active target w/ scintillator only
(FGD1) or scintillator-‐water interleaved (FGD2)o Three TPCs: mainly Argon (95%) filled, for
momentum measurement and particle ID ² 𝜋0 detector (POD) for water-‐scintillator target and 𝜋0
tagging ² Electromagnetic calorimeters (ECal) to detect gamma
rays and reconstruct 𝜋0
² Side muon range detectors (SMRD) to tag entering cosmic muons or side-‐exiting muons
Key features for cross-‐section: o Narrow flux spectrum , mean ~ 0.85 GeVo Multiple targets: scintillator, water, argon, leado High final state ID resolution, charge separation
31
~B
0.2 T
Pre-‐fit: muon momentum
7/14/16 PASCOS 2016, Quy Nhon, VN 32
Muon momentum (MeV/c)0 500 1000 1500 2000 2500 3000 3500 4000 4500 5000
Even
ts/(1
00 M
eV/c
)
0
500
1000
1500
2000
2500Data
CCQEν
CC 2p-2hν
π CC Res 1ν
π CC Coh 1ν
CC Otherν
NC modesν
modesν
FGD1,nu, CC0pi
Muon momentum (MeV/c)0 500 1000 1500 2000 2500 3000 3500 4000 4500 5000
Even
ts/(1
00 M
eV/c
)
0
50
100
150
200
250
300
350
400Data
CCQEν
CC 2p-2hν
π CC Res 1ν
π CC Coh 1ν
CC Otherν
NC modesν
modesν
FGD1,nu, CC1pi
Muon momentum (MeV/c)0 500 1000 1500 2000 2500 3000 3500 4000 4500 5000
Even
ts/(1
00 M
eV/c
)
0
50
100
150
200
250Data
CCQEν
CC 2p-2hν
π CC Res 1ν
π CC Coh 1ν
CC Otherν
NC modesν
modesν
FGD1,nu, CCres
Muon momentum (MeV/c)0 1000 2000 3000 4000 5000 6000 7000 8000 9000 10000
Even
ts/(1
00 M
eV/c
)
0
50
100
150
200
250
Data
CCQEν
non-CCQEν
CCQEν
non-CCQEν
FGD1,Antinu, CC1trk
Muon momentum (MeV/c)0 1000 2000 3000 4000 5000 6000 7000 8000 9000 10000
Even
ts/(1
00 M
eV/c
)
0
5
10
15
20
25
30
35
40Data
CCQEν
non-CCQEν
CCQEν
non-CCQEν
FGD1,Antinu, CCNtrk
Muon momentum (MeV/c)0 1000 2000 3000 4000 5000 6000 7000 8000 9000 10000
Even
ts/(1
00 M
eV/c
)
0
10
20
30
40
50
60
Data
CCQEν
non-CCQEν
CCQEν
non-CCQEν
FGD1,nu, CC1trk
Muon momentum (MeV/c)0 1000 2000 3000 4000 5000 6000 7000 8000 9000 10000
Even
ts/(1
00 M
eV/c
)
0
5
10
15
20
25
30
35
40Data
CCQEν
non-CCQEν
CCQEν
non-CCQEν
FGD1,nu, CCNtrk
Post-‐fit: muon momentum
7/14/16 PASCOS 2016, Quy Nhon, VN 33
Muon momentum (MeV/c)0 500 1000 1500 2000 2500 3000 3500 4000 4500 5000
Even
ts/(1
00 M
eV/c
)
0
500
1000
1500
2000
2500Data
CCQEν
CC 2p-2hν
π CC Res 1ν
π CC Coh 1ν
CC Otherν
NC modesν
modesν
FGD1,nu, CC0pi
Muon momentum (MeV/c)0 500 1000 1500 2000 2500 3000 3500 4000 4500 5000
Even
ts/(1
00 M
eV/c
)
0
50
100
150
200
250
300
350
400Data
CCQEν
CC 2p-2hν
π CC Res 1ν
π CC Coh 1ν
CC Otherν
NC modesν
modesν
FGD1,nu, CC1pi
Muon momentum (MeV/c)0 500 1000 1500 2000 2500 3000 3500 4000 4500 5000
Even
ts/(1
00 M
eV/c
)
0
50
100
150
200
250Data
CCQEν
CC 2p-2hν
π CC Res 1ν
π CC Coh 1ν
CC Otherν
NC modesν
modesν
FGD1,nu, CCres
Muon momentum (MeV/c)0 1000 2000 3000 4000 5000 6000 7000 8000 9000 10000
Even
ts/(1
00 M
eV/c
)
0
50
100
150
200
250
Data
CCQEν
non-CCQEν
CCQEν
non-CCQEν
FGD1,Antinu, CC1trk
Muon momentum (MeV/c)0 1000 2000 3000 4000 5000 6000 7000 8000 9000 10000
Even
ts/(1
00 M
eV/c
)
0
5
10
15
20
25
30
35
40Data
CCQEν
non-CCQEν
CCQEν
non-CCQEν
FGD1,Antinu, CCNtrk
Muon momentum (MeV/c)0 1000 2000 3000 4000 5000 6000 7000 8000 9000 10000
Even
ts/(1
00 M
eV/c
)
0
10
20
30
40
50
60
Data
CCQEν
non-CCQEν
CCQEν
non-CCQEν
FGD1,nu, CC1trk
Muon momentum (MeV/c)0 1000 2000 3000 4000 5000 6000 7000 8000 9000 10000
Even
ts/(1
00 M
eV/c
)
0
5
10
15
20
25
30
35
40Data
CCQEν
non-CCQEν
CCQEν
non-CCQEν
FGD1,nu, CCNtrk
Pre-‐fit: muon angle
7/14/16 PASCOS 2016, Quy Nhon, VN
² 2x3 sample for neutrinos (FGD1,2)
² 2x4 sample for anti-‐neutrinos (FGD1,2)
34
θMuon cos0.8 0.82 0.84 0.86 0.88 0.9 0.92 0.94 0.96 0.98 1
Even
ts/(0
.01)
0
50
100
150
200
250Data
CCQEν
non-CCQEν
CCQEν
non-CCQEν
FGD1,Antinu, CC1trk
θMuon cos0.8 0.82 0.84 0.86 0.88 0.9 0.92 0.94 0.96 0.98 1
Even
ts/(0
.01)
0
50
100
150
200
250Data
CCQEν
non-CCQEν
CCQEν
non-CCQEν
FGD1,Antinu, CCNtrk
θMuon cos0.6 0.65 0.7 0.75 0.8 0.85 0.9 0.95 1
Even
ts/(0
.01)
0
200
400
600
800
1000
1200
1400
1600 Data CCQEν
CC 2p-2hν
π CC Res 1ν
π CC Coh 1ν
CC Otherν
NC modesν
modesν
FGD1,nu, CC0pi
θMuon cos0.6 0.65 0.7 0.75 0.8 0.85 0.9 0.95 1
Even
ts/(0
.01)
0
100
200
300
400
500Data CCQEν
CC 2p-2hν
π CC Res 1ν
π CC Coh 1ν
CC Otherν
NC modesν
modesν
FGD1,nu, CC1pi
θMuon cos0.6 0.65 0.7 0.75 0.8 0.85 0.9 0.95 1
Even
ts/(0
.01)
0
100
200
300
400
500
Data CCQEν
CC 2p-2hν
π CC Res 1ν
π CC Coh 1ν
CC Otherν
NC modesν
modesν
FGD1,nu, CCres
θMuon cos0.8 0.82 0.84 0.86 0.88 0.9 0.92 0.94 0.96 0.98 1
Even
ts/(0
.01)
0
20
40
60
80
100
120
140
160 Data
CCQEν
non-CCQEν
CCQEν
non-CCQEν
θMuon cos0.8 0.82 0.84 0.86 0.88 0.9 0.92 0.94 0.96 0.98 1
Even
ts/(0
.01)
0
20
40
60
80
100
120
140Data
CCQEν
non-CCQEν
CCQEν
non-CCQEν
FGD1,nu, CC1trk
FGD1,nu, CCNtrk
Post-‐fit: muon angle
7/14/16 PASCOS 2016, Quy Nhon, VN 35
θMuon cos0.8 0.82 0.84 0.86 0.88 0.9 0.92 0.94 0.96 0.98 1
Even
ts/(0
.01)
0
50
100
150
200
250Data
CCQEν
non-CCQEν
CCQEν
non-CCQEν
FGD1,Antinu, CC1trk
θMuon cos0.8 0.82 0.84 0.86 0.88 0.9 0.92 0.94 0.96 0.98 1
Even
ts/(0
.01)
0
50
100
150
200
250Data
CCQEν
non-CCQEν
CCQEν
non-CCQEν
FGD1,Antinu, CCNtrk
θMuon cos0.6 0.65 0.7 0.75 0.8 0.85 0.9 0.95 1
Even
ts/(0
.01)
0
200
400
600
800
1000
1200
1400
1600 Data CCQEν
CC 2p-2hν
π CC Res 1ν
π CC Coh 1ν
CC Otherν
NC modesν
modesν
FGD1,nu, CC0pi
θMuon cos0.6 0.65 0.7 0.75 0.8 0.85 0.9 0.95 1
Even
ts/(0
.01)
0
100
200
300
400
500Data CCQEν
CC 2p-2hν
π CC Res 1ν
π CC Coh 1ν
CC Otherν
NC modesν
modesν
FGD1,nu, CC1pi
θMuon cos0.6 0.65 0.7 0.75 0.8 0.85 0.9 0.95 1
Even
ts/(0
.01)
0
100
200
300
400
500
Data CCQEν
CC 2p-2hν
π CC Res 1ν
π CC Coh 1ν
CC Otherν
NC modesν
modesν
FGD1,nu, CCres
θMuon cos0.8 0.82 0.84 0.86 0.88 0.9 0.92 0.94 0.96 0.98 1
Even
ts/(0
.01)
0
20
40
60
80
100
120
140
160 Data
CCQEν
non-CCQEν
CCQEν
non-CCQEν
θMuon cos0.8 0.82 0.84 0.86 0.88 0.9 0.92 0.94 0.96 0.98 1
Even
ts/(0
.01)
0
20
40
60
80
100
120
140Data
CCQEν
non-CCQEν
CCQEν
non-CCQEν
FGD1,nu, CC1trk
FGD1,nu, CCNtrk
² 2x3 sample for neutrinos (FGD1,2)
² 2x4 sample for anti-‐neutrinos (FGD1,2)