K2K far detector analysis
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NuFact04@Osaka2004/Aug/27
K2K far detector analysis
ICRR, Univ. of TokyoKenji Kaneyukifor the K2K collaboration
• oscillation analysis strategy• SK data• oscillation analysis• conclusion
NuFact04@Osaka2004/Aug/27
)27.1
(sin2sin.2
22
E
Lmprob
neutrino oscillation probability
atmospheric observation
zenith angle distribution : L dependence @ each energy
L =250km : fixed reduction of events spectrum distortion
E
K2K Long baseline experiment
NuFact04@Osaka2004/Aug/27K2K oscillation analysis strategy
number of eventsp, measurement
@ ND
flux, spectrum interaction
@ ND
flux, spectrumexpectation
@ SK
number of events reconstructed E
observation@ SK
ND
SK
Far/Near ratio
oscillation analysis(sin22,m2)
NuFact04@Osaka2004/Aug/27
measured flux @ ND (previous talk)– 1 ( E< 500) = 0.78 0.36– 2 ( 500 E < 750) = 1.01 0.09– 3 ( 750 E <1000) = 1.12 0.07– 4 (1500 E <2000) = 0.90 0.04– 5 (2000 E <2500) = 1.07 0.06– 5 (2500 E <3000) = 1.33 0.17– 6 (3000 E ) = 1.04 0.18– nQE/QE = 1.02 0.10
2=638.1 for 609 d.o.f
10-6
1.0 2.0
Far/Near flux ratio
beam MCconfirmed by PION monitor
E(GeV)
NuFact04@Osaka2004/Aug/27
Super-Kamiokande (Far detector on K2K)
39.3m
41.4m
50kt total volume22.5kt fiducial volume
20’PMT photocathode coverage SK-I 11,146 40%SK-II 5,182 19%
1000m underground
NuFact04@Osaka2004/Aug/27
Summary of SK-2 absolute energy calibration
various sources (decay-e, 0, low-energy , high energy ) are usedto estimate the energy uncertainty.data agree with MC within ±1.9%time variation : ±0.9%
total uncertainty : ±2.1%
NuFact04@Osaka2004/Aug/27event reconstruction on K2K-II
sub-GeVsub-GeV Evis>500MeV/c
likelihood distribution for ring counting likelihood distribution for PID
1-ring ≥2-ring
atmospheric dataMC exp.
w/ osc.
Likelihood distribution of atmospheric neutrino data agree with MC.(dis-agreements are taken into account to the systematic error.)
e-like -like
NuFact04@Osaka2004/Aug/27SK event selection
500sec
5sec
Decay electron cut.
20MeV Deposited Energy
No OD activity, fiducial volume,Evis 30MeV
TOF (0.83ms) cut using GPS
108 FC events in fiducial volume
1.6BG eventswithin 500msec
NuFact04@Osaka2004/Aug/27SK event summary
K2K-I+II
(K2K-I, K2K-II)
Data
(K2K-I, K2K-II)
MC
(K2K-I, K2K-II)
FC 108 (56, 52) 150.9 (79.1,71.8)
1ring 66 (32,34) 93.7 (48.6, 45.1)
-like
(for shape)
57 (30, 27)
(56 (29, 27))
84.8 (44.3, 40.5)
e-like 9 (2, 7) 8.8 (4.3, 4.5)
multi-ring 42 (24, 18) 57.2 (30.5, 26.7)
K2K-I(47.9×1018POT), K2K-II(41.2×1018POT)
NuFact04@Osaka2004/Aug/27K2K oscillation analysis
• Total Number of events
• Erec spectrum shape of FC-1ring- events
• Systematic error term
)(),2sin,(),2sin,(
),2sin,(22
2
xsyst
xshape
xnorm
x
fLfmLfmL
fmL
f x : Systematic error parameters
Poisson prob. for FC events
shape for Erec
for 1ring eventsystematic error
normalization, spectrum, nQE/QE, Far/Near, SK systematic uncertainty
NuFact04@Osaka2004/Aug/27Best fit
All parameter region(sin22, m2)=(1.53, 2.12x10-3)
In physical region(sin22, m2)=(1.00, 2.73x10-3)
logL=0.64
1.00
2.73
• NSKobs=108
• NSKexp (best fit)=104.8
shape : KS prob.=52%
Best fit expectation reproduce data well.
sin22≥1.53 can be occurred by statistical fluctuation with 14.4%.
data
oscillated expectation
w/o osc.
NuFact04@Osaka2004/Aug/27
- oscillation allowed region
best fit(sin22, m2)=(1.53, 2.12x10-3) (all)=(1.00, 2.73x10-3) (phys.)
1.7×10-3 ≤Δm2 ≤3.5×10-3 (90%C.L.) @ sin22=1.0
K2K-I+II 8.9x1019POT
NuFact04@Osaka2004/Aug/27
number of events v.s. E shape distortion
•
sin22sin22
m2[eV
2]
m2[eV
2]
number of events E shape
Oscillation analysis results based on number of events and the E spectrum distortion are consistent.
NuFact04@Osaka2004/Aug/27K2K-I vs K2K-II
K2K-I and K2K-II results are consistent.
K2K-I K2K-II
data
best fitoscillated expectation
w/o osc.
Erec
allowed region
NuFact04@Osaka2004/Aug/27
Oscillation analysis results based on neutrino interaction model (CC 1 re-weighted and no coherent )
oscillation results are robust to interaction assumption.
NuFact04@Osaka2004/Aug/27
- oscillation allowed region
K2K
SK-I 2flavor SK-I L/E
K2K result is consistent with SK-I results.
NuFact04@Osaka2004/Aug/27
Null oscillation probability (lnL)
K2K-I K2K-II K2K-I+II
number of events 2.0% 3.7% 0.33%(2.94)
E spectrum distortion 19.5% 5.4% 1.1% (2.53)
Combined 1.3%(2.48)
0.56%(2.77)
0.011%(3.86)
K2K confirmed neutrino oscillation discovered in Super-Kamiokande atmospheric neutrinos at 3.86.
Both number of events and E spectrum distortionare consistent with neutrino oscillation.
NuFact04@Osaka2004/Aug/27
ConclusionK2K confirmed neutrino oscillation at 3.86.
Both number of events and E spectrum distortionare consistent with neutrino oscillation. number of events 2.94 E spectrum distortion 2.53
Allowed region for dis-appearance is1.7×10-3 ≤Δm2 ≤3.5×10-3 (90%C.L.) @ sin22=1.0
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