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July 4, 2002νFact02@Imperial CollegeLondon
Translation from Near to Far t K2Kat K2K
T KobayashiT.KobayashiIPNS, KEK
for K2K beam monitor groupfor K2K beam monitor group(K.Nishikawa, T.Hasegawa, T.Inagaki,
T.Maruyama, T.Nakaya, ....)a uya a, a aya, )Especially for T.Maruyama(KEK Chicago) who
played major role in PIMON i / / l i
1
construction/measurement/analysis
Strategy of K2K
π+ νμπμ+
Target+Horn200
SK
100 250k
Pion monitor(PIMON)
MUMON FD
200mdecay pipe
100m ~250km
( )
12
x1010
8x104
νμ spectrum@productionνμspectrum @SK
(MC)
Extrapolate bymultiplying ratio(≠0)
11.21.41.6
4
8
4
6
8 (MC)
w/o osc.
arb.
uni
t
uni
t
0.20.40.60.81
10 2 43 5E (GeV)ν
4
2
4
(MC)w/ osc?a
arb.
2
00.20 0.5 1 1.5 2 2.5 3 3.5 4 4.5 5
E (GeV)ν10 2 43 5E (GeV)νmeasure w/ FD
measured by PIMON
What’s new in the treatment of far/near extrapolation
• Before– Observable for osc. analysis:
• total # of events
– added syst. error from each energy bins linearly (= 100% iti l ti ) t b f100% positive correlation) to be safe.
• New– Observables for osc. analysis
• total # of events,E rec h f 1 i lik t• Eν
rec spec. shape for 1-ring μ-like events
– Correlation for far/near ratio btw energy bins are taken into account
3
taken into account
Far/Near ratio in oscillation Far/Near ratio in oscillation l i ( th d1)l i ( th d1)analysis (method1)analysis (method1)
Maximum Likelihood Method
)()()( fLfLfLL systshapenormtot ⋅⋅=Maximum Likelihood Method
)()()( fff systshapenormtot
systematics parameterssystematics parameters
),,,,,,( 116F/N nnEsksknQE ffffffff εΦ=spec
nQE/QEFar/near
( ffi i )εSK(efficiency)SK Enegry scale
O
4
Overall Norm ErrorFor Jun99 and Nov99-
Normalization termNormalization term
))(,( fNNPoissonL b=MC PfN )(
))(,( exp fNNPoissonL obsnorm
⋅= MCKT
oscMCSKobs
KT fNPfNNNexp )(
),(
∑ ⋅⋅ΔΦ⋅⋅=
Φji
SKijijji
MCSKNiFi
obs
fmPEffN ,
22/ )()2sin,()( εσθ
∑ ⋅⋅Φ⋅⋅=
Φji
KTijijji
MCKTi
KT fEfN
,)()( εσ
i: energy bin indexi: energy bin indexj: processes (=QE, nQE)
Spectrum meas in FD(f ) cancels first order
5
Spectrum meas. in FD(fΦi) cancels first orderbut far/near ratio fF/N does not.
EEννrecrec spectrum shape term for FC spectrum shape term for FC
1R1R1R1Rμμ∏
29
)( recEPL Total 29 events∏=
≡1
)(i
ecishape EPL Total 29 events
for Nov99~ data
P: reconstructed Eν distribution for 1Rμ (gen’ed by using MC)
( ) ( )truerec EEP Φ∫ Detector response from MC( ) ( )( ) ( ) ( )
ttruerec
QEtrueR
QEtrue
QE
trueSK
rec
EErEE
EEP
νννμ
ν
νν
εσ⎥⎤
⎢⎡ ⋅⋅
⋅Φ= ∫,1
Detector response from MC
( ) ( ) ( )( ) ( ) ( )
truetruerec
nQEtrueR
nQEtrue
nQEnQE
QEQEQE dEEErEEf ν
νννμ
ν
νννν
εσ ⎥⎥⎦⎢
⎢⎣ ⋅⋅+ ,
,1
( ) ( ) ( ) ( )22/ ,2sin mPRffE oscNF
MCFD
meastrueSK Δ⋅⋅Φ=Φ Φ θν
6
( ) ( ) ( ) ( )/ ,ff oscNFFDSK Φν
Systematic constraint termSystematic constraint termyy( ),
1, 2/exp nQEFD
TnQEsyst fMfL Δ⋅⋅Δ−≡ Φ
−Φ
( )( )1
/1//
2/
2/exp T
NFNFT
NF
fMf
fMf
ΔΔ×
Δ⋅⋅Δ−×−
− Far/near ratio
( )( ) ( )2
11211
26
26
1
2exp2exp
2/exp
nnnn
SKSKTSK
ff
fMf
σσεεε
−⋅−×
Δ⋅⋅Δ−×
( ) ( )( )22
111166
2/exp
pp
EskEsk
nnnn
f
ff
σΔ−× 1−≡Δ ff
MFD, Mπ, MSK: error matrix of syst. errors.ll f J 99σn6: overall norm. err. for Jun99 (=+0.80−0.68 evts)
σn11:overall norm. err. for Nov99~ (=5.34%)
7
n11σEsk: SK Enery scale error (3%)
QeustionsQeustions
• Central values of far/near ratio (relative to MC prediction)p )
fF/NiF/Ni• Correlation of far/near ratio btw. energy
bins (error matrix)bins (error matrix)
MMπ
8
A tool:Pion Monitor (PIMON)N(pπ, θπ) Neutrino flux Φ(Eν) at any distance
using only decay kinematics
R(Eν)≡ΦSK(Eν)/ΦFD(Eν)l f i i
To decay volume
200150
2750
Sphericalmirror
Top viewPion monitorGas volume
as a result of pion monitor
Blind
470
230
900
Foca
l le
ngth 34
64mm
Gas o u e~ Design on May 11,'98 ~
190
2448
Gas Cherenkov detector
From2nd Horn
910Beam window
275
2100
to avoid signal from 12GeV protons
332
Photo detector 20 PMTs
200
10
Beam view12GeV protonsinsensitive to pπ
<2GeV (Eν<1GeV)
9
600
110
9
( ν )PMT array
Strategy to obtain f error matrixStrategy to obtain fF/N, error matrixAbove 1GeV PIMON• Above 1GeV PIMON
• Below 1GeV Beam MC(Sanford-Wang parameterization fitted to previous data) validated by p p ) yPIMON measurement at >1GeV
• Error matrixMC part:
⎟⎞
⎜⎛ 0MC
1GeV
(2x2)
MC part:Fit previous pion production databelow ~2GeV/cmove paraemters within error
⎟⎟⎟
⎜⎜⎜ 0
1GeV(2x2) move paraemters within error
get error matrix
⎟⎟⎟
⎜⎜⎜ 0 PIMON
(4x4)
No correlation w/ PIMON part
10
⎟⎠
⎜⎝
(4x4)
Pion Monitor Resultsθ
pπ
θπ
w1 w2 w3 w4 …..: :
: :
11
Pion Monitor Result(relative weight)5)45
mra
d)beam axis
π+ θ
23
(*10
m
01
angl
e
-10
Pio
n
-3-2
-5-4
12
52 3 4 5 6 7Pion momentum (GeV/c)
Pion distribution to far/near ratio (i l t i )(incl. error matrix)
From PIMON fitting ( )SKFD W,φContribution to ν fluxfrom each p-θ bin
5
ad)
Relative weight Wi(i=1~50)( )ji Wφ
(by MC. To 1st order,depend only on decay kinematics &geometry
01234
angl
e (*
10m
ra
Eν
( )WjSKFD
iSKFD
i =Φ ∑50
,, φ FD,SK flux
-4-3-2-10
Pio
n a ( )
( ) ( )WWR FDi
SKii
jjii
ΦΦ=
∑=1
φ ,
Ratio as func. ofweights
-5-4
2 3 4 5 6 7Pion momentum (GeV/c)
50x50 error matrix on weightjdR
U =
( ) ( )iii weights
Dependence
πE50x50 error matrix on weight
iij dW
U =
TR π
of R on W (50x4 matrix)
Error matrixtransformation
13
ijE UEUE TR ⋅⋅= π
(4x4) (4x50) (50x50) (50x4)
transformationfrom π weight
far/near ratio
Other systematic errrosOther systematic errrostreated in matrix form as describedtreated in matrix form as described
1. move syst. parameter within error2. Check correlation btw energy bins
Rj
Ri
14
νμ spectra from Pion Monitor Measurement
15Agree with MC very well.
PIMON result for F/N ratio5
0.3x 10-5
tio
r ra
tPion monitor
Neutrino Beam Simulation
Good Agreement!0.2
/nea
rF
ar/
0.1Integratedabove 2.5GeV
0
16
0 0 1 2 3Eν(GeV)
Far/Near Error MatrixFar/Near Error Matrix“sqrt” of error matrix (%)
( )( ) ijij MM ⋅sign
0-0 5 0 5-1 1-1 5 1 5 2 2-2 5 2 50 0.5 0.5-1 1-1.5 1.5-2 2-2.5 2.5-
Beam MC PIMON17
Summary of systematic errors on total Summary of systematic errors on total # of events w/o osc# of events w/o osc# of events w/o osc.# of events w/o osc.
C t 80 1 t (%)Center: 80.1evts (%)
Jun99(4 55evts)
Total+1.0%−0 9%(4.55evts) 0.9%
Spectrum+0.6%−0.6%
Nov99~(75.5evts)
nQE/QE+0.5%−1.1%+4 9%
Far/Near+4.9%−5.0%
Norm 5.0%
Total +7.7%−6.7%
18
Summaryy• K2K uses pion distribution measured in-
situ(>1GeV) and beam MC(<1GeV) for spectrum extrapolation
• The beam MC is validated by the PIMON measurementsmeasurements
• Correlation of far/near ratio btw energy bins is taken into account (instead of linear sum =taken into account (instead of linear sum = 100% positive correlation
• Still far/near ratio is major source of systematic j yerror
• Expect precise data from HARP (measurement i A 26 ) M th k t HARPin Aug.26~). Many many thanks to HARP collaborators
19
Syst. error: far/near spectrum diff.y p
1600
1800
Typical OA beam(80mDV)
295km16tK2K case (MC)
FD(300m)
800
1000
1200
1400295km
8
12
16b
. uni FD(300m)
(xLSK2/LFD
2)
SK
200
400
600
280m4
8
Arb
SKLarge(~x2) effectaround peak!!
0.8
1
1.2
1.401.2
tio
0
0.2
0.4
0.6
0 0.5 1 1.5 2 2.5 30
0.4
0.8
Rat
00 0.5 1 1.5 2 2.5 3 3.5 4 4.5 5
Important not only for ν disappearance,
20
Important not only for νμ disappearance,but also for sig/BG estimation for νe search
POT
4.8×1019 POT for Analysis
200kA 250kA200kA 250kA
PIMON meas.
21
Stability of μ−Energy Spectrum
Muon energy spectrum stability1it
μ momentum (ms 25t FC,1-ring,μ)
0.8
0.9
1
99Nov
00Jan
00Feb
00Mar
arbi
trar
y un
it
800
1000 IDEntriesMean
1802 9770
711.3
0.5
0.6
0.700Mar
00May
00Jun
01Jan
01Feb
01Mar
600
800 MeanRMS
711.3 259.1
DATA2001
0.2
0.3
0.401Apr
200
400 DATA2000
Every
0
0.1
0.2
0 0.5 1 1.5 2 2.5 3E (GeV)
0
200
0 250 500 750 1000 1250 1500 1750 2000
ymonths
Muon Energy of
Eμ (GeV)
Pμ(GeV)
Muon Energy in
22
Muon Energy of MRD events
gyKT on ’01, ‘00
Exp’ed EExp’ed Eννrecrec spectrum for 1Rspectrum for 1Rμμ estimated by estimated by
FD tFD tFD measurementsFD measurements
23
PIMON in target stationg
24
25
K2K osc. analysis overviewνμ spectrum @ production
F
near/far extrapolationPIMONpπ-θπ dist
Near Far
oscillation probability Want to know this!!
neutrino interaction in water
d t t (1kt ifi) d t t (SK)detector responce(1kt, scifi) detector responce(SK)
FD observation1KTS ifi
SK observationtotal # of events
26
Scifi Eνrec spectrum shape(1ring μ-like events)
(1Rμ)