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July 4, 2002 νFact02 @Imperial College London Translation from Near to Far t K2K at K2K T Kobayashi T.Kobayashi IPNS, KEK for K2K beam monitor group for K2K beam monitor group (K.Nishikawa, T.Hasegawa, T.Inagaki, T.Maruyama, T.Nakaya, ....) Especially for T.Maruyama(KEK Chicago) who played major role in PIMON i / / l i 1 construction/measurement/analysis

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Page 1: July 4, 2002 νFact02 @Imperial College London Translation from …jnusrv01.kek.jp/.../talks/nufact02/nufact02.kobayashi2.pdf · 2008. 12. 8. · Microsoft PowerPoint - nufact02.kobayashi2.ppt

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

Page 2: July 4, 2002 νFact02 @Imperial College London Translation from …jnusrv01.kek.jp/.../talks/nufact02/nufact02.kobayashi2.pdf · 2008. 12. 8. · Microsoft PowerPoint - nufact02.kobayashi2.ppt

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

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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

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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-

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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.

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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

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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%)

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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

Page 9: July 4, 2002 νFact02 @Imperial College London Translation from …jnusrv01.kek.jp/.../talks/nufact02/nufact02.kobayashi2.pdf · 2008. 12. 8. · Microsoft PowerPoint - nufact02.kobayashi2.ppt

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

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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)

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Pion Monitor Resultsθ

θπ

w1 w2 w3 w4 …..: :

: :

11

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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)

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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

( )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

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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

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νμ spectra from Pion Monitor Measurement

15Agree with MC very well.

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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)

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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

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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

Page 19: July 4, 2002 νFact02 @Imperial College London Translation from …jnusrv01.kek.jp/.../talks/nufact02/nufact02.kobayashi2.pdf · 2008. 12. 8. · Microsoft PowerPoint - nufact02.kobayashi2.ppt

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

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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

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POT

4.8×1019 POT for Analysis

200kA 250kA200kA 250kA

PIMON meas.

21

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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

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Exp’ed EExp’ed Eννrecrec spectrum for 1Rspectrum for 1Rμμ estimated by estimated by

FD tFD tFD measurementsFD measurements

23

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PIMON in target stationg

24

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25

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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)