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Neutrino and Anti-Neutrino Cross Sections and CP Phase Measurement

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NuInt01, @ KEK (Tsukuba), Dec. 13, 2001. Neutrino and Anti-Neutrino Cross Sections and CP Phase Measurement. Yoshihisa OBAYASHI (KEK-IPNS). Introduction. MNS Matrix: WHY CP ? In the Quark Sector, CP is violated. Then, also in the Lepton Sector? → Leptogenesys - PowerPoint PPT Presentation
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Dec. 13, 2001 Yoshihisa OBAYASHI, NuInt01@KEK 1 Neutrino and Anti-Neutrino Cross Sections and CP Phase Measurement Yoshihisa OBAYASHI (KEK-IPNS) NuInt01, @ KEK (Tsukuba), Dec. 13, 2001
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Page 1: Neutrino and Anti-Neutrino Cross Sections and  CP Phase Measurement

Dec. 13, 2001 Yoshihisa OBAYASHI, NuInt01@KEK 1

Neutrino and Anti-Neutrino Cross Sections and

CP Phase Measurement

Yoshihisa OBAYASHI(KEK-IPNS)

NuInt01,@ KEK (Tsukuba),

Dec. 13, 2001

Page 2: Neutrino and Anti-Neutrino Cross Sections and  CP Phase Measurement

Dec. 13, 2001 Yoshihisa OBAYASHI, NuInt01@KEK 2

Introduction• MNS Matrix:

• WHY CP ?– In the Quark Sector, CP is violated. – Then, also in the Lepton Sector? → Leptogenesys– CP Measurement is a final goal of flavor physics

100

0

0

0

010

0

00

010

001

0

0

001

1212

1212

1313

1313

2323

2323

321

321

321

cs

sc

cs

sc

ecs

sc

UUU

UUU

UUU

Ui

eee

Page 3: Neutrino and Anti-Neutrino Cross Sections and  CP Phase Measurement

Dec. 13, 2001 Yoshihisa OBAYASHI, NuInt01@KEK 3

CP Phase Measurement• In the case of conventional (super) beam,

– – cf: NuFact:

• Oscillation Probability P(e):

CPV

sinsin

2sin

13

12212

E

LmPPPP

ACP

foraa ,

)()( ee PPCPV )()( ee PPCPV

Page 4: Neutrino and Anti-Neutrino Cross Sections and  CP Phase Measurement

Dec. 13, 2001 Yoshihisa OBAYASHI, NuInt01@KEK 4

Assumed Scenario on physics ~2010• → oscillation is established by Atm, LBL

– sin2223 ~ 1.0

– m223 ~ 3 x 10-3eV2

• LMA solution is established by Sol, KamLAND– sin2212 ~ 0.8

– m212 ~ 5 x 10-5eV2

• Finite 13 is found by JHF1 (, Atm)– sin2213 ~ 0.03

• MiniBooNE excluded LSND result• (Still) Unknown parameters:

– CP phase and sign of m2

Page 5: Neutrino and Anti-Neutrino Cross Sections and  CP Phase Measurement

Dec. 13, 2001 Yoshihisa OBAYASHI, NuInt01@KEK 5

→e oscillation probability

• Asymmetry can be seen at oscillation maximum ~0.7GeV

295km

Solid lines: w/ matter, Dashed lines: w/o matter

Page 6: Neutrino and Anti-Neutrino Cross Sections and  CP Phase Measurement

Dec. 13, 2001 Yoshihisa OBAYASHI, NuInt01@KEK 6

JHF-Kamioka Experiments

• Phase I: 2007(?)~201x– ~1MW 50GeV PS → 22.5kt detector (Super-Kamiokande)

• →x disapp., →e app., NC measurement

• Phase II: 201x(?)~202y(??)– ~4MW 50GeV PS → ~1Mt detector (Hyper-Kamiokande)

• CPV search, Proton Decay, . . .

295km KEK

Kamioka

Tokai

Hyper-K

SK

JHF

Page 7: Neutrino and Anti-Neutrino Cross Sections and  CP Phase Measurement

Dec. 13, 2001 Yoshihisa OBAYASHI, NuInt01@KEK 7

Beams

• Off Axis Beam• Switch and by changing

polarity of horn magnets• Neutrino Flux is almost the s

ame between and    beams

TargetHorns Decay Pipe

Far Det.

-15%@peak

1021POT/yr(1st phase)

Page 8: Neutrino and Anti-Neutrino Cross Sections and  CP Phase Measurement

Dec. 13, 2001 Yoshihisa OBAYASHI, NuInt01@KEK 8

Cross Sections

• • Quasi elastic interactions domi

nate below ~1GeV • •

)(3/1)(

)()( CCqeCCqe e )()( CCqeCCqe e

Page 9: Neutrino and Anti-Neutrino Cross Sections and  CP Phase Measurement

Dec. 13, 2001 Yoshihisa OBAYASHI, NuInt01@KEK 9

Expected Neutrino Events (w/o osc.)• # of events @ far det.

Beam

Beam

• is factor 3 smaller than – Running time of beam

need to be longer

• Wrong sign contribution is 3x3~10 times large for

beam– Cause fake CP asymmetry

)( )(

Page 10: Neutrino and Anti-Neutrino Cross Sections and  CP Phase Measurement

Dec. 13, 2001 Yoshihisa OBAYASHI, NuInt01@KEK 10

Selection for e appearance search• Select e CCqe interactions

– Vertex is in the fiducial volume– Single EM shower ring– No decay electron observed– Evis > 100MeV ( reject NC elastic )– Tight e/ separation

• see next slide

– Reconstructed E cut• 0.4 < E(GeV) < 1.2

Page 11: Neutrino and Anti-Neutrino Cross Sections and  CP Phase Measurement

Dec. 13, 2001 Yoshihisa OBAYASHI, NuInt01@KEK 11

Tight e/ separation• cose: from 0 tend to have a forward peak

• E(2)/E(1+2): Large for BG• Likelihood diff. between 1-ring and 2-rings• Invariant mass: Small for e

Page 12: Neutrino and Anti-Neutrino Cross Sections and  CP Phase Measurement

Dec. 13, 2001 Yoshihisa OBAYASHI, NuInt01@KEK 12

Expected Signal & Backgrounds

• By the present tools,– BG level is ~5x larger than expected CP asymmet

ry.– We need to achieve ~5% precision of BG subtrac

tion if we want to see 3 effect.

• ~90% of BG (50~60% of total BG) are from 0

Beame app.

Signal w/o CP

Effect of CP

Background in Hyper-K

total

699 -123 241 225 34 11 510

w/0 223 13 28 1 264

699 +120 238 164 342 210 953w/0 213 16 302 8 540

e e

• m122 = 5x10-5eV2

• m232 = 3x10-3eV2

• sin2213 = 0.03• sin2223 = 1• sin2212 = 0.8• = 45 deg• 5 x 1021 pot x 450 kt ()• 1.83 x 1022 x 450 kt pot () Off axis 2deg beam No matter effect considered

Page 13: Neutrino and Anti-Neutrino Cross Sections and  CP Phase Measurement

Dec. 13, 2001 Yoshihisa OBAYASHI, NuInt01@KEK 13

Cross Section (& Efficiency) Difference • We want to know

• Observable

• Then Asymmetry Parameter

• Only the difference of r,r between neutrino and anti neutrino appear in the asymmetry

rrPPNN

P eee

e

obse

e exp

ee

obse

e

NP

exp

rrr

rrr

PPP

PPPP

rrPrrPrrPrrP

PP

PPA

ee

eeCP

22

2

'''2

1''''

''''

)()(

)()(

Page 14: Neutrino and Anti-Neutrino Cross Sections and  CP Phase Measurement

Dec. 13, 2001 Yoshihisa OBAYASHI, NuInt01@KEK 14

Cross Section Difference

• CCqe cross section ratio of e

/

– Difference between neutrino and anti-neutrino is at most 5% within the energy window

~5%

Page 15: Neutrino and Anti-Neutrino Cross Sections and  CP Phase Measurement

Dec. 13, 2001 Yoshihisa OBAYASHI, NuInt01@KEK 15

CP Measurement

• Matter effect becomes larger for large 13

• Black circles represent 3 contour for phase 2 of JHF running

Page 16: Neutrino and Anti-Neutrino Cross Sections and  CP Phase Measurement

Dec. 13, 2001 Yoshihisa OBAYASHI, NuInt01@KEK 16

BG subtraction vs Sensitivity• Sensitivity strongly depends on sys

tematic uncertainty of BG subtraction.

• If BG sys. = 2%:– sin2213=0.01→sin>0.55(33o)

– large 13→sin>0.25(14o)

• Sensitivity improves with better BG rejection

Better BG rejection and smaller uncertainty in BG subtraction are strongly preferred in the CP measurement

Chooz excluded@m31~3x10-3eV2

JHF1 cannot discover 13

(3)

Page 17: Neutrino and Anti-Neutrino Cross Sections and  CP Phase Measurement

Dec. 13, 2001 Yoshihisa OBAYASHI, NuInt01@KEK 17

Items for the Improvement of Sensitivity• ~90% of BG are from 0

– Improve the hardware (Hyper-K)• Timing resolution, Light scattering and reflection, Segment . . .

– Improve the software• Reconstruction algorithm, . . .

– Measure NC 0 rate@ Front detector• Energy scan with Narrow Band Beam

• ~50% of BG are from e

– Measure e/ratio @ Front detector– Narrower energy window

• Improvement of energy resolution

• ~50% of BG are from high energy tail of beam– Tune the beam line and reduce HE tail

• Measurement of wrong sign contamination– Magnetized detector?– Recoiled neutron detector?

Page 18: Neutrino and Anti-Neutrino Cross Sections and  CP Phase Measurement

Dec. 13, 2001 Yoshihisa OBAYASHI, NuInt01@KEK 18

Conclusion• Phase 2 of JHF-Kamioka experiment aims at measuring

CP violation• Better BG rejection and smaller uncertainty in BG subtr

action are strongly preferred in the CP measurement• Let's Complete MNS matrix!


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