J-PARCニュートリノ の 将来計画 - KEK

Feb.28,2011
機構シンポ
J-PARCニュートリノ
の
将来計画
Takashi Kobayashi
IPNS/KEK
1
目次
素粒子物理道路計画の中のニュートリノ道路
 現在位置と目標地点の確認
 道路計画:幹線



道路計画:支線


θ13の決定(T2K)CP非保存(+陽子崩壊)探索
ニュートリノの性質の徹底解明驚き?
まとめ
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Neutrino in particle physics

Neutrinos have still lots of mystery, for example

Extremely small (&unknown) mass not yet understood




Flavor relations




Not yet fully known
Looks very much different from quark structure?
Why? May contain some hint to unification?
CP is violated also in lepton sector?


One promising scenario: See-Saw mechanism (Yanagida 1974)
Existence of very large mass Majorana neutrino may explain small neutrino
mass
Neutrino may be window to see very high energy scale physics?
Could provide clue to the mystery of matter dominated universe
Big expectation to find breakthrough to answer the
fundamental questions in particle physics, such as, what is
the unified theory?, origin of mass?, origin of matter in the
universe? by attacking and exploring the mystery of the
neutrino one by one
3
大雑把にいうと
加速器ニュートリノ物理は~10%効果を探す(測
る) 山師的時代から~1%の高感度精密測定の
時代へ。
 そのために欠くべからざる要素は

大強度ビーム


O(100kW)の物理は長年BNL,FNAL,CERNで散々やられ
てきた
高性能検出器

4
現在位置と目標地点の確認
5
ニュートリノの3世代混合
フレーバー固有状態
νe
νµ
ντ
U PMNS
ν e  ユニタリー行列 ν 1 
 
 
ν µ  = U PMNSν 2 
ν 
ν 
 τ
 3
0
1

=  0 + c23
0 − s
23

大気、加速器
0  + c13

+ s23  0
+ c23  − s13eiδ
m1
質量固有状態
m2
m3
0 + s13e − iδ  + c12

1
0  − s12
0
+ c13  0
(大気)、加速器
+ s12
+ c12
0
0

0
1 
太陽、原子炉
ニュートリノ振動をつかさどる6個のパラメータ
θ12, θ23,
θ13,
δ
∆m122, ∆m232, ∆m132
c ij = cos(θ ij ),
s ij = sin(θ ij )
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What’s are known & unknown?
Sol&Reactor
•θ12~34o
•∆m122~0.00008eV2
Atm+Acc
•θ23~45o
•∆m232~0.0024eV2
Unknown
•θ13<10o
• (∆m132~∆m232)?
•δ ???
νe??
ν3
ν2
OR
ν1
どっち??
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•クォークにくらべまだまだ大雑把
•クォークと大きく異なる構造(大きな混合)
青:PMNS
赤:CKM
1.20±0.80 (7%)
0.201±0.011 (5%)
(90%CL)
2.38±0.06 (2.5%)
•θ13, δ未知
<10.5°
????????????????????????????
34.4±1.0 (3%)
13.04±0.05 (0.4%)
Angles in mixing matrix (CKM,PMNS)
PDG, Concha Gonzalez-Garcia(NOW2010) 8
Unkonwn in neutrinos

The last unknown mixing θ13. 3 flavor mixing picture?
First indispensable step to go CPV search
T2K experiment
Reactor experiments


CP is violated in lepton sector?
Could provide hint for matter-anti-matter asymmetry in the
unverse
Future Acclerator neutrino experiments



Mass hierarchy
 Future Acclerator neutrino experiments
Absolute mass
Precision measurement of Tritium beta decay spectrum
Neutrino-less double beta decay

Neutrino is Majorana ? Dirac?
Majorana neutrino: Neutrino = Anti-Neutrino
 Neutrino-less double beta decay

9

道路計画:幹線

θ13の決定(T2K)CP非保存(+陽子崩壊)探索
10
Next most important step: θ13. Why?
CPV & sign(∆m2) will be probed thru νe appearance in accel LBL
Leading
CP-odd
δ−δ, a-a for ν µ → ν e
+ other terms..

CP-odd term
∝ sin δ ⋅ s12 ⋅ s23 ⋅ s13
ρ
  E 
⋅

3  
 [g cm ]   [GeV] 
Matter eff.: a = 7.56 ×10 −5 [eV 2 ] ⋅ 
(where sinθ12~0.5, sinθ23~0.7, sinθ13<0.2)
The size of θ13
Decide future dir.!
1999日本(戸塚+西川)が
世界で初めて着目T2K提案
Takashi Kobayashi (KEK), PAC07
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T2K (Tokai to Kamioka) experiment



High intensity νµ beam from
J-PARC MR to SuperKamiokande @ 295km
Discovery of νe appearance
 Determine θ13
Precise meas. of νµ
disappearance  θ23, ∆m232
Near ν detectors
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Data taking status
135kW(9x1013ppp)
125kW
2010a
100kW
50kW
3.7x1013ppp
2010b




Stable data taking started in Jan. 2010
~135kW stable operation achieved (Feb 14, 2011~)
1.2x1020p’s (59kWx107s) delivered (Feb.21, 2011)
We thank CONTINUOUS GREAT EFFORT of accelerator team
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Mid term goal
By summer 2014
1000[kWx1E7s]
速やかな大強度化必須
Now
0.014
1000[kWx1E7s]
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Quest for the Origin of Matter Dominated Universe
One of the Main Subject of the
KEK Roadmap
T2K
(2009~)
Discovery of
the νe Appearance
Neutrino
Intensity Improvement
Huge Detector R&D
Establish
Huge Detector Construction of
Huge Detector
Technology
v
Water Cherenkov
Liquid Ar TPC
Discovery of
Lepton CP Violation
Proton Decay
Scenario 1
J-PARC to Okinoshima
P32 proposal (Lar TPC R&D)
Recommended by J-PARC PAC
(Jan 2010), arXiv:0804.2111
Scenario 1
J-PARC to Okinoshima
P32 proposal (Lar TPC R&D)
Recommended by J-PARC PAC
(Jan 2010), arXiv:0804.2111
J-PARC to Okinoshima
•Cover 1st and 2nd Maximum
•Neutrino Run Only 5Years×1.66MW
•100kt Liq. Ar TPC
-Good Energy resolution/reconstruction ability
-Good e/π0discrimination
•Keeping Reasonable Statistics
νeSpectrum
sin22θ13=0.03,Normal Hierarchy
δ=0°
δ=90°
δ=180°
δ=270°
CP Measurement Potential
3σ
Beam νe
Background
Okinoshima
658km
0.8deg. almost On-axis
P32 proposal (LAr TPC R&D)
Encouraged by J-PARC PAC (Jan 2010), NP08,
arXiv:0804.2111
Liquid Argon TPC R&D (T32)
250L TPC beam exposure in
Oct/Nov, 2010
ETHZ
Iwate
KEK
Waseda


Largest K and π samples ever accumulated for Liquid Argon TPC
Results will be presented in PAC in July 2011
19
J-PARC-Okinoshima feasibility studies
(Some examples)
Site visit
Potential LiqAr supply
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実現のためには。
大強度(>1MW)達成
着実な検出器開発継続

21

道路計画:支線

ニュートリノの性質の徹底解明驚き?
22
Other important physics in LBL
experiment (J-PARC  SK)

Precision measurement of numu disappearance

Precise measurement of spectrum shape


T2K proposal (3750kWx1E7sec)


T2K proposal (3750kWx1E7sec)


δ(∆m232)~1x10-4eV2, δ(sin22θ23)~1%
Sterile neutrino search


Really (only) oscillation??? No other exotic mode????
O(100) neutral current enhanced sample
Anti-neutrino measurement (appearance and
disappearance)
Precision measurement of θ13
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Precision measurement of numu
Disappearance




Really follow oscillation pattern??
Mixing really maximal???
Same for anti-nu???
T2K proposal (3750kWx1E7sec)

δ(∆m232)~1x10-4eV2,
δ(sin22θ23)~1%
Need Power!!!
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Sterile neutrino search in T2K



100% νµ  νs disfavored by SK
Probe small mixing to sterile
Select NC enhanced sample


From T2K proposal
2 e-like ring, no decay electron
Nevt = 255 vs 104 with
“750kWx5yr”
From T2K proposal
Need Power!!!
25
νe appearance search/measurement
in anti-neutrino mode



Once finite θ13 is firmly
established, move to antineutrino
If no signal is observed in
neutrino mode (θ13 is small),
we need to move to antineutrino at some optimized
timing.
 Some early hint on CPV??
26
νµ/νµ # of CC int.
(Very old sim(2001) w/ 50GeV)
νµ beam
1021pot/yr
~800kWx107sec
Need Power!!!
νµ beam
right sign
wrong sign
 # of int. for νµ is factor ~3 smaller than νµ due to cross section.
大強度
(Over several 100kW)
実現不可欠
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Existing puzzles
= Yet another physics opportunities
Example
 LSND/MiniBooNE anomaly
2
2
 Sterile neutrino at ∆m ~2eV ??
 (Weinberg angle?)
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Another (sterile) neutrino at large ∆m2 ???
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Another (sterile) neutrino at large ∆m2 ???
Need to be concluded!
 ∆m2~eV2, sin22θ~10-3


 L(m)/E(MeV) ~ 1.2  740m @ 600MeV
High statistics high sensitivity short baseline νe
appearance experiment
 Suited at J-PARC
 To decisively conclude

High PID performance detector LiqAr? Liq Scin?
 Energy spectrum measurement
 Precise normalization

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Reactor anomaly ??






Recently reactor flux calculation is refined
Flux prediction slightly increased
Results in almost all experiment observation more
smaller than prediction
Other disappearance from anti-νe to sterile neutrino?
∆m2~2eV2
To conclude in accelerator experiment





Short baseline ne disappearance experiment
~17% deficit expected
Very high PID performance required (because nm
interaction dominate)
High intensity needed! (νe is ~1% of νµ)
Precise normalization of νe prediction needed!


Near/far configuration??
Dichromatic beam??
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The Reactor Antineutrino Anomaly
Best fit:
∆m2=2.35±0.1eV2
sin22θ=0.165±0.04
arXiv:submit/0179257
[hep-ex] 14 Jan 2011
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大強度
実現不可欠
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Summary

Big goal
Search for CPV and proton decay
w/
 >MW beam power machine
 Huge/high sensitivity detector



To realize, need




Discovery of non-zero θ13
Accelerator power upgrade
step-by-step sure R&D of detector
Because neutrino has many unknowns, various
EXCITING physics exists along the road toward
realizing the big goal


100kt LiqAr TPC at Okinoshima is seriously being investigated
Gold may be buried???
All these can only be realized with HIGH POWER JPARC (& GOOD IDEA!)
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