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Precision measurement of mixing angles and CP Precision measurement of mixing angles and CP

Precision measurement of mixing angles and CP - PowerPoint Presentation

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Precision measurement of mixing angles and CP - PPT Presentation

Hisakazu Minakata PUCRio PUCRio where June 13 2013 RENO50KNRCSeoul Maracana June 13 2013 RENO50KNRCSeoul All the angles are measured lepton CP phase d left n a U a i ID: 760199

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Slide1

Precision measurement of mixing angles and CP

Hisakazu MinakataPUC-Rio

Slide2

PUC-Rio, where?

June 13, 2013

RENO50@KNRC-Seoul

Maracana

Slide3

June 13, 2013

RENO50@KNRC-Seoul

All the angles are measured !lepton CP phase d left

na=Uai ni

solar+KamLAND

SK-atm+MINOS+T2K

T2K-MINOS-DC-DB-RENO

Slide4

June 13, 2013

RENO50@KNRC-Seoul

q12

Slide5

q12 has been measured by solar and KamLAND experiments

June 13, 2013

RENO50@KNRC-Seoul

KamLAND

Mar. 2013

Slide6

q12

sin2q12 = 0.304 +/- 0.013Error of sin2q12 = 4.3%Error of Dm221 = 2.4%

June 13, 2013

RENO50@KNRC-Seoul

KamLAND

Mar.2013

Slide7

June 13, 2013

RENO50@KNRC-Seoul

How to improve q12?

Slide8

SADO idea/proposal (July 2004)

“SADO” = Several tens of km Antineutrino DetectOr Basic idea: 1st oscillation minima of Pee is the right place for precision measurement of q12

June 13, 2013

RENO50@KNRC-Seoul

HM-

Nunokawa-

Teves

-Zukanovich

Funchal

,

ArXiv

0407326 PRD(2005)

Slide9

Optimal distance estimated as 50-60 km

June 13, 2013

RENO50@KNRC-Seoul

Without geo-nu 40km would be fine

Slide10

SADO-vs KamLAND sensitivity

June 13, 2013

RENO50@KNRC-Seoul

SADO 3

s sensitivity ~ KamLAND 1s sensitivity

Slide11

June 13, 2013

RENO50@KNRC-Seoul

Solar+KamLAND and SADO are good competitors

Tuned reactor may have better sensitivity with long-run because tuning L is powerful

2% (1

s) in sin2q12 reachable with systematic error of 4%

Bahcall-Pena-Garay

Slide at World Physics Summit @Galapagos, June 22-25, 2006

Slide12

Quark-Lepton Complementarity

June 13, 2013

RENO50@KNRC-Seoul

Bi-maximal mixing from

neutrinos

Predicted value of

q13 in this model agrees well with experiments !  Large q13 natural in QLC

HM-A.Smirnov PRD 2004

QLC is based on observation: q12 + qC = p/4

Slide13

Impressive to see the real proposals today!

June 13, 2013

RENO50@KNRC-Seoul

Sin

2

q12 error: RENO ~ 1% (K.K.Joo) Daya Bay II 0.63% claimed! (Yifang Wang), Talk both at ICRR)

Daya

Bay II

Slide14

June 13, 2013

RENO50@KNRC-Seoul

q13

Slide15

q13: RENO

If added quadrature, sin22q13 = 0.1 +/- 0.018sin2q13 = 0.0257 +/- 0.0048Error of sin2q13 = 19%

June 13, 2013

RENO50@KNRC-Seoul

Slide16

q13: Daya Bay

If added quadrature, sin22q13 = 0.089 +/- 0.011sin2q13 = 0.0228 +/- 0.0029Error of sin2q13 = 13%

June 13, 2013

RENO50@KNRC-Seoul

Slide17

How to improve q13?

Continued running of reactor experimentsCan accelerator measurement supersade reactor q13 accuracy? If yes, when?What is the ultimate error of q13 ? If sin22q13 = 0.1 +/- 0.005  5% error for sin2q13 Is 2-3% error achievable for sin2q13 ? Neutrino factory?Reactor + identical 2 detector appears to be practically the best way

June 13, 2013

RENO50@KNRC-Seoul

Memory of Lev

Mikaelyan

@

Kurchatov

Inst.

Slide18

Ultimate error of q13?

June 13, 2013

RENO50@KNRC-Seoul

Daya

Bay ultimate (syst. only)

P. Coloma

etal. JHEP12

D

(sin

2

q

) / sin

2

q

= (1.6-2.0)

(

Dq

/

q

)

Slide19

June 13, 2013

RENO50@KNRC-Seoul

Least accurately measured angle q23

Slide20

q23: mixing angle with the largest error of 10-20% level

June 13, 2013

RENO50@KNRC-Seoul

Concha

etal

. JHEP 2012

Slide21

Error of q23 is large because ..

Jacobian effect:Octant degeneracy + exp. uncertainty  merging of clone solution to true one

June 13, 2013

RENO50@KNRC-Seoul

HM-

Sonoyama-Sugiyama PRD 2004 

Slide22

June 13, 2013

RENO50@KNRC-Seoul

How to measure q23 accurately?

Slide23

June 13, 2013

RENO50@KNRC-Seoul

Use solar term or R+A to solve q23 octant degeneracy

T2K-II + phase II reactor

T2KK

d

=0 assumed

sin

2

2

q13

sin2 q23

sin2 2q13

> 3

s

2~3s

T2KK 2

s

(rough)

T2KK has better sensitivity

at sin

2 2q13 < 0.06~0.07 .

hep-ph/0601258

Hiraide etal. PRD2006

Kajita

etal

. PRD2007

Slide24

Use atmospheric neutrino to probe solar n oscillation

June 13, 2013

RENO50@KNRC-Seoul

Hyper-K LOI :

ArXiv 1109.3262

Barger

etal

.

PRL 2012

Slide25

June 13, 2013

RENO50@KNRC-Seoul

Toward measuring d

Slide26

How to measure CP

nm superbeam appears to be the prime candidateT2KK CP sensitivity ~ T2HK CP sensitivity

June 13, 2013

RENO50@KNRC-Seoul

Slide27

Determination of d in correlation with q13?

So far CP d measurement has been discussed in a framework of simultaneous d – q13 determination  intrinsic d - q13 degeneracy enriched with unknown mass hierarchyRight framework? NO!  Better setting: simultaneous d – q23 determination

June 13, 2013

RENO50@KNRC-Seoul

People were focused

on another cosmos ..

Slide28

Why q23 relevant for CP?

In precision era for CP the errors of d will be dominated by uncertainty of s223D sind =D cosd =

June 13, 2013

RENO50@KNRC-Seoul

For a given set of (P, P-bar) with finite error, a change in s

2

23 can be compensated by adjusting d

Error formula for CP d h = order unity

HM-Parke,

ArXiv

1303.6178

Slide29

June 13, 2013

RENO50@KNRC-Seoul

A new method for q23 and d

Slide30

Simultaneous q23– d determination

June 13, 2013

RENO50@KNRC-Seoul

For a given set of (P, P-bar) there are 2x2=4 solutions of

q23 and d

What you need is to switch q13  q23 everything goes through as in (q13-d) case

Slide31

1st Oscillation maximum

June 13, 2013

RENO50@KNRC-Seoul

Things are much simpler in oscillation maximum

Slide32

1st Oscillation maximum (continued)

June 13, 2013

RENO50@KNRC-Seoul

HM-Parke,

ArXiv

1303.6178

Slide33

Use ne appearance channel

simultaneous d – q23 determination by ne and ne-bar appearance channelsq23 intrinsic degeneracy

June 13, 2013

RENO50@KNRC-Seoul

Slide34

Breaking q23– d degeneracy

June 13, 2013

RENO50@KNRC-Seoul

At 1

st

VOM

Spectrum information must solve the degeneracy!

Off 1st VOM

Hyper-K: DE= +/- 10%:

LBNE

:

D

E= +/- 20%:

Slide35

2nd vacuum oscillation maximum

June 13, 2013

RENO50@KNRC-Seoul

At 2nd VOM, D=3p/2

D

E= +/- 3%:

M

ovement of clone solution is more prominent at 2

nd

VOM

Slide36

Conclusion

Current status of mixing angle measurement outlinedSome ideas seeking for better precision discussed Further improvement appear realistic for q12 (new projects) and q13 (continue running), but may not be for q23 at near maximal, because…Fortunately, if you measure d, then you automatically get q23!

June 13, 2013

RENO50@KNRC-Seoul