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TAUP07, Sep.2007, Sendai. Updating the future neutrino oscillation experiment With the Kamioka-Korea 2 detector setup. Takaaki Kajita, ICRR, Univ. of Tokyo. ◆Introduction ◆ T2KK @TAUP05 ◆Updating T2KK - L dependence, - Higher energy option, - Octant of q 23 , ◆Summary.
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TAUP07, Sep.2007, Sendai Updating the future neutrino oscillation experiment With the Kamioka-Korea 2 detector setup Takaaki Kajita, ICRR, Univ. of Tokyo ◆Introduction ◆T2KK @TAUP05 ◆Updating T2KK - L dependence,- Higher energy option, - Octant of q23, ◆Summary
Introduction sin2q12, sin22q23, Dm122, |=Dm232|・・・・ Already measured. Let’s assume that non-zero q13 will be observed by the next generation oscillation experiments. If q23 ≠p/4, is it >p/4 or <p/4 ? q13 Sign of Dm232 nenmnt or n3 nenmnt n3 n2 n1 or n3 CP ? How much will Kamioka-Korea 2 detector setup (T2KK) contribute to these measurements?
Detector in Korea ? T2KK @TAUP05
Possible experimental setup 0.27Mton 0.27Mton 2.5 deg. off axis (or smaller off-axis Angle) 2.5 deg. off axis Distance from the target (km) JPARC 0754MW 2.5deg.off-axis beam @Kamioka Fig. from Senda NP04 Off-axis angle
Osc. probability in Kamioka and Korea sin22q13=0.05 BG & efficiency: almost identical both 2.5 deg. off axis beam
Expected sensitivity hep-ph/0504026 Total mass of the detectors = 0.54 Mton fid. mass 4 years neutrino beam + 4 years anti-neutrino beam Mass hierarchy CP violation (sind≠0) 3 s (thick) 2 s (thin)
Update (1)- 1050km: a special baseline ? - K.Okumura, 2nd T2KK workshop, Seoul 2006 2.5 degree off-axis beam with L between 1000km and 1250km is available. Checked if the sensitivity depends strongly on the baseline length. sin22q13 Kam only L=1000km L=1050km Sensitivity to mass hierarchy (True = normal hierarchy) L=1100km L=1150km The sensitivity does not depend strongly on L ! L=1200km L=1250km d 3s sensitivity
Update (2): higher energy option Motivation: Mass hierarchy arXiv:0705.4396 3(black) 3 s (thick) T2KK ‘s sensitivity on mass hierarchy is still limited compared with the US studies… Higher energy better ?
Higher energy beam Flux (arb. unit) 1.0 to 2.5 degree off axis beam available in Korea. P(nmne) Energy Dependent Maximum Likelihood Analysis En (GeV)
Signal and BG for various off-axis beams Korea Kamioka 1.5 degree 1.0 degree 2.5 degree signal signal BG BG sin2(2q13)=0.1 d=1/2p 4 year neutrino run 4MW beam 2.5 degree 2.0 degree Smaller off-axis angle: Low E BG more serious. (2nd osc. Max. difficult to see.) But larger matter effect at the 1st osc. Max..
3s sensitivities for various OA angles F.Dufour, 2nd T2KK workshop, July 2006, Seoul (Updated) Mass hierarchy CP violation Preliminary 3 Could be slightly too optimistic for OA angle less than 2.5 degrees (The syst errors are assumed to be fully correlated between 2 detectors) Kam only (OA2.5) Kam + Korea OA1.0 Kam + Korea OA1.5 Kam + Korea OA2.0 Kam + Korea OA2.5 Mass hierarchy: OA1.0 @Korea gives the best sensitivity CP violation: Sensitivity depends weekly on the beam option
Update (3):Octant ambiguity of q23 In the previous study, maximal q23 mixing (q23=p/4) was assumed. However, q23 might not be p/4. In this case, there should be additional ambiguity in the parameter measurements (especially in that of sin2q13) due to the ambiguity in the octant of q23 (i.e., q23 >45 or <45 deg.). It will be very nice if the same setup can solve the octant ambiguity of q23. Resolving 8 fold parameter degeneracy in T2KK
Oscillation probabilities and the signal P(nmne) by the solar Dm2 is proportional to sin22q12・cos2q23 Solar oscillation effect visible in a very long baseline (or very large L/E) experiment. sin22q12・cos2q23 effect visible Atm. + CP terms BG events Solar term ○sin2 q23= 0.4, sin2 2q13= 0.01 ●sin2 q23= 0.6, sin2 2q13= 0.0067 (sin2q23・sin22q13 is equal in the two cases.) Dm2: positive, d=p3/4
sin22q13 Sensitivity to octant of q23 sin22q23=0.96 hep-ph/0609286 OA 2.5 degree for both Kamioka and Korea sin22q23=0.99 2s 3s Octant ambiguity of q23 can be resolved at 2sif sin22q23 < ~0.97 (almost independent of the value of sin22q13 and mass hierarchy). Could resolve the 8 hold degeneracy of the oscillation parameters.
Discussing T2KK more Sep.30 and Oct. 1 Univ. of Tokyo Your participation and contribution are most welcome! http://www-rccn.icrr.u-tokyo.ac.jp/workshop/T2KK07/
Summary If non-zero q13 is observed…. • We hope to proceed to the next phase of experiment with higher power beam and larger detector(s). • Goals: discovery of leptonic CP violation, and determination of mass hierarchy and octant of q23. (+ Various non-LBL physics). • T2KK is one of the serious possibilities. • We will continue the studies.