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The Very Long Baseline Neutrino Oscillations Experiment Presented to FCP05 Neutrino Session by Tom Kirk Brookhaven National Laboratory Nashville, TN May 23, 2005. Chiaki Yanagisawa – SBU February 28, 2005. Signal/Background. n e CC for signal ; all n m,t, e NC , n e beam
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The Very Long Baseline Neutrino Oscillations Experiment Presented to FCP05 Neutrino Session by Tom Kirk Brookhaven National Laboratory Nashville, TN May 23, 2005
Chiaki Yanagisawa – SBU February 28, 2005 Signal/Background • ne CC for signal ; all nm,t,e NC , ne beam • for background Effect of cut on D likelihood No Dlikelihood cut (100%signal retained) Dlikelihood cut (~50%signal retained) Traditional Analysis Maximum Likelihood Method Preliminary Preliminary Background from p0 o CP+45 o CP+45 ne background Signal Erec Erec Signal 700 ev Bkgs 2005 (1878 from p 0+others) ( 127 from ne) Signal 321 ev Bkgs 169 (112 from p 0+others) ( 57 from ne)
Maximum Likelihood Method S/B • ne CC for signal ; all nm,t,e NC , ne beam • for backgrounds Effect of cut on likelihood o CP +45o CP-45 Preliminary Preliminary 50% 100% 100% 50% All Background Erec Erec Erec Erec 40% 40% Erec Erec Chiaki Yanagisawa – SBU February 28, 2005
Maximum Likelihood Method S/B • ne CC for signal ; all nm,t,e NC , ne beam • for backgrounds Effect of cut on likelihood o CP +135o CP-135 Preliminary Preliminary 100% 50% 100% 50% All Background Erec Erec Erec Erec 40% 40% Erec Erec Chiaki Yanagisawa – SBU February 28, 2005
Best Bets Scientific Reach of Future Neutrino Oscillations Exps. Parameter T2K T2K2 Reactor Nona Nona2 VLBNO. Dm322 4 % 4 % - 2 % 2 % 1 % sin2(2q23) 1.5 % 0.4 % - 0.4% 0.2 % 0.5 % sin2(2q13) a >0.02 >0.01 >0.01 >0.01 >0.01 >0.01 Dm212 sin(2q12) b - - - - - 12 % sign of (Dm322) c - - - possible yes yes measure dCP d- ~20 - - ~20 13 N-decay gain x1 x20 --- x8 Detector (Ktons) 50 1000 20 30 30+50 400 Beam Power (MW) 0.74 4.0 14000 0.4 2.0 1.5 Baseline (km) 295 e 295 e 1 810 e 810 e >2500 Detector Cost ($M) exists ~1000 20 165 +200 400 Beam Cost ($M) exists 500 exists 50 1000 400 Ops. Cost ($M/10 yrs) 500 700 50 500 600 150/500 f a detection of nm ne , upper limit on or determination of sin2(2q13) bdetection of nm ne appearance, even if sin2(2q13) = 0; determine q23 angle ambiguity cdetection of the matter enhancement effect over the entire dCP angle range d measure the CP-violation phase dCP in the lepton sector; Nona2 depends on T2K2 ebeam is ‘off-axis’ from 0-degree target direction; fwith/without RHIC operations Both results needed to resolve ambiguities! T. Kirk May 3, 2005
Comments on Neutrino Oscillations Experiments •Allparameters of neutrino oscillations can be measured in one experiment - the Very Long Baseline Neutrino Oscillation (VLBNO) at >2000 km - Use of a broadbandSuper Neutrino Beam at very long distances is the key - worries about p0 channel background have been successfully addressed - the VLBNO cost is comparable to or lower than less comprehensive methods •The massive LBNO detector empowers additional forefront physics topics - a powerful next-generationNucleon Decaysearch - supernova and relic neutrino searches are also possible - a deep underground detector is required for these searches – NSF’s DUSEL! • The CP-violation parameter dCP is the most difficult parameter to determine - matter effects interact with CP-violation effects - the CP-violation phase dCP has distinct effects over the full 360º range •Off-axis beam method requires multiple distances and detectors - all experiments will require of order 10 Snomass years of running - each proposed detector will achieve good statistics for most parameters • All measured oscillation parameters will be limited to ~1% precision by systematic errors except sin2(2q23) T. Kirk May 3, 2005