the very long baseline neutrino oscillations experiment presented to fcp05 neutrino session by
DESCRIPTION
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 - PowerPoint PPT PresentationTRANSCRIPT
The Very Long BaselineNeutrino Oscillations
Experiment
Presented toFCP05 Neutrino Session
byTom Kirk
Brookhaven National Laboratory
Nashville, TNMay 23, 2005
likelihood cut (100%signal retained)
Background from
CP+45o
Signal 700 evBkgs 2005 (1878 from +others) ( 127 from
e)
Signal
e backgroundo
CP+45
likelihood cut (~50%signal retained)
Effect of cut on likelihood
Erec Erec
Preliminary Preliminary
Signal/Background
Signal 321 evBkgs 169 (112 from +others) ( 57 from
e)
e CC for signal ; all e NC , e beam for background
Traditional Analysis
Chiaki Yanagisawa – SBUFebruary 28, 2005
Maximum Likelihood Method
Effect of cut on likelihoodCP +45o
Background
All
oCP-45
Erec
Erec
Preliminary Preliminary
S/B
Erec
Erec
Erec Erec
e CC for signal ; all e NC , e beam for backgrounds
100% 50%
40%
50%100%
40%
Chiaki Yanagisawa – SBUFebruary 28, 2005
Maximum Likelihood Method
Effect of cut on likelihood
CP +135o
Background
All
oCP-135
Erec
Erec
Preliminary Preliminary
S/B
Erec
Erec
Erec Erec
100% 100%50% 50%
40% 40%
e CC for signal ; all e NC , e beam for backgrounds
Chiaki Yanagisawa – SBUFebruary 28, 2005
Maximum Likelihood Method
T. Kirk May 3, 2005
Scientific Reach of Future Neutrino Oscillations Exps. Parameter T2K T2K2 Reactor Noa Noa2 VLBNO.
m322 4 4-
221sin2(223) 1.50.4- 0.4%0.20.5sin2(213) a >0.02 >0.01 >0.01 >0.01 >0.01 >0.01
m212 sin(212) b - - - - - 12 %
sign of (m322) c - - - possible yes yes
measure CP d
- ~20 - - ~2013N-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 1.5Baseline (km) 295 e 295 e 1 810 e 810 e >2500
Detector Cost ($M) exists ~1000 20 165 +200 400Beam Cost ($M) exists 500 exists 50 1000 400Ops. Cost ($M/10 yrs) 500 700 50 500 600 150/500 f
a detection of e , upper limit on or determination of sin2(213)b detection of e appearance, even if sin2(213) = 0; determine 23 angle ambiguity
c detection of the matter enhancement effect over the entire CP angle ranged measure the CP-violation phase CP in the lepton sector; Noa2 depends on T2K2 e beam is ‘off-axis’ from 0-degree target direction; f with/without RHIC operations
Both results needed toresolve ambiguities!
Best Bets
T. Kirk May 3, 2005
Comments on Neutrino Oscillations Experiments
• All parameters of neutrino oscillations can be measured in one experiment- the Very Long Baseline Neutrino Oscillation (VLBNO) at >2000 km- Use of a broadband Super Neutrino Beam at very long distances is the key- worries about 0 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-generation Nucleon Decay search- supernova and relic neutrino searches are also possible- a deep underground detector is required for these searches – NSF’s DUSEL!
• The CP-violation parameter CP is the most difficult parameter to determine
- matter effects interact with CP-violation effects- the CP-violation phase CP 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(223)