long baseline neutrino oscillation projects · minos opera ikarus experiments coming not so soon...
TRANSCRIPT
Long Baseline Neutrino Oscillation Projects
Alfons Weber 18 January 2004
RAL/CCLRC
Jan 2005 2
Overview
Current statussee S. King’s talkglobal fits
Experiments coming soonMINOSOPERAIKARUS
Experiments coming not so soonT2KNOvA
Jan 2005 3
Results of Global Fits
Jan 2005 4
The MINOS Experiment
• NuMI beam to Soudan in MN (distance 735 km)
• Sagitta:10 km• >1 km wide at destination
Jan 2005 5
The NuMI Beam“Neutrinos at the Main Injector”
•NuMI has 400kW primary proton beam
120 GeV8.67 µsec spill1.9 sec rep rate5 Booster batches
(2.5×1013 prot/spill)
p beam
Pion beam
Jan 2005 6
νµ CC Energy AnalysisSelect νµ charge current events
Energy resolution:
Compare energy spectrum in near and far detectorMeasure ∆m2 and sin22θ
hEEE += µν
range, B field calorimetric
EEE
pp
hh /%60/
%10/
=∆
=∆ µµ
∆m2
sin22θ
Jan 2005 7
MINOS SensitivityMuon Disappearance Measurement
Jan 2005 8
CNGS BeamBaseline: 730 km<Eν> = 17 GeVoptimised for τappearance
CERN Neutrinos to Grand Sasso
CERN SPSEp = 400 GeV4.8*1013 ppp cycle 6 - 27.6 sec7.6*1019 pot/year
• Experiments– OPERA– ICARUS
Jan 2005 9
brick(56 Pb/Em. “cells”)
8 cm (10X0)
Jan 2005 10
OPERA ντ Candidates
“ Long decays″reconstruct kink topology
“ Short decays ″detect large impact parameter track
Loose cut to reject low momentum tracks
Jan 2005 11
OPERA: ∆m2
OPERA90 % CL in 5 years
(mixing constrained by SuperK)90 % CL limits * ∆m2 ( 10-3 eV2 )
1.5 3.2 5.0
Upper limit 2.1 3.8 5.6
Lower limit 0.8 2.6 4.3(U - L) / (2*True) 41 % 19 % 12 %
Nτ / year 0.82 2.82 3.66
* assuming the observation of a number of events corresponding to those expected for the given ∆m2
Probability to observe SuperK signal
years P3σ P4σ
3 93% 83%
5 96% 91%
Jan 2005 12
ICARUS
Liquid Argon TPC Physics Program
Nucleon DecayAtmospheric NeutrinosSolar NeutrinosBeam Neutrinos
Electronic bubble chamber
Jan 2005 13
2
El.m. shower
Full 2D View from the Collection Wire Plane
2 4 6 1812Wire coord. (m)
2Drift coord. (m)
Zoom views
1
32
2
3
µ stop and decay in e
Detail of a long (14 m) µ track with δ-ray spots
El.m. shower
T600 test @ Pv: Run 201 - Evt 12
1
Jan 2005 14
The Status so farSolar Neutrinos
good measurement
Atmospheric Neutrinosinitial measurement
Precision measurement to follow soonMINOS
What is missing?
0122 5 212
30
7 10 eVm
θ−
≈
∆ ≈ ×
0232 3 223
45
2 10 eVm
θ−
≈
∆ ≈ ×
or e µ τν ν ν→
µ τν ν→
Jan 2005 15
The Missing Pieces
1312 13 13 12 1
23 12 12 23 12 23 12 23 13 23 2
23 12 12 23 12
13 13
23 23 1213 13 13 23 3
ei i
i i
c c c sc s e c s c c e s s c s
s
s s e c c c s e c s cs
cs
s s
δ
δτ
δ
δµ
ν νν νν ν
⎛ ⎞ ⎛ ⎞⎛ ⎞⎜ ⎟ ⎜ ⎟⎜ ⎟= − − −⎜ ⎟ ⎜ ⎟⎜ ⎟⎜ ⎟ ⎜ ⎟⎜ ⎟− − −⎝ ⎠ ⎝ ⎠⎝ ⎠
One mixing angle largely unknown: θ13Small, only limits existResults in sub-dominant oscillations
CP violating phase δPossible large CP violation in lepton sectorMay give hints towards GUTWhy are we here?
matter vs. anti-matter asymmetry
eµν ν→
Jan 2005 16
Sub-Dominant OscillationsSome Math:
A. Cervera et al., Nuclear Physics B 579 (2000) 17 – 55,
expansion to second order in 12 1213 12
23
, , , LA
θ ∆ ∆∆
∆
P (νµ → νe) = P1 + P2 + P3 + P4
Jan 2005 17
Why Off-Axis?
0
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0 2 4 6 8 100
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0 2 4 6 8 10
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0 2 4 6 8 100
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0 2 4 6 8 10
Jan 2005 18Next generation LBL experiments in Japan“T2K neutrino project”
• Baseline ~295 km• Energy ~ 1 GeV• Sensitive to
•Θ13 andδ
1st phase 0.75MW
Beam power
2nd phase ~4MW
Far detector
SuperKamiokande(50kt)
HyperKamiokande(1Mt)
PhysicsXννµ →disappearance
appearance eννµ →NC measurements
CP violationProton decay
Jan 2005 19
Sensitivities in first phase(5yrs)
δ(si
n2 2θ 2
3)δ(∆m
232
)
0.01
1×10-4
True ∆m232 (eV2)
d(sin22θ)~0.01 d(∆m2) ~<1×10-4
OAB-2degree
Search for νe appearance νµ disappearance
excludedby reactor
132
2322 2sinsin2sin θθθµ ⋅≡e
~0.5sin22θ13>0.006 (90%)sin22θ13>0.018 (3σ) w/ beam MC, & full SK det. simulation
x20
Sensitive
in 5 years
Jan 2005 20
NOvA: Potential Sites
Vermilion Bay, Ontario,CN980 km, 18 km up
Fort Frances, Ontario,CN875 km, 9 km up
Ash River, MN825 km, 5 km up
Buyck, MN775 lm, 2 km up
LTV site, MN715 km, 1 km down
MINOS Location735 km
Jan 2005 21
NOvA (TASD)
Totally Active Scintillator Detector
Jan 2005 22
NOvA (TASD) Performance
Jan 2005 23
Physics Reach
Jan 2005 24
ComparisonP. H
uber et al. hep-ph/0403068
T2K
NOvA
Jan 2005 25
Mass Hierarchy (sign of ∆m213)
CombineT2KNOvA
Use right baseline to determine sign of ∆m2
13
best, if E/L is the same! S.
Par
ke@
Arg
onne
NuM
I OA
mee
ting
Jan 2005 26
CP violation & Mass Hierarchy
Jan 2005 27
Summary
In LBL ExperimentsNeutrino Oscillation well established
Next generation of detectors precision measurements of some parameters
New generation of experiments might reveal unknown neutrino parameters
Masses & hierarchyAnglesCP phase
Jan 2005 28
KamLAND
Jan 2005 29
Measured Energy Spectrum
Jan 2005 30
“Solar” Neutrino Results
Jan 2005 31
Jan 2005 32
Zenith Angle Distribution
Jan 2005 33
SuperKamiokande Results
Jan 2005 34
K2K Experiment
Jan 2005 35
K2K Results