measuring 13 with reactors stuart freedman university of california at berkeley slac seminar...
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![Page 1: Measuring 13 with Reactors Stuart Freedman University of California at Berkeley SLAC Seminar September 29, 2003](https://reader036.vdocuments.site/reader036/viewer/2022062421/56649d805503460f94a64a56/html5/thumbnails/1.jpg)
Measuring 13 with ReactorsStuart Freedman
University of California at Berkeley
SLAC Seminar September 29, 2003
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I am going to argue that --
the fastest and cheapest way to determine the value of Sin2213 is to
measure two big things and subtract the results.
- =
How to Weigh Dumbo’s Magic Feather
1313
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Neutrino LANDscape
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Constraints from most recent Experiments
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€
U =
Ue1 Ue2 Ue3
Uμ1 Uμ 2 U μ 3
Uτ1 Uτ 2 Uτ 3
⎛
⎝
⎜ ⎜ ⎜
⎞
⎠
⎟ ⎟ ⎟
=
cosθ12 sinθ12 0
−sinθ12 cosθ12 0
0 0 1
⎛
⎝
⎜ ⎜ ⎜
⎞
⎠
⎟ ⎟ ⎟×
cosθ13 0 e−iδ CP sinθ13
0 1 0
−e iδCP sinθ13 0 cosθ13
⎛
⎝
⎜ ⎜ ⎜
⎞
⎠
⎟ ⎟ ⎟×
1 0 0
0 cosθ23 sinθ23
0 −sinθ23 cosθ23
⎛
⎝
⎜ ⎜ ⎜
⎞
⎠
⎟ ⎟ ⎟×
1 0 0
0 e iα / 2 0
0 0 e iα / 2+iβ
⎛
⎝
⎜ ⎜ ⎜
⎞
⎠
⎟ ⎟ ⎟
12 ~ 30° 23 ~ 45°tan2 13 < 0.03 at 90% CL
UMNSP Matrix
Mass Hierarchy
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Slide Courtesy of B. Kayser
What do we know and how do we know it
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Is it important to measure 13?
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Testimonials
L. Wofenstein
S. Glashow
B. Kayser S. Bilenky
A Smirnov
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Measuring 13 Accelerator Experiments
• appearance experiment• measurement of e and e yields 13,CP
• baseline O(100 -1000 km), matter effects present
Reactor Neutrino Oscillation Experiment
• disappearance experiment • but: observation of oscillation signature with 2 or multiple detectors• look for deviations from 1/r2 • baseline O(1 km), no matter effects
QuickTime™ and aTIFF (Uncompressed) decompressorare needed to see this picture.
€
Pee ≈1− sin2 2θ13 sin2 Δm312L
4Eν+
Δm212L
4Eν
⎛
⎝ ⎜
⎞
⎠ ⎟cos4 θ13 sin2 2θ13
€
e →ν x
e
ee
€
→ e
€
Pμe ≈ sin2 2θ13 sin2 2θ23 sin2 Δm312L
4Eν+ ...
decay pipehorn absorbertargetp detector
+
+ +
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Minakata and Nunokawa, hep-ph/0108085
Figuring out CP for leptons
€
P(ν μ →ν e ) − P(ν μ →ν e ) = −16s12c12s13c132 s23c23 sinδ sin
Δm122
4EL
⎛
⎝ ⎜
⎞
⎠ ⎟sin
Δm132
4EL
⎛
⎝ ⎜
⎞
⎠ ⎟sin
Δm232
4EL
⎛
⎝ ⎜
⎞
⎠ ⎟
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Basic Idea for a Disappearance Experiment
?
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ReactorDetector 1Detector 2
d2
d1
Experimental Design
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First Direct Detection of the Neutrino
Reines and Cowan 1956
€
E prompt ≅ Eν − En − 0.8 MeV
)2.2( MeVdpn γ+→+
nepe +→+ +
sτ 210≈e ne+
2.2MeV~210 ms
Scintillator
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Inverse Beta Decay Cross Section and Spectrum
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Neutrino Spectra from Principal Reactor Isotopes
235U fission
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1m
Poltergeist
Chooz4 m
KamLAND20 m
Long Baseline Reactor Neutrino Experiments
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CHOOZ
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CHOOZ
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20
15
10
5
0
reactor neutrinos geo neutrinos background
25
20
15
10
5
086420
Prompt Energy (MeV)
2.6 MeVanalysis threshold
KamLAND data no oscillation best-fit oscillation
sin22 = 1.0 Δm2= 6.9 10x -5 eV2
KamLAND
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KamLAND
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from 12C(n, γ )
τcap = 188 +/- 23 sec
Inverse Beta Decay Signal from KamLAND
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13 at a US nuclear power plant?
Site Requirements
• powerful reactors
• overburden
• controlled access
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Diablo Canyon Power Station
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scintillator e detectors
e + p e+ + n
coincidence signalprompt e+ annihilationdelayed n capture (in s)
€
Pee ≈1− sin2 2θ13 sin2 Δm312L
4Eν+
Δm212L
4Eν
⎛
⎝ ⎜
⎞
⎠ ⎟cos4 θ13 sin2 2θ12
• disappearance experiment • look for rate deviations from 1/r2 and spectral distortions• observation of oscillation signature with 2 or multiple detectors• baseline O(1 km), no matter effects
e< 1 km
e,,τ~ 1.5-2.5km
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Overburden Essential for Reducing Cosmic Ray Backgrounds
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~60,000
~10,000
Statistical error: stat ~ 0.5% for L = 300t-yr
~250,000
Detector Event Rate/Year
Statistical Precision Dominated by the Far Detector
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2 or 3 detectors in 1-1.5 km tunnel
Diablo Canyon
Variable Baseline
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Ge
Issues
- folding may have damaged rock matrix- steep topography causes landslide risk- tunnel orientation and key block failure- seismic hazards and hydrology
Geology
I
II
IIIaIIIb
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liquid scintillatorbuffer oil
muon veto
passive shield
Detector Concept
5 m
1.6 m
Variable baseline to control systematics and demonstrate oscillations (if |13| > 0)
acrylic vessel
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Movable Detectors
5 m~12 m
• Modular, movable detectors• Volume scalable• Vfiducial ~ 50-100 t/detector
610
1-2 km
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Kashiwazaki: 13 Experiment in Japan
- 7 nuclear reactors, World’s largest power station
near near
far
Kashiwazaki-KariwaNuclear Power Station
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near near
far
70 m 70 m
200-300 m
6 m shaft hole, 200-300 m depth
Kashiwazaki: Proposal for Reactor 13 Experiment in Japan
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Ref: Marteyamov et al, hep-ex/0211070
Reactor
Detector locations constrained by existing infrastructure
Features - underground reactor - existing infrastructure
~20000 ev/year~1.5 x 106 ev/year
Kr2Det: Reactor 13 Experiment at Krasnoyarsk
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%Total LS mass 2.1Fiducial mass ratio 4.1Energy threshold 2.1Tagging efficiency 2.1Live time 0.07Reactor power 2.0Fuel composition 1.0Time lag 0.28e spectra 2.5
Cross section 0.2
Total uncertainty 6.4 %
Systematic Uncertainties
E > 2.6 MeV
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Systematics
Reactor Flux • near/far ratio, choice of detector location
Best experiment to date: CHOOZ
Target Volume & • well defined fiducial volume
Backgrounds • external active and passive shielding for correlated backgrounds
Detector Efficiency • built near and far detector of same design • calibrate relative detector efficiency variable baseline may be necessary
Ref: Apollonio et al., hep-ex/0301017
Total syst ~ 1-1.5%
rel eff ≤ 1%
target ~ 0.3%
n bkgd < 1%
flux < 0.2%
acc < 0.5%
.
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MC Studies
Normalization: 10k events at 10km
‘far-far’ L1=6 km L2=7.8 km
‘near-far’ L1 = 1 km L2 = 3 km
Oscillation Parameters:sin2213 = 0.14Δm2= 2.5 x 10-3 eV2
Optimization atLBNL
P νe → νe( )≈sin4θ13+cos4θ13 1−sin2(2θ12) ⋅sin2 Δm122 L
4Eν
⎛
⎝ ⎜
⎞
⎠ ⎟
⎧ ⎨ ⎩
⎫ ⎬ ⎭
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Sensitivity to sin2213 at 90% CL
Reactor-I: limit depends on norm (flux normalization)
Reactor-II: limit essentially independent of norm
statistical error only
fit to spectral shape
cal relative near/far energy calibration
norm relative near/far flux normalization
Reactor I12 t, 7 GWth, 5 yrs
Reactor II250 t, 7 GWth, 5 yrsChooz 5 t, 8.4 GWth, 1.5 yrs
Ref
: H
uber
et a
l., h
ep-p
h/03
0323
2
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statistics StatisticsSystematicsCorrelationsDegeneracies
Ref
: H
uber
et a
l., h
ep-p
h/03
0323
2
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Expected Constraints on 13
Experiment sin2(213) 13 When?
CHOOZ < 0.11 < 10
NUMI Off- Axis (5 yr) < 0.006-0.015 < 2.2 2012
JPARC-nu (5 yr) < 0.006-0.0015 < 2.3 2012
MINOS < 0.06 < 7.1 2008
ICARUS (5 yr) < 0.04 < 5.8 2011
OPERA (5 yr) < 0.06 < 7.1 2011
KR2DET (Russia) < 0.016 < 3.6 ?
Kashiwazaki (Japan) < 0.026 < 4.6 [2008]
Penly/Cruas (France) < 0.025 < 4.5 [2010]
Diablo Canyon (US) < 0.01-0.02 < 2.9 [2009]
Upper limits correspond to 90% C.L.
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