Upload
ursula-craig
View
217
Download
1
Embed Size (px)
Citation preview
Simulation study of RENO-50
Jungsic ParkSeoul National University
RENO-50 International WorkshopJune 13-14, 2013
Hoam Faculty House, Korea
Preliminary RENO-50 Detector Concept
25 m
27 m
RENO-50
25 m
27 m
LS (10 kton)
15000 10” PMTs
Mineral Oil
32 m
32 m
Water
KamLAND x 10
1000 10” OD PMTs Concentric cylindrical detector.
- Initial concept is same as RENO.- No gamma-catcher region and filled with Liquid Scintillator Only.
- Install 15000, 10 inch inner PMTs and 1000, 10 inch outer PMTs.
RENO-50 Detector with Monte-Carlo
Target : Acrylic, 25m*25mBuffer : Stainless-Steel, 27m*27mVeto : Concrete, 32m*32m
PMT attachment scheme.
Barrel : 50 raw * 200 column (9*26 for RENO)Interval of each PMT center is 50cm.
Top & Bottom
2501 PMTs for each region. (60 for RENO)45cm
45cm
2700cm
270
0c
m
Energy resolution
Assume that optical properties and thickness of detector materials are same as RENO detector.
For the energy resolution, we generate single gamma of various energy (1~10MeV)at the detector center.
Using the initial concept, we get~7% resolution @ 1MeV and calculated PMT coverage is 24%. PMT coverage : 23.95%
sensitivity test by Monte-Carlo.
Using the Pseudo-experiment , check the sensitivity of θ12 and Δm221 measurement.
True value : varied varied
002320
0000760
1002
855602
231
221
132
122
.
.
.sin
.sin
m
m
fixed
Measurement of θ12 and Δm221
Assume 10kton * 20GW * 5years exposure
002320
1002
855602
0000760
231
132
122
221
.
.sin
.sin
.
m
m
fixed
222
2
26
1
12
2
11
)()()(
)*(
))(*)(**)(*exp*(
reb
bbkgbkgsignal
r
oscirbkgsignal
feb
NNN
funcefNbNN
Nsignal = 30000 (oscillation , 10kton, 20GW, 5years, 100% efficiency & Livetime )Nbkg = 300 (~1% level)
ε = 1.0 (detection efficiency)b,e, f : pull parameter (e : efficiency, f : reactor)σeff = 0.015 (1.5%)σr = 0.03 (current limit : ~3% goal is below 1%)σb = 0.05 (5%)
Nexpr : Expected event number without oscillationFuncosci(θ12) : oscillation / No oscillation (fraction)
Χ2 fitting with pulls for θ12
True value : 0.8556Fitting value : 0.8552 +- 0.0162 (1σ) ~1.89%
Χ2 fitting result
σeff = 0.015 (1.5%)σr = 0.03 (3%)σb = 0.05 (5%)
Statistics part decrease very rapidly.The main portion is systematic part.
Statistical part only for θ12
Uncertainty of detection efficiency and reactor uncertainty are both important.
Systematical part for θ12
We assumed σb is zero.
222
2
26
1
22111
1
2
)()()(
)*(
))(*)(**)(*exp*(
r
f
e
e
b
b
bibkgNi
bkgNisignalN
rmoscifuncefr
iNbibkgNi
signalNNbin
i
For the Δm221 , we should use the spectrum shape.
N_signal, N_expr N_bkg should be considered bin by bin.Assumed that background is flat. (same number for each bin content)
50bin/MeV 1.8 ~ 8 MeV range cut
Χ2 fitting with pulls for Δm221
ε = 1.0 (detection efficiency)b,e, f : pull parameter (b: background, e : efficiency, f : reactor)σeff = 0.015 (1.5%)σr = 0.03 (current limit : ~3% goal is below 1%)σb = 0.05 (5%)
Systematical part for Δm221
True value : 7.6e-5
Fitting value : (7.598 +- 0.048)e-5 (1σ) ~0.64%
σeff = 0.015 (1.5%)σr = 0.03 (3%)σb = 0.05 (5%)
Expected neutrino visible energy spectrum of RENO-50
002320
0000760
1002
855602
231
221
132
122
.
.
.)(sin
.)(sin
m
m
Energy resolution plays a crucial role to RENO-50
Solid line : Normal HierarchyDashed line : Inverted Hierarchy
So, How can we increase the energy resolution ?
@1MeV
1. Increase the attenuation length of Liquid Scintillator. - 1.5 times current value : 18.7m @ 430 nm - 2.0 times current value : 24.9m @ 430 nm
2. Increase the PMT Quantum Efficiencies. - 1.25 times current value : 30.0% @ 427 nm - 1.5 times current value : 36.0% @ 427 nm
3. Increase the PMT coverage. - 25000 PMTs : 40.86 % coverage
Cf) Default value 24% PMT coverage Att.length of LS is 12.4m @ 430 nm PMT QE is 24% @ 427 nm
Improve the optical properties
24% @ 430 nmMaximum 25% @ 390nm
PMT Quantum Efficiency of R7081 Hamamatsu 10 inch PMT
Mineral OilLiquid Scintillator
Liquid Scintillator : 12.4m @ 430 nmMineral Oil : 17.0m @ 430 nm
Attenuation Length of Current Materials.
Increase the Attenuation Length
Attenuation length should be comparable of detector size.
Increase the PMT Quantum Efficiency
Increase the PMT Coverage
Applying all the Improvement Effect
It’s very challenging task to acquire ~3% energy resolution.
Summary
RENO-50 Monte-Carlo preliminary version was made.
Statistical uncertainty decrease rapidly within few years.
Detection efficiency and reactor uncertainty contributes to systematic a lot.
Including other uncertainty parameters is still keep going.
3% energy resolution is very challenging task. We should improve all the Optical properties about twice. It’s time to think about the improvement method all together.