Title: METU
1METU
2- Status and Preliminary Results
- Future Plans and Conclusion
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4CsI(Tl) Crystal Array
5 Z 0 cm
QR
Z 40 cm
208Tl
40K
FADC Readout 16 ch., 20 MHz, 8 bit
QL
137Cs
Region of Interest for SM ???ee)
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7 Period II Data Volume (186 kg in mass) Total
95 / 50 days ON/OFF Period III Data Volume (200
kg in mass) Total 190 / 40 days ON/OFF
- Energy resolution info
- ? 10 FWHM _at_ 660 keV
- Z-position resolution is
- ? ?(z) 2 cm _at_ 660 keV
- ? ?(z) lt2 cm _at_ higher energies
8- Get z-definition correction parameter f
Whats wrong
SEH, SCH
SEH, SCH
SEH, SCH
SEH, SCH
9Data Analysis Techniques - Calibration
10Event Selection
11Data Analysing Techniques - Defining Cuts
12Data Analysing Techniques - Defining Cuts
13P-II and P-III OFF CsI Energy Spectra with
Various Cuts
14ON and OFF Energy Spectra
36 Crystals (40 cm) Mass 57.6 kg Basic
cuts PSD 4 cm Z-cut
ON spectrum 0.5086 0.0093/day/kg in Period II
(5922 kg-day)
OFF spectrum 0.4502 0.0127/day/kg in Period
II (2786 kg-day)
15P-II and P-III OFF CsI Energy Spectra with
Various Cuts
Period-III
Period-II
16P-II P-III CsI Energy Spectra
17Background Understanding
B. Environmental Backgrounds
- IDEA multiple-hit analysis can give us very good
understanding especially Tl-208 and cosmic
related background in the region of interest. - Cosmic
- - By comparing cosmic and not-cosmic
multiple-hit spectra. - - Tl-208
- - By examining multiple-hit spectra
as well as simulation of Tl-208 decay chain
energies to understand/suppress background in the
region of 3-4 MeV.
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19Intrinsic 137Cs Level
31.3 kgday of CsI(Tl) data was analysed.
137Cs contamination level in CsI was drived gt
(1.55 0.02 ) X 10-17 g/g
20Event Configuration
- Pulse shape (ß or a)
- Timing of event
- 50 ns per bin (20 MHz FADC)
- 10,000 bins (500 µs) per event
- 356 bins (17.8 µs) for following pulse
2050ns
21The Event Selection 238U chain
238U abundance (0.86 0.03) x10-12 g/g
238U abundance 0.82 0.02 x10-12 g/g
22The Event Selection 235U chain
(a) 223Ra(a)? 219Ra(a, 3.96 s)? 215Po
(b) 219Ra(a)? 215Po(a, 1.78 ms)? 211Pb
- Selection 3-a signature
- both time delay greater than 500 ms
- No signal
- DAQ Inactive
235U abundance lt 4.9 x10-14 g/g
23The Event Selection 232Th chain
232Th abundance (2.23 0.06) x10-12 g/g
24The Event Selection 232Th chain
232Th abundance (2.3 0.1) x10-12 g/g
25Delta Z Distributions
26Environmental Background Understanding
81 crystals including 2020 and 40 cm crystals in
PII was analysed.
27Simulation 4 MeV pair-production
511 keV
S1
S2
S3
28Background Understanding via Multi Hit
External Source(s)
511 keV
605 keV
2100 keV
796 keV
1173 keV
1332 keV
- Co-60 contamination
- 1173.2 keV 99.86 accompanied with 1332.5 keV
99.98 - The background related to reactor. Mostly come
from the dust. - Tl Pair Production One escape peaks
- ( 2105 511 keV)
- Cs-134 (n 133Cs g 134Cs)
- 605 keV 97.6
- 796 keV 85.5
583 keV
External Source(s)
2614 keV
With the Q of beta decay at 2MeV
Internal Source(s)
2614 keV 99 accompanied with 583 keV 85 510.8
keV 23 860 keV with 13
860 keV
- Cosmic induced neutrons can be captured by the
target nuclei 133Cs.
- Combination of Tl gammas can affect up to around
4 MeV
29Background Understanding Due to Tl-208 and
Cosmic Inefficiency
30SH Prediction for Cosmic Background
- ? ON - OFF
- ? ON - (SH)pred.
where T1 (SH)not cos (SH)cos and
T2 (MH)not cos (MH)cos
d(SH)pred lt dOFF we win
with this alternative approach
- Single Hit Prediction is made by using ON period
data. We can improve accuracy profoundly since we
have more than 100 days ON data in PII and 200
days in PIII and more for other periods
31Background Understanding Due to Tl-208
32Background Understanding Due to Tl-208
580 keV
510 580 keV
860 keV
860 keV
33Background Understanding Due to Tl-208
580 keV g 2614 keV g
860 keV g 2614 keV g
No z cut
34Tl-208 SH Estimation 3 - 3.5 MeV PIII-ON Period
Tl 2614 583 keV
No z-cut
4 cm z-cut
Best fit 0.0343 0.0025 c2 10.89/(nof8)
SH 471.11 34.34
35Tl-208 SH Estimation 3 - 3.5 MeV PIII-ON Period
Tl 2614 860 keV
No z-cut
4 cm z-cut
Best fit 0.002722 0.000199 c2 11.52/(nof8)
SH 38.17 2.79
36Tl-208 SH Estimation 3.5 - 4 MeV PIII-ON Period
Tl 2614 860 keV
No z-cut
4 cm z-cut
SH 18.29 1.69
Best fit 0.001305 0.000121 c2 11.011/(nof8)
37Background Expectation via PAIR PRODUCTION
3 - HIT
2 - HIT
q
p
q
q
p
SH
p
38Background Understanding via Pair-Pro
d lt 2 crys
K-40 950 keV
K-40 950 keV
Tl-208 2100 keV
Tl-208 2100 keV
Tl-208 2614 keV
Tl-208 2614 keV
1 cry d
39Background Understanding via Pair-Pro
850 keV K-40
1600 keV Tl -208
2100 keV Tl -208
2614 keV Tl -208
40Background Understanding via Multi-Hit
Cosmic-Ray Inefficiency
- Red Cosmic
- Blue not-cosmic
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42OFF-BKG (Multi-Hit)
Period-III
Period-II
Sin2qW 0.0001 0.13
Sin2qW 0.00005 0.109
43SH Prediction via Multi-Hit for ON Data
Period-II
Period-III
Energy (MeV)
Single-Hit
Single - Hit
Prediction
Prediction
961 31
3 3.5
961 31
937.6 42.2
1747 41.8
1641.4 46.6
287.2 15.9
734 27.1
292 17.1
3.5 4
741.825.1
524 22.9
4 4.5
193 13.9
188.6 13.2
504.320.9
356 18.9
4.5 5
141 11.9
128.3 10.9
368.0 17.8
5 5.5
117 10.8
91.4 9.2
270.615.3
263 16.2
203 14.3
5.5 6
81 9
66.4 7.9
202.113.2
6 6.5
50.6 6.9
175 13.2
175.112.1
55 7.4
200 14.14
6.5 7
77 8.8
79.1 8.3
180.112.0
157 12.5
76 8.7
7 7.5
84.1 8.3
177.011.5
7.5 8
137 11.7
73 8.5
60.9 7.1
109.9 9.3
44sin2qW measurement for Period-II
ON-OFF
ON-(BKG)expec.
s (1.786 1.297) sSM
s (1.194 1.145) sSM
Sin2qW 0.328 0.137
Sin2qW 0.259 0.153
45sin2qW measurement for Period-II
ON-(OFF BKG)expec
s (1.454 1.859) sSM
Sin2qW 0.291 0.102
46sin2qW measurement for Period-III
ON-OFF
ON-(BKG)expec.
s (1.298 1.413) sSM
s (1.0004 0.8977) sSM
Sin2qW 0.272 0.179
Sin2qW 0.231 0.133
47sin2qW measurement for Period-III
ON-(OFF BKG)expec
s (1.01 0.77) sSM
Sin2qW 0.233 0.114
48sin2qW measurement for Period-II Period-III
ON-(BKG)expec.
s (1.207 0.577) sSM
Sin2qW 0.260 0.076
49Expected Accuracy with data size
sSin2qW 0.13 sSM
50TEXONO and World status
Characteristics of the previous and current n-e
scattering experiments
51Background Expectation via PAIR PRODUCTION
3 - HIT
2 - HIT
q
p
q
q
p
SH
p
52Conclusion
Sin2?W was observed but there is NO real
measurement for reactor neutrino YET.