kr2det: two - detector reactor neutrino oscillation experiment at krasnoyarsk underground site l....
TRANSCRIPT
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Kr2Det:
TWO - DETECTOR REACTOR NEUTRINO OSCILLATION
EXPERIMENT AT KRASNOYARSK UNDERGROUND SITE
L. Mikaelyan for KURCHATOV INSTITUTE NEUTRINO
GROUP
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TOWARDS VERY SMALL MIXING PARAMETERS IN THE ATMOSPHERIC
NEUTRINO MASS REGION
THE MAIN GOAL OF THE PROJECT IS :
TO FIND THE CONTRIBUTION of m-3 MASS STATE to the ELECTRON NEUTRINO FLAVOR STATE or to SET NEW MORE STRINGENT CONSTRAINTS
WE HOPE THAT at 1km from REACTOR the SENSITIVITY
sin2213 2.010-2 for m2 = 2.510-3 eV2
CAN BE ACHIEVED.
For larger mixing parameters the experiment is sensible to
m2 410-4 eV2
(PART of the HLMA REGION!)
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NEUTRINO OSCILLATION LIMITS
0.01 0.10 1.00
10-2
10-3
sin 2 2
m
, eV
2
2
C H O O Z
K r2 D e t (ex p ec ted )
m a tm2
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Plan of the report
The CHOOZ oscillation limits
Kr2Det:
• Idea of experiment,• Detectors,• Neutrino detection rates,
backgrounds,• Method of analysis,
Systematics,• Expected sensitivity,• Other applications,• Conclusions
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Philosophy: Reactors vs Accelerators
Strategy: Step by step progress
If sin2213 is 100-1000 times smaller than present CHOOZ limits then necessary sensitivity can be achieved (in distant future and in several steps) with neutrino super beams and neutrino factories using 25-1000 kt (!) detectors located at a few thousand km from accelerator source.See for example: S.Geer, hep-ph/0210113
However, the first step can be done sooner (an cheaper) at reactors.
It is quit possible that sin2213 is just a few times smaller than present limit. No physical principal is known why it should be so terribly small.
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REACTOR ANTINEUTRINO DETECTION REACTION:
e + p e+ + n
Positron visible energy Ee+vis :
Ee+vis E - 0.8 (MeV)
(E is the energy of incident e)
The neutron is captured in H (or in Gd).
In the experiment spatial- and time correlated (e+ , n ) pairs are detected and positron energy spectrum measured.
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Positron spectrum
0 1 2 3 4 5 6 7 8Positron visible energy, MeV
0.00
0.05
0.10
0.15
0.20
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REACTOR ANTINEUTRINO OSCILLA-TIONS AT ~ 1 km FROM THE REACTOR SOURCE
e = Ue1 1 + Ue2 2 + Ue3 3 ( Ue3 sin13 )
We conservatory assume here that
m1 < m2 < m3 and m2sol = m2
2 – m12 < 10-4 eV2
m2atm
= m32 – m1
2 m32 – m2
2 2.510-3 eV2 >> m2sol
The e survival probability P(e e ) is then:
P(e e ) = 1 – sin22sin2 ,
sin22 sin2213 4Ue32(1-Ue3
2),
= (1.27m2 L E-1),
L(m) is the distance from the reactor
Numerically: = 1.05 = 60 for m2 = 2.510-3 eV2, L = 1000 m, E= 3 MeV
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CHOOZ detector (300 mwe)The detector is contained in 5.5 m diameter cylindrical steel tank shielded by low radioactivity sand (75 cm) and cast iron (14 cm)
Gd
Inside the tank there are three concentric regions:•Central 5-ton target in a transparent Plexiglas container filled with a 0.09% Gd loaded scintillator,•Intermediate 17-ton volume filled with unloaded scintillator,•Outer 90-ton optically separated veto counter filled with unloaded scintillator
Very important to suppress -s
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CHOOZ final results
France-Italy-Russia-US Collaboration
College de France LAPP, AnnecyINFN&Univ. of Pisa INFN&Univ. of TriesteKurchatov Institute, MoscowUniv. of Irvine Drexel Univ. Univ. of New
Mexico
Two reactors of summed rated power W=8.5 GW (thermal)Detector located at a depth of 300 mwe,
at ~1000 m from the reactors.
Neutrino events selectionSummary of data acquisition (April 1997 – July 1998)
Neutrino detection efficiency: 70%Total No of detected neutrinos: ~2700Neutrino detected rate at full power: 26 d-1
Background: ~1.2 d-1
Neutrino/BKG, typically ~10:1
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CHOOZ final results
Neutrino detection rates
Xrate = measured/expected
Positron spectrum shape: measured vs expected
Number neutrino separately measured from two reactors
CHOOZ’97 Xrate = 0.98 4%(stat) 4%(syst)
CHOOZ’99 Xrate = 1.01 2.8%(stat)
2.7%(syst)
CHOOZ’97 used (0) calculated (2.5%)
CHOOZ’99 uses (0) measured (1.4%)
CdF+LAPP+Kurchatov, 1994 y.
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Kr2Det - probing Ue3 with reactor e
Method:
Two identical detectors (BOREXINO, KamLAND design) 600 mwe
100 m 1000 m
Target: 50 t 50 t Rate: 1.5 ·106 /year 15 ·103 /yearS:B >>1 ~ 10:1
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Kr2Det, detector scheme500 PMT EMI 9350 Diameter – 8 inches,
Coverage – 20%
V e to z o n e
tra n sp a re n t f ilm
B u ffe rlig h t g u id(m in e ra l o il)
T u b e s fo r f ill in g a n d in tro d u c in g ra d io a c tiv eso u rc e s
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NEUTRINO DETECTION RATES
Assuming: Target radius 2.35 m Target volume 54 m3
Scintillator: Density: 0.85 g/cm3
Mass: 46 ton H/C ratio: 1.8 # of H atoms 0.7851029 / ton Detection efficiency 0.75 300 days/year Lfar = 1000 m, Lnear = 100 m
One finds: N far = 17103/year N near = 1.7106/year
( 1.2 / tonday ) ( 120 / tonday)
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BACKGROUNDS Time correlated BKG is found by extrapolating the value measured at CHOOZ : CHOOZ: 300 m.w.e., 0,24 / daytarget ton Kr2Det: 600 m.w.e., 0.08/ daytarget ton, which is less than 10% of the far detector e detection rate Accidentals
Due to high neutrino rates requirements to radiopurity of the detector materials are much less severe than in BOREXINO and KamLAND experiments.
The target scintillator can have U, Th, 40K and 222Rn concentrations 10-13, 10-13 , 10-13 g/g and 1mBq/m3 respectively.
In no Gd case the surrounding rock is expected to be the main source of the BKG…
Additional passive shielding around the detector may be required.
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ANALYSIS
The RATIO of the two MEASURED POSITRON SPECTRA in no-oscillation case is ENERGY INDEPENDENT. Small specific deviations from the constant value of this ratio:
Sfar/S near = const [1 – Sin22Sin2(1.27m2 LE-
1)] are searched for oscillations.
The analysis is independent of the exact knowledge of the neutrino flux and their energy spectrum, burn up effects, numbers of target protons… HOWEVERE RELATIVE DIFFERENCE of the DETECTOR RESPONCE FUNCTIONS MUST BE STRICTLY CONTROLLED. CALIBRATION OF THE DETECTORS IS THE KEY PROBLEM OF THIS EXPERIMENT
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0 1 2 3 4 5 6 7 8 90
10000
20000
30000
C s137
annih illa tiongam m as
H (n, )D
60Co
24N a
G d(n, )
Prom pt gam m as from C f
Visible positron energy, MeV
Positron spectrum
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DIFFERENCE of the DETECTOR’s RESPONSE CAN
BE MEASURED AND CORRECTED FOR
WE HOPE THAT WITH CALIBRATION PROCEDURES DETECTOR SPECTROMETRIC DIFFERENCE CAN BE CONTROLLED DOWN TO 0.5%.
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0 1 2 3 4 5 6 7 8Positron vis ib le energy, M eV
0.01
0.03
0.07
0.14 C H O O Z lim it
m =2.5 10 eV2 -3 2
0.85
0.90
0.95
1.00
Ratio of positron spectra far/near
Lfar = 1000 m, Lnear = 100 m, Nfar = 16·103/year
Values of sin22 are shown at the curves
m2 = 2.510-3 eV2
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Ratio of positron spectra far/near
Lfar = 1000 m, Lnear = 100 m, Nfar = 15·103/year
Values of sin22 are shown at the curves
0 1 2 3 4 5 6 7 8Positron vis ib le energy, M eV
0.11
C H O O Z lim it
m =3.0 10 eV2 -3 2
0.07
0.03
0.01
0.85
0.90
0.95
1.00
m2 = 310-3 eV2
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CONCLUSIONS & DISCUSSIONS
1) In the one reactor – two detector scheme systematic errors are minimized since NO ACCURATE KNOWLEDGE is needed of
- Reactor power and its fuel composition,
- Reactor e energy spectrum, its variation during the operational run - Hydrogen atom concentrations - Target volumes
With ONE reactor backgrounds can periodically be measured.
We conclude that
Kr2Det can sensitively search for neutrino oscillations in the atmo-spheric mass region
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2) Kr2Det uses available underground halls for the Far (1000m) and Near (115m) 50 ton detectors
The oscillation signal could be some-what increased with the Far detector at ~ 1400-1900 m or
with two far detectors at ~ 1300 and 2600 m…This however would require digging new caverns and using detectors with larger target masses…
* * *
The Kr2Det project is still in R&D phase
All parameters of the experiment are open for discussions…
Use of a good Gd scintillator would help to suppress accidentals from U/Th in the rock
Effective collaborators are welcome to join.