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NuFACT'01 29/05/2001 Tsukuba, Japan. Introduction, ge? at PSI ... PMTs operated for 2.5 days stably. Calibration with LED and a source signals done ... – PowerPoint PPT presentation

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Title: R


1
RD works on Liquid Xenon Photon Detectorfor
µge? experiment at PSI
  • Outline
  • Introduction
  • Prototype RD works
  • Summary
  • Satoshi Mihara
  • ICEPP, Univ. of Tokyo

2
Introduction, µge? at PSI
aims to achieve the sensitivity down to
Br(µge?)10-14
  • Detect e and ?, back to back and in time
  • 100 duty factor continuous beam of 108µ/sec
  • Liquid Xe photon detector
  • Solenoidal magnetic spectrometer with a graded
    magnetic field

http//meg.psi.ch
STARTS IN 2003 and RUNS 1- 2 years
3
Introduction,contd
  • µ beam stopped on the target 108/sec
  • Ee52.8MeV E?52.8MeV
  • Back to back, in time
  • Sensitivity
  • Nm1x108/sec, 2.2x107 sec running
    O/4p0.09,ee0.95, e?0.7, and esel0.8
  • aSingle Event sensitivity 0.94x10-14
  • Main background sources
  • Radiative µ decay
  • Accidental overlap
  • NOT back to back, NOT in time
  • Reduced down to 10-15 level

?
µ
e
µge???
µge???
?
?
?
?
?
e
?
e
?
4
Requirement on the Photon Detector
  • Good Energy Resolution
  • Good Position Resolution
  • Good time Resolution

5
Liquid Xe Photon Detector
  • 800 liter liquid Xe
  • 800 PMTs inside liquid(HAMAMATSU R6041Q)
  • Detect scintillation light(?175nm) from Liq.
    Xe(-100?)
  • Fast response, Good Energy, and Position
    resolutions
  • Wph 24 eV
  • (c.f. Wph(NaI) 17eV)
  • tfast 45nsec
  • Mini-Kamiokande type

NaI too slow CsI, BGO poor resolution
at 52.8MeV Inhomoginity to cover large
area
!
6
Strategy for the Detector Construction
  • PMT Development
  • Refrigerator Development
  • Purification System Development
  • Attenuation Length Measurement
  • Small Prototype
  • Large Prototype
  • Final Detector

7
Small Prototype ofLiquid Xe Photon Detector
  • 32 2-inch PMTs surround the active volume of 2.34
    liter
  • ?-ray sources of Cr,Cs,Mn, and Y
  • a source for PMT calibration
  • Metal channel dynodes
  • Possible to be operated at low -100o
  • Silica window to transmit UV light
  • Typical gain 106, Typical Q.E. 10
  • Possible to sustain up to 3 atom

8
Small PrototypeExperimental Procedure
  • Xenon liquified with a nitrogen cooling pipe
  • Kept in stable temp.(-100o) and pressure (1.2
    atom) by controlling the flow of liquid nitrogen
  • PMT operation in liquid xenon has been successful
    for more than one month

9
Small PrototypeSignal from PMTs
  • Typical PMT output for liq. Xe scintillation
    light
  • Triggering condition for ? ray events
  • (ex. For g from Mn)
  • gt 220 p.e. in R1
  • gt 50 p.e. in R2
  • gt 10 p.e. in R3
  • gt 100 p.e. in E1
  • gt 20 p.e. in E2
  • Loose enough to trigger
  • Almost all events where ?
  • interacted well inside the
  • sensitive volume

c
10
Small PrototypeAnalysis
  • Position of ? interaction
  • Weighting the position of the PMTs with their
    individual pulse heights
  • For selecting the fully contained events
  • Requiring the ? int. position should lie within
    a central region of 2cmx1cmf

11
Small PrototypeResult, Energy Resolution
  • Fitting the spectrums with an asymmetric Gaussian
    function.
  • Results are compared with MC prediction.
  • Simulation of ? int. and energy deposition EGS4
  • Simulation of the propagation of scint. Light
  • EGS cut off energy 1keV
  • Att. Length (absorption)29cm
  • Wph 24eV
  • 0.7 in s is expected at 52.8MeV.

12
Small PrototypeResult, Position Resolution
  • PMTs are divided into two groups by the y-z
    plane.
  • ? int. positions are
  • calculated in each
  • group and then
  • compared with
  • each other.
  • Position resolution
  • is estimated as
  • sz1-z2/v2
  • Possible to achieve for 52.8MeV ?
  • slt3mm in position meas.

13
Small PrototypeResult, Time Resolution
  • PMTs are divided again into two groups by the y-z
    plane.
  • In each group the average of the time measured by
    TDC is calculated after slewing correction for
    each PMT.
  • The time resolution
  • is estimated by
  • taking the difference
  • between two groups.
  • Resolution improves
  • as 1/vNpe
  • slt50psec
  • at 52.8 MeV.

14
Short Summary on the Small Prototype
Extrapolation to Higher Energy
  • Energy 0.7
  • Position lt3mm
  • Time lt50psec

in s at 52.8MeV
Excellent!
Go to the next step Large Prototype
15
Large PrototypeHow Large?
  • To study the detector response to higher energy ?
    rays, large volume is required to fully contain
    events.

Depth
40cm x 40cm x 50cm Active Volume
224 PMTs
16
Large PrototypeVessel Design
  • Vessel should be large enough to install the
    detector.
  • Possibility to reuse for future PMT calibration.
  • Thinner entrance window thickness.
  • Thermal insulation.
  • Most of all components used in the final detector
    should be tested in Large Prototype.
  • Refrigerator
  • Feedthrough
  • PMT holder structure
  • Surface level meter etc, etc

17
Construction ofthe Large Prototype Vessel
18
Construction of the Large Prototype Vessel
  • Pressure test up to 0.6MPa
  • Vacuum leak test
  • Cooling test with liquid nitrogen

All OK. Ready to fill liquid xenon inside
19
Assembling
  • Holder
  • Front G10, Plastic
  • Side, RearAluminum
  • Blue LEDs for PMT gain adjustment
  • a sources for calibration
  • Temperature sensors
  • Surface Level meter

20
Pulse Tube Refrigerator
  • Conventionally liq. Nitrogen has been used
  • g waste of nitrogen, not suitable for long
    term physics experiment.
  • Purse tube refrigerator is the best for this
    purpose since there is no moving part
  • in the low temperature stage.

Pressure Oscillation
Mechanically moving
70W
21
Liquefaction Test
  • Pre-cooling before liquefaction
  • with 0.2MPa gas xenon inside.
  • Liquefaction of xenon 100 liter liquid for 2
    day (2.0 liter/hour) .
  • Recondensation using the refrigerator was
    successfully done.
  • Several basic measurements done.
  • PMTs operated for 2.5 days stably.
  • Calibration with LED and a source signals done
  • Currently preparing ? beam test in June.

22
? beam at TERAS
  • Use inverse-compton scattered ? beam provided at
    TERAS in ETL AIST in Tsukuba, Japan.
  • E?10,20,30,40MeV
  • ? beam intensity 1kHz (typ.)
  • Analyze the edge of the Compton photon spectrum.
  • Test will start in the middle of June.

40MeV ?
NaI
Taken after acc. trouble. Better BG condition now!
23
Plan for Attenuation Length Measurement
  • Step1
  • PMT1Absorption Scattering Length meas.
  • PMT2 used as a reference.
  • Collimators to prevent scinti. light from hitting
    the wall.
  • Mask in fron of PMT1 to define the illuminated
    are on the photo cathode.

Liq. Nitrogen
PMT1
Step2 PMT2 Scatt. Length meas. PMT1 reference
at a fixed point.
PMT2
dL/L 5 x L(m)
X ray
24
Summary
  • Small Prototype
  • Small prototype of liquid Xe photon detector was
    successfully constructed and tested with ?-ray
    sources of 320keV-1836keV.
  • Scintillation light from xenon is directly
    observed with PMTs located inside the liquid.
  • Excellent Energy, Position, Time resolutions.
  • Large Prototype
  • 100 liter liquefaction test was successfully
    done.
  • Currently preparing for a large prototype test
    using inverse-compton scattered beam of higher
    energy ? rays gt 40MeV.

25
Summary contd
  • Refrigerator
  • Recondensation of 100 liter of liq. Xenon was
    successful.
  • Studying other coolants for obtaining better
    cooling efficiency.
  • Attenuation Length Measurement
  • Setup construction is going on.
  • Measurements will start in this autumn at
    Novosibirsk.
  • Final Detector
  • Design work just started.
  • Xenon, ? window, PMT mass-production.
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