Stefano Pirroilias.in2p3.fr/.../ILIAS_6th_Annual_Meeting/180209_Pirro.pdfStefano Pirro Ilias 6 th...

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Background Limitation for Simple bolometers Principles of operation Cd-Mo based crystals ZnSe crystals Conclusions Stefano Pirro Ilias 6 th Annual Meeting - Dresden 16 - 19 February 2009 JRA2 Highlights JRA2 Highlights Scintillating Bolometers Scintillating Bolometers - Milano

Transcript of Stefano Pirroilias.in2p3.fr/.../ILIAS_6th_Annual_Meeting/180209_Pirro.pdfStefano Pirro Ilias 6 th...

  • • Background Limitation for Simple bolometers• Principles of operation• Cd-Mo based crystals• ZnSe crystals• Conclusions

    Stefano Pirro

    Ilias 6th Annual Meeting - Dresden 16 - 19 February 2009

    JRA2 Highlights JRA2 Highlights –– Scintillating Bolometers Scintillating Bolometers

    - Milano

  • Sum energy: 5407 keV

    210Po α

    line

    3600 keV

    Bkg in DBD region

    Continuum

    2530 keV

    CUORICINO TO CUOREA serious problem : Surface contaminationsA serious problem : Surface contaminations

  • Environmental “underground” Background:238U and 232Th trace contaminations

    Surface and Bulk contaminationsSurface and Bulk contaminations

    CUORICINO α

    Background

    130Te76Ge

    100Mo116Cd

    Furthermore a not negligible part of the background can arise from high energy neutrons from μ-spallation

    γ-region α-region

    82Se

  • Principles of operationPrinciples of operation

    τ=C/GΔT=ΔE/C

    A Bolometric Light Detector is fully active a particle detector

    The QE of a BLD is, probably close to 1 but it is rather difficult to measure it

    The time response of a BLD is the same of a standard bolometer O (ms)

  • Light Light DetectorsDetectors -- PerformancesPerformancesOur Light detectors are generally Pure Germanium disks (thickness 0.3-1 mm) . The Performance of a LD are normally evaluated through the Energy resolution on the 55Fe doublet (6 & 6.5 keV X-Ray)

    Ge (Ø = 66 mm)

    FWHM=550 eV

    Ge (Ø = 35 mm)

    FWHM=250 eV

  • Our SetupOur Setup

    3x3x3 cm3 CaF2

    3x3x6 cm3 CdWO4

    3x3x2 cm3 CdWO4

    Reflecting foils

    Light detectors

  • Li2

    MoO4

    ZrO2

    Good Scintillation light Poor Scintillation light No Scintillation light

    MgMoO4

    TeO2

    SummarySummary of (of (almostalmost) ) allall the the measuredmeasured crystalscrystals

    ZnSe

    PbMoO4

    SrMoO4

    CdMoO4

    CdWO4

    CaF2

    CaMoO4ZnMoO4

  • ResultsResults on the first on the first arrayarray of CdWOof CdWO44

    crystalscrystals

    (1)(1)

    Reflecting Foil

    Coupled with a light detector

    In may 2008 we performed the first measurement of an Array of 5 CdWO4 crystal to finallydemonstrate the feasibility of this technique

    3x3x6 cm3 (420 g) CdWO4

  • ResultsResults on the first on the first arrayarray of CdWOof CdWO44

    crystalscrystals

    (2)(2)

    CdWO4 – 3x3x6

    4 3x3x3 cm3 (215 g each) CdWO4

    1 common LD facing the 4 crystals

  • ResultsResults on the first on the first arrayarray of CdWOof CdWO44

    crystalscrystals

    (3)(3)

    Internal Roman lead shield

    CdWO4 3x3x6 cm3

    4 CdWO4 3x3x3 cm3 crystal array

    Large light detector

    CUORE test crystal

    Small light detector

  • ResultsResults on the first on the first arrayarray of CdWOof CdWO44

    crystalscrystals

    (4)(4)The data analysis on the 4 3x3x3 cm3 crystals is not finished. The data on the single 3x3x6 cm3 crystal is presented here.The obtained scatter plot is shown it corresponds to 1066 hours of background measurement

    Back

    groun

    d-Free

    area

    2615 keV 208Tl γ

    The MC simulation predicts a background level of 10-4 c/keV/kg/y in the region of interest

    44 days background

  • ResultsResults on on ““largelarge”” crystalscrystals –– CaMoOCaMoO44

    CaMoO4 is not a “perfect candidate” for future DBD Experiment since it contains 48Ca

    But this compound did show an extreme interesting feature

    Decay time of the CaMoO4 crystal – no light detection

    CaMoO4 Bolometers permits alpha discrimination without Light detection !!!!

    Rise time of the CaMoO4 crystal – no light detection

    147Sm- 2310 keV

  • ZnMoOZnMoO4 4 –– A promising MolibdateA promising Molibdate

    A 22 g ZnMoO4 crystal was grown by Institute for Scintillation Materials (Kharkov, Ukraine) In collaboration with by Institute for Nuclear Research (Kiev, Ukraine)

    226Ra, 222Rn, 218Po, 214Bi-214Po

    (56 mBq/kg)

    210Pb

    (360 mBq/kg)

  • ZnSe ZnSe –– an extremely interesting compound (1)an extremely interesting compound (1)

    ZnSe crystal was/is an extremely puzzling and interesting material.ZnSe crystal has a huge scintillation output but the emission spectra is close to the absorption spectra (λ≈1 mm)

    It normally doped with Te in order to increase the overall light output (we tested UNDOPED crystals)

    4 cm dia, 1.7 cm height, 120 g

    2 cm dia 3 cm height, 39 g

  • ZnSe ZnSe –– an extremely interesting compound (2)an extremely interesting compound (2)

    In the first run we observed a “very” strange scatter plot

  • ZnSe ZnSe –– an extremely interesting compound (3)an extremely interesting compound (3)Li

    ght S

    igna

    l [a

    u]

    Energy [keV]

    224Ra α-source

    ZnSe

    “Matted” – non optical – surface lapped with 3÷20 μm Al2 O3 powder

    “near optical” optical – surface

    Light detectorLi

    ght S

    igna

    l [a

    u]

    Energy [keV]

  • ZnSe ZnSe –– an extremely interesting compound (4)an extremely interesting compound (4)

    Energy [keV]

    Ligh

    t Sig

    nal

    [au]

    Energy [keV]

    Ligh

    t Sig

    nal

    [au]

    224Ra α-source

    ZnSe

    “Matted” – non optical – surface lapped with 3÷20 μm Al2 O3 powder

    “near optical” optical – surface

    Light detector “Penetration”: 6%

  • ZnSe ZnSe –– an extremely interesting compound (5)an extremely interesting compound (5)

    The “penetration” of alpha particles in the “beta” scintillation region seems to depend on the “surface”

    In fact we believe it depends on the residual lapping (non scintillating) powder on the crystal surface

    XRF Analysis

    We have other clear evidence for this explanation, but other tests will be made in order to proof and in order to AVOID this problem

  • ZnSe ZnSe –– an extremely interesting compound (6)an extremely interesting compound (6)

    But the “major” (nice) surprise comes from the time development of the Scintillation Signal

    The scintillation signal has a difference in the O(10ms) range. This effect is absolutely unexpected, even at very low temperatures

  • ZnSe ZnSe –– an extremely interesting compound (7)an extremely interesting compound (7)

    Looking at the coincidences between Heat in ZnSe and “Light” in the light detector, threepopulation appears

    β/γ

    α

    Ionizing particles

  • ZnSe ZnSe –– an extremely interesting compound (8)an extremely interesting compound (8)

    Another important feature is the Decay time of thermal signals in ZnSe(No light signal considered)

    337 g “new” ZnSe Crystal

  • SummarySummary

    116Cd CdWO482Se ZnSe

    100Mo …. ZnMoO4

    Reproducibility Radiopurity Availability α/n rejection

    β

    LY QF(α/β)keV/MeV [%]

    CdWO4 34 19ZnSe (Red) 7.4 420

    ZnSe (Yellow) 1.6 395ZnMoO4 1.4 16

  • ConclusionsConclusions

    We tested several types of scintillating crystals with interesting ββ

    emitters (100Mo,116Cd, 82Se, 48Ca)

    Within them CdWO4 gave excellent results

    The first measurements of ZnSe are very promising, even if some more tests are needed

    Molibdates needs more R&D both for radioactivity and scintillation light

    This technique is the only one that can be used for several interesting DBD emitters with excellent energy resolution.

    The energy resolution needed to go towards direct hierarchy can be achieved only by bolometers and Semiconductors…

  • BackupsBackups

  • Background Suppression : Bulk contaminationsBackground Suppression : Bulk contaminations

    Thanks to Bi-Po’s and Beatles internal contaminations do not play a significant role

    BI-Po

    Bi-Tl“BEATLE”

    Does not hold for 234Pa (Q=2195 keV)

  • Background analisys 3x3x6 crystal (2)

    γ- Background - It is rather low

    α

    Background

  • Data Analisys- results on the 4 3x3x3 crystals

  • CaCaFF22

    resultsresults

    There is a lack of an actual calibration due to the “lightness”

    of the compound

    JRA2 Highlights – Scintillating Bolometers A serious problem : Surface contaminations Surface and Bulk contaminationsPrinciples of operation Light Detectors - PerformancesOur SetupSummary of (almost) all the measured crystalsResults on the first array of CdWO4 crystals (1)Results on the first array of CdWO4 crystals (2)Results on the first array of CdWO4 crystals (3)Results on the first array of CdWO4 crystals (4)Results on “large” crystals – CaMoO4ZnMoO4 – A promising MolibdateZnSe – an extremely interesting compound (1)ZnSe – an extremely interesting compound (2)ZnSe – an extremely interesting compound (3)ZnSe – an extremely interesting compound (4)ZnSe – an extremely interesting compound (5)ZnSe – an extremely interesting compound (6)ZnSe – an extremely interesting compound (7)ZnSe – an extremely interesting compound (8)Summary ConclusionsBackupsBackground Suppression : Bulk contaminationsBackground analisys 3x3x6 crystal (2)Data Analisys- results on the 4 3x3x3 crystalsCaF2 results