Shielding Strategies. Karl Tasso Knöpfle MPI Kernphysik, Heidelberg

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Transcription:

Shielding Strategies Karl Tasso Knöpfle MPI Kernphysik, Heidelberg ktkno@mpi-hd.mpg.de Application of Germanium Detector in Fundamental Research Tsinghua University Bejing, March 24-26, 20011

outline Introduction Shielding against external background cosmics natural long-lived activities examples passive shields Surface contamination active shields Intrinsic background Ultimate designs? Conclusion 2

our radiation environment England Germany total: 2.6 msv / a (NPL-UK 2008) (PTB-BMU 2003) 1mSv ~ 80 kbq 3

Introduction the need for shielding Ge-76 T1/2 ln2 Natom time = = Ndcy 5.47 1024 (mass / kg) (time / yrs) Ndcy [yrs] 90% confidence limit (C.L.) in case of zero event (F.C.: Ndcy=2.44): T1/2 > 2.2 1024 (m / kg) (t / yrs) [yrs] increase mass and time, too naïve: 2) sensitivity in case of background : Ndcy Nbgnd + Ndcy ~ c b m t ΔE Ge-76 b: background index in [cts/(kg kev yrs)] 0.1 3.3 ΔE: resolution [kev] T1/2 > const (m t) / (B ΔE) reduce background index b optimize energy resolution ΔE *RevModPhys 80(08)481 4

Introduction it s all about background no count 0.0001 0.001 0.01 Caldwell & Kröninger, PRD74 (2006) 092003 5

cosmic rays G.Heusser Cosmics produce backgrounds by direct interaction and activation 75% muons on sea level, rest pions, protons, neutrons, electrons, gamaas 6

cosmic rays G.Heusser 7

cosmic rays see talk by B. Schwingenheuer 8

cosmic rays vertical muon intensity 9

cosmic rays muon induced neutron flux Mei and Hine, PRD 2006 low-z preferred! NB: Low energy neutrons are also produced by fission and (α,n) reactions! Conflicting predictions for hard component spectrum, measure n-spectra 10

cosmic rays Even deep underground, shielding is needed against muons standard active veto fast/slow neutrons difficult, composite high/low-z passive shields 11

natural long-lived activities Rn-222 Rn-220 12

shielding against radon Rn-222 (Rn-220,-219): gaseous, highly volatile/penetrating! ~40 Bq/m^3, in salt mines less (screen materials and setup) UHV tight experimental setup, (metal seals only) 13

Heidelberg-Moskau Experiment. background spectra spectra measured at LNGS with Ge diode Bi-214 unshielded Background Index Tl-208 shielded predominantly external γ-rays GERDA phase I 14

Heidelberg-Moskau Gerd Heusser Exp. : One option for background reduction is to immerse the almost bare crystals in liquid N, which would serve as a shield. background spectra spectra measured at LNGS with Ge diode Bi-214 unshielded Tl-208 Background Index Ann.Rev.Nucl.Part.Sci.1995. 45:543 shielded predominantly external γ-rays GERDA phase I 15

(μbq/kg) 3000000 ~ 5000 <20 <1 ~0 background spectra spectra measured at LNGS with Ge diode Bi-214 unshielded Tl-208 Background Index Activity of Tl-208 rock, concrete stainless steel Cu(NOSV), Pb water, purified LN2, LAr shielded predominantly external γ-rays GERDA phase I 16

intrinsic contamination of shielding materials Material activity [ μbq / kg ] Ra-226 (U) Th-228 K-40 misc 10-3: Ar-39 liq. nitrogen <0.3* - - liq. scintillator (PC) 10-6 <10-6 <10-3 water <1 0.008 <2 liq. argon 600* - - 106: Ar-39, ~150:Ar-42 steel 130 <40 50 140: Co-60 copper <16 9,<19 <88 <10: Co-60 Lead <29 <22 270 <4000: Pb-210 * Rn-222 Thickness for 10-6 attenuation of 2.61 MeV gamma rays [ cm ] Data from G. Heusser, LNGS DBD workshop 2010 17

GERDA graded shield options log(surface activity for 2.6 MeV γ) [Bq/cm2] required attenuation factor 2.5 10-8 baseline: water / copper / LN (none of them implemented!) alternative: water / steel / lead / LN material thickness [m] many possibilities to comply with constraints like feasibiliy, size, cost, 18

generic external background shields GERDA (low Z shield) Majorana (high Z shield; deep underground) bare Ge diodes in high-purity LAr Ge diodes housed in vacuum cryostat, ultra-high-purity electroformed Cu shield < 1μBq/m3 STP Rn-222 (established) water: γ & n shield, Cherenkov medium for μ veto stainless steel cryostat w Cu shield, Rn tight also active shield! LAr H 2.5 m source=detector 10 cm electroformed Cu H 10 m bare Ge diodes < 1 μbq/kg Th-232 (not yet established) 45 cm lead Ø 2.1 m Ø4m 30 cm PE, active μ veto, Rn tight box Ø 10 m α(lar) = 0.050/cm α(cu) = 0.34/cm α(h2o) = 0.043/cm α(pb) = 0.48/cm 19

examples GERDA & Majorana Majorana GERDA bare enrge array in liquid argon shield: high-purity liquid Argon / H2O array(s) of enrge housed in high-purity electroformed copper cryostat shield: electroformed copper / lead 20

GERDA location 3800 m w.e. Gran Sasso - Italy GERDA in Hall A of LNGS LNGS: Laboratori Nazionali del Gran Sasso

GERDA clean room with lock f muon & cryogenic infrastructure cryostat with internal Cu shield control rooms 14.8m water plant & radon monitor water tank, Ø10m, part of muon detector) 22

Majorana setup 5000 m w.e. rock above vacuum cryostat of electroformed Cu, 40 kg, Ø & H: 400 mm 57 segmented n-type Ge-76 diodes (60 kg) μ-veto lead cold finger PE electroformed Cu monolith μ-induced events vs depth dewar 23

active shielding discrimination of single / multi site events SSE (2ββ) MSE (Compton sc) anti-coincidence MSE (intrinsic) pulse shape analysis segmentation anti-coincidence 24

active shielding discrimination of single / multi site events LAr scintillator MSE (Compton sc) anti-coincidence Ge diode - LAr SSE (2ββ) 25

R&D liquid argon instrumentation Low background GERDALArGe test facility @ LNGS: Detection of coincident liquid argon scintillation light to discriminate background see talk by D. Budjas 9x 8 ETL9357 Operation of GERDA BEGe detector prototype in LArGe: Measured suppression factor at Qβ β : ~0.5 104 for a near 228Th calibration source (M. Heisel, PhD thesis, Heidelberg 2011) Potential problem:ar-42 decay to K-42 with Qβ(K-42)=3.5MeV 26

self-shielding & fiducial volume cleanlinest place on/under earth! Franco, APC 2010 buffer Ø3m water position sensitive 27

fiducial volume for Ge diodes? Yes! (trivial if position sensitive) deadlayer Practical: p-type Ge diode with ~1mm thick Li-diffused contact, material loss ~6% n-type ultrapure coating?! Possible - but affordable?: 3d array of ~1000 Ge-diodes, material loss ~50% 28

ultimate segmentation: pixelisation Particle ID by tracking in pixel detector (TimePix: alpha 1 pixel beta t=1mm, 1.4x1.4 cm2, 55μm pixel pitch) muon connected pixels gamma disconnected pixels K.Zuber taup09 Exploit topology! 29

conclusions Effective shielding is crucial for next generation of double beta decay experiments. Both passive and active shields needed Two competing concepts for passive shields (Majorana GERDA) being realized conventional high Z (Cu, Pb) graded shield with extra muon veto & neutron absorber (How large are contaminations of electroformed copper?) novel low Z (water, LN, LAr?) graded shield with integral muon veto & neutron absorber (latter approach is much more demanding w.r.t. space, infrastructure, safety) Adequate screening of all shielding materials/volumes essential; dto mounting material! Promising R&D results for active veto if LAr: use depleted argon?! Transfer of concepts from other successful low counting experiments might be useful fiducial volume pixelisation in-situ cleaning of shield & detector, (practical for Ge?) 30