Experimental Techniques for Nuclear and Particle …...Experimental Techniques for Nuclear and...
Transcript of Experimental Techniques for Nuclear and Particle …...Experimental Techniques for Nuclear and...
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Introduction to scintillators
Experimental Techniques for
Nuclear and Particle Physics
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Properties: - Should convert the kinetic energy of charged particles into detectable light with high efficiency - The conversion should be linear - The medium should be transparent to the wavelength of its own emission for good light collection - The decay time of the induced luminescence should be short so that fast signal pulses can be generated - The material should be of good optical quality and subject to manufacture in sizes large enough to be of interest - Its index of refraction should be near that of a glass (n≈1.5) to permit efficiency coupling of the scintillation light to a photomultiplier tube or other light sensor
Scintillators
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Incident particles or photons excite atoms or molecules in the scintillating medium Excited states decay under emission of photons, which are detected and converted into electric signals. Light yield - number of emitted photons/MeV
10 - 120 000 photons/MeV λ – wavelength of the emitted light
typically 200 – 700 nm (UV –visible red) Time constant for the emitted light
~ 0.6 ns – 100 µs Scintillation materials: Both organic and inorganic materials Can be in solid, liquid or gaseous state
Scintillators
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● Inorganic scintillators Best light output and linearity but slow in their response
time Intrinsic crystals BaF2, CdWO4, CsF, etc Doped crystals NaI(Tl), CsI(Tl), ZnSe(Te), LSO(Ce), LaBr3(Ce) etc
● Organic scintillators Generally faster but yield less light Plastic Liquid scintillators
Some crystals show two or more light components with different wave lengths and time constants.
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Solid state detectors Scintillators Si, Ge + good energy resolution - poor energy resolution ~ 0.1 % + electronic segmentation typically > ~5 % at best - slow + fast – slow - low stopping power + high – low stopping power ----------------------------------------------------------------------- wide bandgap semiconductors new materials CdTe, CdZnTe, HgI2 e.g. LaBr3(Ce) + high stopping power + electronic segmentation + high light yield (~70 ph/keV) - energy resolution ~ 1 %
+ energy resolution ~ 3 % + fast (τ~20ns)
Typical scintillator properties compared to semicionductor detectors
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Organic scintillators
• The states of interest are energy levels of individual molecules, i.e. no interactions with neighbours.
• excitation and emission spectra
practically the same whether in solid, liquid or gaseous state.
• Low stopping power for gamma radiation. • Mostly used for detection of neutrons
and charged particles.
plastic scintillators liquid scintillators
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Conduction band
Activator excited states
Activator ground state
valence band
band gap (forbidden band)
If forbidden band >> kT, no electrons in conduction band. è insulator Radiation excites electron from valence into conduction band, forming an electron-hole pair. Electrons in conduction band and holes in valence band can move freely throughout crystal.
Inorganic scintillators
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Scintillation photons are emitted from activator excited states, fast transition, visible light.
Competing processes: Electron arrives to excited states from which transition to ground state is forbidden. Additional small energy is required to lift the electron to other excited states (thermal excitation) with higher transition probability. This results in phosphorescence radiation, or ”afterglow”, which is a slow time component.
Some excited states cause radiationless transitions, which represents loss mechanism in the conversion of the radiation energy to scintillation light. This is the quenching effect.
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Egap [eV] Ee-h [eV] Si 1.12 3.61 Ge 0.74 2.98 CdTe 1.47 4.43 HgI2 2.13 4.2 NaI(Tl) 5.9 15.3 CsI(Tl) 6.5 15.2
Band gap energies in semiconductors and scintillators
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See http://scintillator.lbl.gov for updated and complete table
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Scintillation efficiency Energy required to generate one e-h pair
Ee-h=βEgap β≈2.3 (2-3) CsI(Tl) Egap=6.4 eV assume Eγ=1 MeV Number of light photons 1 MeV/(2.3xEgap)= 1 000 000 eV/(2.3x6.4 eV)≈67 000 ph
compare with measured 60 000 ph NaI(Tl) Egap=5.9 eV 1 000 000 eV/(2.3x5.9 eV)≈73 000 ph
measured 40 000 ph
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BaF2 (fastest commercial scintillator) fast component Egap=18.0 eV
1 000 000 eV/(2.3x18.0 eV) ≈ 24 000 ph
measured 2200 ph
slow component Egap=10.6 eV
1 000 000 eV/ (2.3x10.6 eV) ≈ 41 000 ph
measured 7000 ph Most crystals show very low efficiency for the scintillation
process
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Scintillation process - conversion to e-h pairs - transfer to luminescence centre - luminescence, i.e. photon emission
Nph=(Eγ/Ee-h)SQ S – transfer efficiency of the e-h pair to luminescence
centre Q – efficiency for photon emission
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Decay times
Radiative decay time for electric dipole emission τr~λ2
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Tradeoff: timing – energy resolution
High light yield → low energy gap crystals → long wavelength of the scintillation light Fast crystals → short wavelength (UV region) → high energy gap
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Amplifier MCA
scintillator photodetector PIN photodiode Photomultiplier (PM-tube) avalanche photodiode
How to measure light yield
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Photomultiplier These detectors multiply the current produced by incident light by as much as 100 million times in multiple dynode stages, enabling individual photons to be detected when the incident flux of light is very low
Photocathode: convert light photons into low energy electrons (photoemission)
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Nphotons=Nphe/Q.E(λ)
number of photons entering PM-tube
number of photoelectrons emitted from the photocathode
Quantum Efficiency
Photomultiplier
Quantum efficiency around 20-30 % Strong function of the wavelength of the incident light
Secondary electron emission Overall multiplication factor: δ = n° of secondary electrons emitted/primary incident electron
Gain of the PM = αδΝ
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Higher quantum efficiency Lower power consumption Compact size Insensitive to magnetic fields
Photodiodes
Nphotons=Ne-h/Q.E(λ)
number of electron-hole pairs
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Energy resolution (ΔE/E)2=(δintr)2+(δst)2+(δn)2
δintr – intrinsic resolution of the crystal
δst – statistical contribution δn – dark noise contribution For PM-tubes δst =2.35x(1/Nphe)1/2x(1+ε)1/2
ε – variance of the electron multiplier gain For avalanche photodiodes (APD) δst =2.35x(F/Ne-h)1/2
F – excess noise factor, reflecting statistical fluctuation of the APD gain Energy resolution strongly depends on Nphe, alt. Ne-h
–
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Light yield non-proportionality ideal case:
E
channel number (light yield)
l.y./E
E
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Light yield non-proportionality
This assumption is based on two requirements: (1) the light output of the scintillator is proportional to
the energy of the incident radiation; (2) the electrical pulse produced by the photomultiplier
tube is proportional to the emitted scintillation light.
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In real life
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Electron response
Most scintillators show light yield non-proportionality, due to non-proportional electron response.
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Temperature dependence
In organic scintillators the light output is practically independent of the temperature between -60° and 20°
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room temp. LN2 temp. energy light yield energy light yield resolution resolution [%] [ph/MeV] [%] [ph/MeV]
pure NaI 16.5 3800 4.3 84 000 BGO 10.0 6900 6.5 29 000 pure CsI 2000 4.3 124 000 -------------------------------------------------------------------------------------------------------------- CsI(Tl)
Number of light photons 1 MeV/(2.3xEgap)= 1 000 000 eV/(2.3x6.4 eV)≈67 000 ph
compare with measured 60 000 ph --------------------------------------------------------------------------------------------------------------
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Dopants λ τ light yield [nm] [ns] [ph/MeV]
undoped CsI 315 16 2000 CsI(Tl) 540 800/6000 60 000 CsI(Na) 420 630 37 000 CsI(CO3) 405 2000 26 000
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● Light yield depends on the charge, mass and energy of the detected particles
● For some scintillators with two light
components (fast and slow components) the amplitude ratio of the two components varies with the particle types and there is a change in the decay constant with the density of ionization of the particle, mainly the short decay constant, e.g. CsI(Tl).
Particle identification
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Johan Nyberg
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Johan Nyberg
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CsI(Tl) has intrinsic particle discrimination properties due to its different decay components
L1, L2 are light outputs from integrating the signal within short and long time intervals
CsI(Tl)
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phoswich detectors
fast crystal (plastic scint.)
slow crystal
photodetector (PMT, photodiode)
L1, L2 are light outputs from integrating the signal within short and long time intervals
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phoswich detectors The Comprehensive Nuclear-Test-Ban Treaty establishes a network of monitoring stations to detect radioactive xenon in the atmosphere from nuclear weapons testing. Detect beta-gamma coincidences from the Xe isotope of interest
- CsI(Tl) crystal to measure gamma rays - Plastic scintillator BC-404 to measure the electrons
Coincidence events form two horizontal bands, corresponding to 30 keV X-rays or 81 keV gamma rays in coincidence with betas of varying energy
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Radiation hardness Scintillators, like other detector materials, are
sensitive to high radiation doses. Radiation damage is exhibited in form of lowered light
yield and optical transmission.
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Optical transmission
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Recovery (optical transmission)
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Problems
If the energy resolution of a particular NaI(Tl) scintillation detectors is 7% for 137Cs gamma rays (662 keV), estimate its energy resolution for the 1.28 MeV gamma rays of 22Na
Solution: R=FWHM/Ho with
FWHM: FWHM of the full energy peak Ho: mean pulse height corresponding to the same peak
Therefore, R=K/E1/2
K=RCsECs0.5=7%*662 keV=5.695
RNa=5.695/ENa0.5=5.695/12800.5=5.03%
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Solution:
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Solution: