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Nuclear Spectrometry Users’ ForumNPL 22nd May 2007
Neutron SpectrometryDavid Thomas
Neutron Metrology National Physical Laboratory, UK
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Introduction
• Why do neutron spectra need to be measured?
• Why is it difficult? C.f photon spectrometry
• How neutron spectrometry is done
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Reasons for making neutron spectrum measurements
• Photon spectrometry is performed for: radioisotope identification (including absolute measurements), activation analysis, nuclear physics, PIXE, PIGE, etc.
• In general neutron spectrometry is performed for different reasons
• Neutron spectrometry measurements may be made, for example, to validate shielding calculations, for nuclear physics experiments, or to characterise calibration fields, but much of the development of neutron spectrometry has been to enable measurements of neutron spectra for radiation protection
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Rationale for neutron spectrometry
10-3 10-2 10-1 100 101 102 103 104 105 106 10710-1
100
101
Personal dosemeters Albedo dosemeter Track etch device
Thermal
Under- and over-read for samples of area survey meters andpersonal dosemeters
Dosemeters.opj
Area survey instruments Leake survey meter LB6411 survey meter
Dos
e eq
uiva
lent
resp
onse
Neutron energy (eV)
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Why is neutron spectrometry difficult?C.f. photon spectrometry
Photons interact primarily with electrons -importance of photoelectric effect -electron acquires all the energy of the gamma ray
Neither photons or neutrons are directly ionising. To detect them they need to be converted to directly ionising particles
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Neutron spectrometry
• There is no real equivalent of the photoelectric effect for neutrons
• At low energies some reactions with low-Z nuclei can be used to transfer the neutron energy to charged particles: e.g.
• Note: both products are charged and can be detected
Reaction Q value3He(n,p)T 764 keV6Li(n,α)T 4.78 MeV
10B(n,α) 7Li 2.79 MeV
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3He or 6Li sandwich spectrometer
Neutron
3Heor
6Li
ChargedParticle
Detectors
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3He Sandwich Spectrometer
Complex electronics
Extremely low efficiency
In no way is it a field instrument
But: it works well in the lab
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241Am-B spectrum measured with a 3He sandwich spectrometer
0 1 2 3 4 5 60.0
0.1
0.2
0.3
0.4
0.5
37 GBq Am-B
Flue
nce
per u
nit e
nerg
y (c
m-2 M
eV-1)
Neutron energy (MeV)
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3He Proportional Counter Spectrum for Monoenergetic Neutrons
480 keVmonoenergetic
neutrons
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3He Proportional Counter in field with thermal neutrons
0 400 800 1200 1600 2000 2400100
101
102
103
104
105
106
107C
ount
s
Energy (keV)
Pulse height spectrum for a 3He gridded ionisation chamber in a realistic neutron field
764 keV
Pulser peak
Pile-uppeak
Energy region of interest
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Use of (n,p) Scattering in Neutron Spectrometry
• One of the most important reactions in neutron spectrometry is (n,p) scattering
• When a neutron collides with a hydrogen nucleus some of the neutron energy is transferred to the recoil proton
• The actual amount depends on the scattering angle
Incident neutron
Recoiling proton
Scatteredneutron
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Use of (n,p) Scattering in Neutron Spectrometry
2
o
(cos )
recoil scattering angle, when =0 p n
p n
E E
E E
θ
θ θ
=
= =
If the recoils can be restricted to those where θ ~ 0o get a measure of En
This is the principle of the proton recoil telescope
Chargedparticledetector
Neutron Recoil proton
Radiator (CH2)
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Use of (n,p) Scattering in Neutron Spectrometry
• If the restriction to θ ~ 0o is removed get a much higher detection efficiency
• However, this introduces the requirement to unfold the spectrum
• Nevertheless proton recoil spectrometers are one of the most commonly used
• There are two basic types:-
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Use of (n,p) Scattering in Neutron Spectrometry
Scintillator
Proton
Scatteredneutron
Proton
Hydrogen-filledproportional
counter
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A proton recoil proportional counter
60 80 100 120 140 160 180
0
500
1000
1500
2000
2500
Cou
nts
Energy (keV)
Measured Calculated
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Characteristics of proton recoil proportional counter spectrometers
Broad pulse height distribution even for monoenergetic neutrons.
Unfolding needed to derive the neuron spectrum from the pulse height distribution.
Response functions must be known, but can be derived from measurement and calculation.
Need several counters (3 or 4) to cover energy range (roughly 50 keV to 1.5 MeV).
For higher energies can use methane or 4He counters, but scintillators are better.
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Scintillator spectrometer e.g. NE213
Similarities to proportional counters, but:more efficient,must have n-γ discrimination, andonly one counter needed to cover 1 MeV to >20 MeV.
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Summary for proton recoil devices
High resolution.
Cover an important portion of the neutron energy region where a significant fraction of the dose is often located.
Not particularly easy to use or unfold –often need to combine data from several detectors.
Still to some extent under development, digital signal processing being investigated.
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Scintillator measurement of 241Am-Be compared with 3He sandwich spectrometer
NPL 10 Ci241Am-Besource
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Energy Range for Neutron Spectra
10-3 10-2 10-1 100 101 102 103 104 105 106 1070.00
0.05
0.10
0.15
0.20
0.25
E.Φ
E o
r H*(
10) (
Nor
mal
ised
to u
nity
)
Neutron Energy (eV)
Neutron fluence per unit lethargy Ambient dose equivalent, H*(10)
Range for nuclearrecoil spectrometers
Range for Bonner sphere spectrometers
Fraction of total H*(10) for reactor spectrum shown
69.6% 10.8%19.6%
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Principle of operation
Escape
Capture in thepolyethylene
Capture in thethermal sensor
Thermalsensor
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Response Functions of Bonner spheres
10-3 10-2 10-1 100 101 102 103 104 105 106 1070
1
2
3
4
5
6
Flue
nce
resp
onse
(cm
2 )
Neutron energy (eV)
Bare 6.0" 3.0" 8.0" 3.5" 10.0" 4.0" 12.0" 5.0" 15.0"
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Bonner sphere spectra from comparison exercise
10-3 10-2 10-1 100 101 102 103 104 105 106 1070
5
10
15
20
25
30
35
MCNP Calcn. AECL BfS IPSN-Cad
Flue
nce
per u
nit l
etha
rgy
(cm
-2 α
-1)
Neutron energy (eV)
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Schauinsland: 1195 m
Schneefernerhaus: 2650 m
Neutron spectrometry: outside the lab, all Bonner spheresNeutron spectrometry: outside the lab, all Bonner spheres
Outside containment UK South Coast
Inside containment
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Characteristics of neutron spectrometers
Property3He
SpectrometersNuclear Recoil
DevicesBonner Spheres
Energy resolution Good
50 keV to ~6 MeV
Low
Bulky
Straightforward
Photons OKThermals problem
Not very isotropic
Reasonable straightforward
Good Poor
Energy range 50 keV to 20 MeV Thermal to >20 MeV
Efficiency Low to medium High
Size & mass Bulky Large
Operation Complex Simple
Photon discrimination
Pulse shape analysis essential
for scintillatorsExcellent
Angle response Near isotropic Isotropic
Unfolding Solvable but complex
Complex and subjective
Bonner spheres have been used for more field measurements than all the other devices put together