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Radiation Detection and Counting Statistics

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Title: Radiation Detection and Counting Statistics


1
Radiation Detection and Counting Statistics
  • Please Read Chapters 3 (all 3 parts), 8, and 26
    in Doyle

2
Types of Radiation
  • Charged Particle Radiation
  • Electrons
  • b particles
  • Heavy Charged Particles
  • a particles
  • Fission Products
  • Particle Accelerators
  • Uncharged Radiation
  • Electromagnetic Radiation
  • g-rays
  • x-rays
  • Neutrons
  • Fission, Fusion reactions
  • Photoneutrons

Can be easily stopped/shielded!
More difficult to shield against!
3
Penetration Distances for Different Forms of
Radiation
as
bs
gs
ns
Paper
Plastic (few cm)
Lead (few in)
Concrete (few feet)
4
Why is Radiation Detection Difficult?
  • Cant see it
  • Cant smell it
  • Cant hear it
  • Cant feel it
  • Cant taste it
  • We take advantage of the fact that radiation
    produces ionized pairs to try to create an
    electrical signal

5
Ideal Properties for Detection of Radioactivity
6
How a Radiation Detector Works
  • The radiation we are interested in detecting all
    interact with materials by ionizing atoms
  • While it is difficult (sometime impossible) to
    directly detect radiation, it is relatively easy
    to detect (measure) the ionization of atoms in
    the detector material.
  • Measure the amount of charge created in a
    detector
  • electron-ion pairs, electron-hole pairs
  • Use ionization products to cause a secondary
    reaction
  • use free, energized electrons to produce light
    photons
  • Scintillators
  • We can measure or detect these interactions in
    many different ways to get a multitude of
    information

7
General Detector Properties
  • Characteristics of an ideal radiation detector
  • High probability that radiation will interact
    with the detector material
  • Large amount of charge created in the interaction
    process
  • average energy required for creation of
    ionization pair (W)
  • Charge must be separated an collected by
    electrodes
  • Opposite charges attract, recombination must be
    avoided
  • Initial Generated charge in detector (Q) is very
    small (e.g., 10-13C)
  • Signal in detector must be amplified
  • Internal Amplification (multiplication in
    detector)
  • External Amplification (electronics)
  • Want to maximize V

8
Types of Radiation Detectors
  • Gas Detectors
  • Ionization Chambers
  • Proportional Counters
  • Geiger-Mueller Tubes (Geiger Counters)
  • Scintillation Detectors
  • Inorganic Scintillators
  • Organic Scintillators
  • Semiconductor Detectors
  • Silicon
  • High Purity Germanium

9
Gas Detectors
  • Most common form of radiation detector
  • Relatively simple construction
  • Suspended wire or electrode plates in a container
  • Can be made in very large volumes (m3)
  • Mainly used to detect b-particles and neutrons
  • Ease of use
  • Mainly used for counting purposes only
  • High value for W (20-40 eV / ion pair)
  • Can give you some energy information
  • Inert fill gases (Ar, Xe, He)
  • Low efficiency of detection
  • Can increase pressure to increase efficiency
  • g-rays are virtually invisible

10
Ionization Chambers
  • Two electric plates surrounded by a metal case
  • Electric Field (EV/D) is applied across
    electrodes
  • Electric Field is low
  • only original ion pairs created by radiation are
    collected
  • Signal is very small
  • Can get some energy information
  • Resolution is poor due to statistics, electronic
    noise, and microphonics

Good for detecting heavy charged particles, betas
11
Proportional Counters
  • Wire suspended in a tube
  • Can obtain much higher electric field
  • E ? 1/r
  • Near wire, E is high
  • Electrons are energized to the point that they
    can ionize other atoms
  • Detector signal is much larger than ion chamber
  • Can still measure energy
  • Same resolution limits as ion chamber
  • Used to detect alphas, betas, and neutrons

12
Examples of Proportional Counters
13
Geiger Counters
  • Apply a very large voltage across the detector
  • Generates a significantly higher electric field
    than proportional counters
  • Multiplication near the anode wire occurs
  • Geiger Discharge
  • Quench Gas
  • Generated Signal is independent of the energy
    deposited in the detector
  • Primarily Beta detection
  • Most common form of detector

No energy information! Only used to count /
measure the amount of radiation. Signal is
independent of type of radiation as well!
14
Examples of Geiger Counters
Geiger counters generally come in compact, hand
carried instruments. They can be easily operated
with battery power and are usually calibrated to
give you radiation dose measurements in rad/hr
or rem/hr.
15
Scintillator Detectors
  • Voltage is not applied to these types of
    detectors
  • Radiation interactions result in the creation of
    light photons
  • Goal is to measure the amount of light created
  • Light created is proportion to radiation energy
  • To measure energy, need to convert light to
    electrical signal
  • Photomultiplier tube
  • Photodiode
  • Two general types
  • Organic
  • Inorganic

light ? electrons
16
Organic Scintillators
  • Light is generated by fluorescence of molecules
  • Organic - low atomic numbers, relatively low
    density
  • Low detection efficiency for gamma-rays
  • Low light yield (1000 photons/MeV) - poor signal
  • Light response different for different types of
    radiation
  • Light is created quickly
  • Can be used in situations where speed (ns) is
    necessary
  • Can be used in both solid and liquid form
  • Liquid form for low energy, low activity beta
    monitoring, neutrino detection
  • Very large volumes (m3)

17
Organic Scintillators Come in Many Forms
18
Inorganic Scintillators
  • Generally, high atomic number and high density
    materials
  • NaI, CsI, BiGeO, Lithium glasses, ZnS
  • Light generated by electron transitions within
    the crystalline structure of the detector
  • Cannot be used in liquid form!
  • High light yield (60,000 photons / MeV)
  • light yield in inorganics is slow (ms)
  • Commonly used for gamma-ray spectroscopy
  • W 20 eV (resolution 5 for 1 MeV g-ray)
  • Neutron detection possible with some
  • Can be made in very large volumes (100s of cm3)

19
Inorganic Scintillators
20
Solid State (Semiconductor) Detectors
  • Radiation interactions yield electron-hole pairs
  • analogous to ion pairs in gas detectors
  • Very low W-value (1-5 eV)
  • High resolution gamma-ray spectroscopy
  • Energy resolution ltlt 1 for 1 MeV gamma-rays
  • Some types must be cooled using cryogenics
  • Band structure is such that electrons can be
    excited at thermal temperatures
  • Variety of materials
  • Si, Ge, CdZnTe, HgI2, TlBr
  • Sizes lt 100 cm3 some even less than 1 cm3
  • Efficiency issues for lower Z materials

21
NaI Scintillator
Ge Detector
22
(No Transcript)
23
Ideal Detector for Detection of Radiation
Excellent table on Page 61 shows numerous
different technologies used in safeguards
24
Counting Statistics
25
Three Specific Models
  1. Binomial Distribution generally applicable to
    all constant-p processes. Cumbersome for large
    samples
  2. Poisson Distribution simplification to the
    Binomial Distribution if the success probability
    p is small.
  3. Gaussian (Normal) Distribution a further
    simplification permitted if the expected mean
    number of successes is large

26
The Binomial Distribution
n number of trials p probability of success
for each trial We can then predict the
probability of counting exactly x successes
P(x) is the predicted Probability Distribution
Function
27
Example of the Binomial Distribution
Winners 3,4,5, or 6
P 4/6 or 2/3 10 rolls of the die n10
28
Results of the Binomial Distribution
p 2/3 n 10
29
Some Properties of the Binomial Distribution
It is normalized
Mean (average) value
30
Standard Deviation
Predicted variance
Standard Deviation
s is a typical value for
31
For the Binomial Distribution
where n number of trials and p success
probability
Predicted Variance
Standard Deviation
32
For our Previous Example
p 2/3 n 10
33
The Poisson Distribution
Provided p ltlt 1
34
For the Poisson Distribution
Predicted Mean
Predicted Variance
Standard Deviation
35
Example of the Application of Poisson Statistics
Is your birthday today?
Example what is the probability that 4 people
out of 1000 have a birthday today?
36
Discrete Poisson Distribution
37
Gaussian (Normal) Distribution
p ltlt 1
Binomial
Poisson
Poisson
Gaussian
38
Example of Gaussian Statistics
What is the predicted distribution in the number
of people with birthdays today out of a group of
10,000?
39
Distribution Gaussian Distribution
40
The Universal Gaussian Curve
to f(to)
0 0
0.674 0.500
1.00 0.683
1.64 0.900
1.96 0.950
2.58 0.990
41
Summary of Statistical Models
For the Poisson and Gaussian Distributions
Predicted Variance
Standard Deviation
42
CAUTION!!
Does not apply directly to
  1. Counting Rates
  2. Sums or Differences of counts
  3. Averages of independent counts
  4. Any Derived Quantity

43
The Error Propagation Formula
Given directly measured counts (or other
independent variables)
x, y, z,
for which the associated standard deviations are
known to be
sx, sy, sz,
Derive the standard deviation of any calculated
quantity
u(x, y, z, )
44
Sums or Differences of Counts
u x y or u x - y
Recall
45
Example of Difference of Counts
total x 2612 background y
1295 net u 1317
Therefore, net counts 1317 62.5
46
Multiplication or Division by a Constant
47
Example of Division by a Constant
Calculation of a counting rate
x 11,367 counts t 300 s
? rate r 37.89 0.36 s-1
48
Multiplication or Division of Counts
49
Example of Division of Counts
Source 1 N1 36,102 (no BG) Source 2 N2
21,977 (no BG)
R N1/N2 36102/21977 1.643
? R 1.643 0.014
50
Average Value of Independent Counts
Sum S x1 x2 x3 xN
Average
Single measurement
Improvement Factor
51
For a single measurement based on a single count
Fractional error
x 100 1000 10,000
Fractional Error 10 3.16 1
52
Limits of Detection
  • In many cases within non-proliferation, you are
    required to measure sources that have a small
    signal with respect to background sources of
    radiation
  • Thus, we need to assess the minimum detectable
    amount of a source that can be reliably measured.
  • Lets look at an example of testing the limits of
    detection

53
Limits of Detection
Two basic cases No Real Activity Present Real
Activity Present
54
Limits of Detection No Source
Goal Minimize the number of false positives
(i.e., dont want to holdup many containers that
do not contain anything interesting)
Want to set critical counting level (LC) high
enough such that the probability that a
measurement Ns that exceeds Lc is acceptably
small. Assuming Gaussian distribution, we are
only concerned with positive deviations from the
mean. If we were to accept a 5 false positive
rate (1.645s or 90 on distribution), then
55
Limits of Detection Source Present
Goal Minimize the number of false negatives
(i.e., dont want to let many containers that
contain radioactive materials get through). Let
ND be the minimum net value of NS that meets this
criterion. We can then determine our lower
critical set point. Lets assume an acceptable 5
false negative rate.
Assumes the width of the distribution of the
source background is approximately the same as
that of the background only. In reality, these
widths are not the same.
56
Limits of Detection Source Present
57
Two Interpretations of Limits of Detectability
  • LC lower limit that is set to ensure a 5
    false-positive rate
  • ND minimum number of counts needed from a
    source to ensure a false-negative rate no larger
    than 5, when the system is operated with a
    critical level (or trigger point) LC that ensures
    a false positive rate no greater than 5

58
Neutron DetectionNeutron Coincidence Counting
59
Neutron Energy Classification
60
Slow Neutron Detection
Need exoenergetic (positive Q) reactions to
provide energetic reaction products
61
Useful Reactions in Slow Neutron Detection
10B (n, a) 7Li 6Li (n, a) 3H 3He (n, p) 3H (n,
fission)
62
The 10B(n,a) Reaction
63
10B (n, a) 7Li
Conservation of energy Eli Ea Q 2.31
MeV Conservation of momentum
64
Other Reactions
65
Detectors Based on the Boron Reaction
  1. The BF3 proportional tube
  2. Boron-lined proportional tube
  3. Boron-loaded scintillator

66
The BF3 Tube
  • Typical BF3 pressure lt 1 atm
  • Typical HV 2000-3000 V
  • Usual 10B enrichment of 96

67
BF3 Pulse Height Spectrum
68
Boron-Lined Proportional Tube
  • Conventional proportional gas
  • Detection efficiency limited by boron thickness

69
Boron-Lined Proportional Tube Pulse Height
Spectrum
70
Fast Neutron Detection and Spectroscopy
  • Counters based on neutron moderation
  • Detectors based on fast neutron-based reactions
  • Detectors utilizing fast neutron scattering

71
Moderated Neutron Detectors
72
Moderating Sphere
73
Moderating Sphere
74
Neutron Rem Counter
75
Long Counter
76
Long Counter Sensitivity
77
Application of the 3He(n,p) reaction the 3He
Proportional Tube
78
3He Proportional Counter
79
Detectors that Utilize Fast Neutron Scattering
  • Proton recoil scintillator
  • High (10 50) detection efficiency, complex
    response function, gamma rejection by pulse shape
    discrimination
  • Gas recoil proportional tube
  • Low (.01 - .1) detection efficiency, can be
    simpler response function, gamma rejection by
    amplitude
  • Proton recoil telescope
  • Very low ( .001) detection efficiency, usable
    only in beam geometry, simple peak response
    function
  • Capture-gated spectrometer
  • Modest (few ) detection efficiency, simple peak
    response function

80
Proton Recoil Scintillators
81
Recoil Proton Spectrum Distortions
82
Recoil Proton Detector Efficiency
83
Proton Recoil Telescope
84
Proton Recoil Telescope Response Function
Ep Encos2 ?
85
Capture-Gated Proton Recoil Neutron Spectrometer
86
Capture-Gated Spectrometer Timing Behavior
Accept first pulse for analysis if followed by
second pulse within gate period
87
Capture-Gated Spectrometer Response Function
  • Only events ending in capture deposit the full
    neutron energy
  • Energy resolution limited by nonlinearity of
    light output with energy (Two 0.5 MeV protons
    total yield less than one 1 MeV proton.)

88
Neutron Coincidence Counting
  • Technique involving the simultaneous measurement
    of neutrons emitted from a fission source (in
    coincidence with each neutron)
  • Used to determine mass of plutonium in unknown
    samples
  • Most widely used non-destructive analysis
    technique for Pu assay, and can be applied to a
    variety of sample types (e.g., solids, pellets,
    powders, etc.)
  • Requires knowledge of isotopic ratios, which can
    be determined by other techniques
  • Also used in U assay

89
Neutron Distribution from Pu Fission
90
Neutron Coincidence Counting
  • Makes use of the fact that plutonium isotopes
    with even mass number (238, 240, 242) have a high
    neutron emission rate from spontaneous fission
  • Spontaneous fission neutrons are emitted at the
    same time (time correlated), unlike other
    neutrons (a,n), which are randomly distributed in
    time
  • Count rate of time correlated neutrons is then a
    complex function of Pu mass

91
Fission Emission Rates for Pu isotopes
Isotope Spontaneous Neutron Emission Rate (neutrons/sec-g)
Pu-238 2.59 x 103
Pu-239 2.18 x 10-2
Pu-240 1.02 x 103
Pu-241 5 x 10-2
Pu-242 1.72 x 103
In reactor fuel, Pu-240 signal dominates over
Pu-238 and Pu-242 due to abundance
92
Neutron Coincidence Counting
  • In neutron coincidence counting, the primary
    quantity determined is the effective amount of
    Pu-240, which represents a weighted sum of the
    three even numbered isotopes
  • Coefficients for contributions from Pu-238 and
    Pu-242 are determined by other means, such as
    knowledge of burnup of reactor fuel. Without
    additional information, calculation will have
    errors but will give a good estimate of Pu mass
    due to relative abundance of the three isotopes.
    Generally, a 2.52, c 1.68

93
Neutron Coincidence Counting
  • In order to determine the total amount of Pu,
    mPu, the isotopic mass fractions (R) must be
    known. These can be easily determined through
    mass-spectroscopy or gamma-ray spectroscopy, and
    is then used to calculate the quantity

94
NCC Technique
  • Utilize He-3 detectors, which can moderate and
    detect spontaneous fission neutrons
  • He-3 detectors usually embedded in neutron
    moderating material to further slow down neutrons
  • Increases detection efficiency
  • Most common measurement is the simple (2-neutron)
    coincidence rate, referred to as doubles
  • If other materials present in the material
    contribute to neutron signal, or impact neutron
    multiplication, other effects may become
    significant, producing errors
  • Generally carried out on relatively pure or well
    characterized materials, such as Pu-oxides, MOX
    fuel pins and assemblies

95
NCC Counters
96
NCC Sources of Uncertainty
  • Counting statistics (random)
  • Can be a significant issue since efficiency can
    be low
  • Calibration parameters and uncertainties
    associated with reference materials (systematic)
  • Correction for multiplication effects, detector
    dead time, other neutron emission (systematic)
  • Nuclear data

97
NCC Parameters to Consider
  1. Spontaneous fission rate
  2. Induced fission
  3. (a,n) reaction rate
  4. Energy spectrum of (a,n) neutrons
  5. Spatial variation of multiplication
  6. Spatial variation of detection efficiency
  7. Energy spectrum effects on efficiency
  8. Neutron capture in the sample
  9. Neutron die-away time in the detector

Clearly, there can be more unknowns than can be
determined in conventional NCC
98
NCC Parameters
  • We want to determine 1,2,3
  • 4 and 5 can be determined with proper use of
    modeling and simulation
  • 6 and 7 can be determined through proper
    calibration
  • 8 and 9 are usually unknown, but in general, are
    of minor consequence
  • Traditional NCC can end up indeterminate only 2
    equations, but three unknowns

99
Neutron Multiplicity Measurements
  • In neutron multiplicity counting (NMC), one
    utilizes triple coincidence rates (in addition to
    single and double counting rates) to provide a
    third measurement such that all parameters can be
    determined
  • Thus, we are solving three equations with three
    unknowns solution is self contained and
    complete
  • One significant advantage of NMC is that there is
    no need for careful calibration with Pu standards
  • Also, can measure samples where there may be
    significant uncertainties in composition

100
Design of NMC
  • Maximize detection efficiency
  • Minimize signal processing time
  • Minimize detector die-away time to decrease
    accidental coincidences
  • Minimize geometry effects to efficiency
  • Minimize spectral effects on efficiency

101
Advantages of NMC
  • Greater accuracy in Pu mass determination
  • Self-multiplication and (a,n) rates are directly
    determined
  • Calibration does not necessarily require
    representative standards
  • Measurement time on the order of a few thousand
    seconds, shorter than the 10,000s typical of NCC
  • Higher efficiency NMC systems can provide even
    shorter measurement times with improved accuracy

102
Disadvantages of NMC
  • Cost
  • More floor space required
  • Some other techniques can provide shorter
    measurement times
  • Some biases can remain if there is a high degree
    of uncertainty in measured samples
  • Running out of He-3

103
Examples
  • In-Plant NMC measurement system

104
Examples
  • 30-gallon drum measurement system

105
Examples
  • High efficiency neutron counter
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