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Monte Carlo solutions for several problems in low level underground gamma-ray spectrometry O. Sima and D. Arnold Bucharest University and PTB Braunschweig Bucharest Workshop 25 – 27 April 2007
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Monte Carlo solutions for several problems in low level

underground gamma-ray spectrometryO. Sima and D. Arnold

Bucharest University and PTB Braunschweig

Bucharest Workshop 25 – 27 April 2007

Overview

1. Introduction - Low level gamma-ray spectrometry

2. Specific problems solved by Monte Carlo simulation

3. Validation

4. Conclusions

Bucharest Workshop 25 – 27 April 2007

1. Introduction

• Broad range of samples (type, volume, matrix) • High efficiency detectors, high efficiency measurement

geometries • Severe requirements on quality control and quality assurance,

on detection limit • Automatic analysis of spectra

Gamma-ray spectrometry today:

Bucharest Workshop 25 – 27 April 2007

Low level and ultra-low level gamma-ray spectrometry:

• purpose: the best detection limit

- very low background

- high efficiency detectors and measurement geometries

• Volume samples with various matrices: => self-attenuation effects=> sample specific efficiency

• High efficiency detectors and measurement geometries: => coincidence-summing effects=> nuclide specific efficiency

Experimental calibration possible in relatively few cases;expensive, problems with sources

Monte Carlo simulation able to cover all cases of interest in gamma ray spectrometryAfter validation, very useful to complement experimental

calibration

Difficulties in efficiency calibration:

Bucharest Workshop 25 – 27 April 2007

2. Specific problems solved by Monte Carlo simulation

Evaluation of efficiency correction factors:

- self-attenuation corrections

- coincidence-summing corrections

- geometry corrections

Direct evaluation of efficiency

Background under the peaks

Spectrum simulation

= > GESPECORBucharest Workshop 25 – 27 April 2007

GESPECOR• GERMANIUM SPECTROSCOPY CORRECTION

FACTORS, authors O. Sima, D. Arnold, C. DovleteRealistic Monte Carlo simulation program

- detailed description of the physics processes (photon interactions: XCOM; electron interactions; bremsstrahlung)

- detailed description of the measurement arrangement- nuclear decay data: NUCLEIDE, ENDSF (250

nuclides in GESPECOR data base)- efficient algorithms – variance reduction techniques- user friendly interfaces- thoroughly tested at PTB (D. Arnold)

Bucharest Workshop 25 – 27 April 2007

Bucharest Workshop 25 – 27 April 2007

Bucharest Workshop 25 – 27 April 2007

Bucharest Workshop 25 – 27 April 2007

Coincidence summing:

- Summing out = Losses from peaks due to simultaneous detection of other photons (γ, X-ray) => apparent efficiency lower than corrected efficiency

- Summing in = additional counts in the peak no. 3 due to simultaneous complete energy absorption of photons 1 and 2 => apparent efficiency higher than corrected efficiency

Magnitude of coincidence-summing effects• Enhanced in high efficiency measurement conditions => important

in low level gamma-ray spectrometry• Depend on the detailed decay scheme of the nuclide (peak energy,

probability of emission of other photons in cascade, energy of the cascading photons)=> nuclide dependent efficiency

• Depend on the geometry (including surrounding materials), matrix⇒Difficult to evaluate: nuclear data + radiation transport

GESPECOR: automatic evaluation of decay data, variance reduction techniques implemented

Bucharest Workshop 25 – 27 April 2007

GESPECOR versus GEANT

-14

-12

-10

-8

-6

-4

-2

0

2

10 100 1000 10000

Energy (keV)

% D

iffer

ence G 1

G 2

G 3

Peak Efficiency

Bucharest Workshop 25 – 27 April 2007Bucharest Workshop 25 – 27 April 2007Bucharest Workshop 25 – 27 April 2007

Differences in photon cross sections in Ge

XCOM versus GEANT 3.21

-2

-1

0

1

2

3

4

5

0.00E+00 5.00E-01 1.00E+00 1.50E+00 2.00E+00 2.50E+00 3.00E+00 3.50E+00

Energy (MeV)

% D

iffer

ence Ge Photoeffect

Ge Compton

Ge Rayleigh

Ge Pair Production

Bucharest Workshop 25 – 27 April 2007

Bucharest Workshop 25 – 27 April 2007

GESPECOR: coincidence-summingSum peaks with X-rays (n-type HPGe)

Ba-133 spectrum - low energy part

1.0E+02

1.0E+03

1.0E+04

1.0E+05

1.0E+06

1.0E+07

0 50 100 150 200 250

Energy (keV)

Cou

nts

1

2

3

4

5

6

7

89

1011

12

13

14

20

1516

1718

19

21 22

24

23 25 26

• Ba-133 point source

• Corrections in good agreement with experimental data (PTB)

Bucharest Workshop 25 – 27 April 2007

GESPECOR: coincidence-summingSum peaks with X-rays (n-type HPGe)

• Ba-133 point source

• Corrections in good agreement with experimental data (PTB)

Ba-133 spectrum - high energy part

1.0E+00

1.0E+01

1.0E+02

1.0E+03

1.0E+04

1.0E+05

1.0E+06

250 300 350 400 450 500Energy (keV)

Coun

ts

27

29

2830 31

32

3

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3

3

3940

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4243

44

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47 48

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5758 59

60

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62

Bucharest Workshop 25 – 27 April 2007

Are the small coincidence summing peaks present in the spectrum relevant?

Yes, especially in low background measurements:• Corrections factors for the main peaks required for activity

determination, but:• All features of the spectra should be correctly described

(including small peaks and pure sum peaks)- peak interference- nuclide identification problems=> more important in low background measurements!

• Present day tendency: completely automatic analysis of spectra => requires improvement [Arnold, Blaauw, Fazinic, Kolotov, Nucl. Instrum. Meth. A 536 (2005) 196 ]

Bucharest Workshop 25 – 27 April 2007

Efficiency transfer for volume sources with slightly different geometry

• actual geometry slightly different from the reference geometry– identical containers but different filling height

• Transfer factor: – Monte Carlo simulation based on a correlated sampling technique– simultaneous computation of each efficiency

Actual geometry Reference SimulationBucharest Workshop 25 – 27 April 2007

- at low energy, weak dependence of scattered photon energy on angle

e.g. 45 keV: all cases with scattering angle <30° have E>44.5 keV

⇒ Should it be included in the peak efficiency definition? (in programs like GEANT the efficiency is usually defined by the number of counts in a given region of the peak)

⇒ it might be also influenced by the environment of the

measurement, not only by the source, detector and media

in betweenBucharest Workshop 25 – 27 April 2007

Background under the peaks: Small angle scattering in the source and other media

Scatteringmedium

3. Validation

Monte Carlo techniques are well established, but

- are the detector data perfectly known ?

- are the interaction data absolutely correct ?

- is the calculation model perfect ?

⇒Validation required

⇒ Comparison of selected experimental results with calculation,

adjustment of some parameters in case of discrepancy

Bucharest Workshop 25 – 27 April 2007

Comparison between GESPECOR and GEANT 3.21

ICRM Gamma-ray spectrometry Working Group action:

Comparison of Monte Carlo simulation evaluation of the efficiency for 3 geometries:

1. Point source and a bare crystal;

2. Point source and a realistic Ge detector

3. Volume source and a realistic Ge detector

Bucharest Workshop 25 – 27 April 2007

Results

Comparison between our results obtained with GESPECOR and with GEANT:

- in geometry 1 reasonable agreement- in geometry 2 and 3 higher discrepancies, especially at low energies

Agreement of the results for geometry 1 implies that cross sections are in accord?

- no, in geometry 1 at low energy the detector is practically an „infinitely thick“ detector, irrespective to the exact values of the cross sections.- in fact, important differences between XCOM and GEANT cross sections, especially in photoelectric cross section (XCOM – from NIST, Berger and Hubbell)

Bucharest Workshop 25 – 27 April 2007

Differences in photon cross sections in Ge

XCOM versus GEANT 3.21

-2

-1

0

1

2

3

4

5

0.00E+00 5.00E-01 1.00E+00 1.50E+00 2.00E+00 2.50E+00 3.00E+00 3.50E+00

Energy (MeV)

% D

iffer

ence Ge Photoeffect

Ge Compton

Ge Rayleigh

Ge Pair Production

Bucharest Workshop 25 – 27 April 2007

Differences in photon cross sections in Al and H2O

XCOM versus GEANT

0

1

2

3

4

5

6

7

8

9

10

0.00E+00 5.00E-01 1.00E+00 1.50E+00 2.00E+00 2.50E+00 3.00E+00 3.50E+00

Energy (MeV)

% D

iffer

ence

Al Photoeffect

H2O Photoeffect

Bucharest Workshop 25 – 27 April 2007

Effect of the differences in cross sections in the case of geometry 1:- at 45 keV, peak efficiency is changed by 0.08% and totalefficiency is changed by 0.07% if artificial Ge density equal to 6 g/cm^3 (instead of 5.323) is used in GEANT calculations

Effect of differences in cross sections in the case of other geometries:- at 45 keV, if in GEANT the dead layer density is changedfrom 5.323 g/cm^3 to 5.565 and the Al density is changed from 2.7 g/cm^3 to 2.828, the XCOM and GEANT 3.21 cross sections become equal

=> change in peak efficiency –12.6% (G2)=> change in total efficiency –12.2% (G2)

- at 45 keV if in GESPECOR the cross sections are modifed artificially to be equal to the GEANT cross sections, the differences between GESPECOR and GEANT decreaseto 0.5% (G2) and 1.2% (G3) (Ge X-Ray escape excluded)

Bucharest Workshop 25 – 27 April 2007

⇒At low energy photon attenuation in the media between the emission point and the sensitive volume of the detector aremost important

=> dependence on the photon cross sections (especially for photoeffect)

⇒Which cross sections are the best?==========================

Effect of the low energy cut-off:- in GESPECOR 1.9 keV for photons, 10 keV for

electrons- in GEANT 3.21 10 keV for photons, 10 keV for

electronsComputations with GEANT also with 15 and 20 keV low energy

cut-off=> small change in peak efficiency, practically no changein total efficiency Bucharest Workshop 25 – 27 April 2007

Is the 10 keV energy cut-off of no importance?Ge K X-Rays: Kα2 9.85543 (51.49%),

Kα1 9.88653 (100%), Kβ3 10.9781 Kβ1 10.9822

Kβ5” 11.0748 (22.37), Kβ2 11.101 (0.49%)

=> 6.63 times higher probability of X Rays with E < 10 keVthan with E > 10 keV

If in GESPECOR the simulation of Ge X-Rays is prohibitted, the discrepancy in geometry 1 at low energies between GESPECOR and GEANT is much reduced

Bucharest Workshop 25 – 27 April 2007

4. ConclusionsMonte Carlo methods are very useful for assisting in gamma ray spectrometry calibration problemsBest results in the case of the evaluation of efficiency correction factors => robust results, not sensitive to detector data and other imperfections of the model and data

- self-attenuation corrections- coincidence summing corrections- small geometry differences

Direct evaluation of the efficiency => less robust- good detector data are required;- good cross sections ( most important: photoelectric cross sections)- proper values of the simulation parameters (energy cut)

-Validation requiredBucharest Workshop 25 – 27 April 2007

M. C. Simulations of detector efficiencies

GESPECOR and GEANT 3.21-2 sets of results:

- first set: peak efficiency defined as in experimental work(1/10 from the peak height: 96.82 % from Gaussian)

- second set: ideal peak efficiency (the complete Gaussian)

GESPECOR-User friendly MC software for solving problems in gamma ray spectrometry with Ge detectors:

- self-attenuation- coincidence summing- peak and total efficiency

Bucharest Workshop 25 – 27 April 2007

- in measurement: based on a region of interest from the peak,e.g. between 1/10 from the peak height (for a Guassian shape, 96.82% from the ideal peak)

- in simulations peak width is not normally reproduced – it depends on charge production and collection etc. Possible to apply a Gaussian spread of the energy deposited in the sensitivevolume of the detector, assuming that the peak has a Gaussianshape or simply to take 0.9682 from the ideal efficiency.

- possible practical definitions in simulations based on:- interactions in the sensitive volume without any energy lost

outside the sensitive volume- the number of counts in a suitably defined energy bin

- important to have a consistent use of the definition of the peak,especially when coincidence summing effects are present

Peak efficiency definition

Bucharest Workshop 25 – 27 April 2007

Monte Carlo simulation is very useful to complement experimental calibrations- experimental calibration possible in relatively few cases;

expensive, problems with sources - Monte Carlo simulation capable to cover all cases of interest

in gamma ray spectrometry- Problems: requires good knowledge of the experimental setup,

especially detector data, good cross sections and appropriatecorrespondence between the simulated quantities and the quantities applied in experimental data

- Flexibility, user friendliness and short computing times

ICRM Gamma WG Meeting Paris Nov. 2006

GESPECOR physicsPhoton cross sections:

- for each material 100 points between 1.9 keV and 4 MeV; in addition, values before and after each X-Ray absorption edge, on the basis of XCOM- log-log interpolation- very good accord with XCOM (also in the close vicinity of absorption edges)

Electron processes:- multiple scattering (Moliere, third function included), orfaster semiempirical method- bremsstrahlung: fast algorithm, sampling using Walker algorithm- energy loss fluctuations neglected- delta electron production neglected- energy cut: 10 keV Bucharest Workshop 25 – 27 April 2007

GESPECOR – variance reduction- Peak and total efficiency evaluated separately:

-peak efficiency: photon history stopped when energy lost outsidethe sensitive volume of the detector-materials between the point of emission and the sensitivevolume of the detector : attenuating media-emission from source: focalized towards the detector

-total efficiency: photon history stopped at the first interaction inthe sensitive volume of the detector

- Always force the first interaction in the detector- Whenever possible use mean values instead of random sampling

(e.g. use probability of the emission of groups of photons instead of random simulation of decay cascades in coincidence summing computations)

- Use efficient sampling (Walker, interpolation)Bucharest Workshop 25 – 27 April 2007

Computing times: ACER Notebook, Pentium M Centrino 1.4 GHz

GESPECOR GEANTGeometry 1 Peak efficiency: 3 min 1100 minTotal efficiency: 3 min Geometry 2 Peak efficiency: 4 min 2150 min Total efficiency: 15 min Geometry 3 Peak efficiency: 8 min 17000 minTotal efficiency: 60 min

Bucharest Workshop 25 – 27 April 2007


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