principles of liquid scintillation counting: theories and … · principles of liquid scintillation...
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Paul Scherrer Institut • 5232 Villigen PSI lecture: principles of LSC, RISO, September 6, 2013
PAUL SCHERRER INSTITUT
Principles of liquid scintillation counting: theories and applications
Jost EikenbergDivision for Radiation Safety and Security
Paul Scherrer InstitutCH-5232 Villigen PSI / Switzerland
Paul Scherrer Institut • 5232 Villigen PSI lecture: principles of LSC, RISO, September 6, 2013
PAUL SCHERRER INSTITUT
Development and implementation of radiochemical separation techniques for emission and immission measurements such as actinides in soil samples Ra isotopes in groundwater etc.Research projects with universities: dating
of Pleistocene samples with applications in volcanology, paleoearth quake dating , ice core samples (global warming)
R&D projects of the PSI radioanalytical laboratory
Paul Scherrer Institut • 5232 Villigen PSI lecture: principles of LSC, RISO, September 6, 2013
PAUL SCHERRER INSTITUT
Table of Contents
1. Introduction to the LSC counting technique2. Quenching effects and correction procedures3. Alpha/Beta separation via pulse shape analysis4. Introduction to the triple to double coincidence
ratio measurement technique (TDCR)5. Example of a simultaneous alpha/beta analysis
using Radium isotopes in drinking water
Paul Scherrer Institut • 5232 Villigen PSI lecture: principles of LSC, RISO, September 6, 2013
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Example: decay scheme of -emitting 228Ra
ZA
ZAX Y e decay energy
1
1
Z = 88
Z = 89228Ac (6.13 h)
1-
0.0
0.0
0.0067
228Ra (5.75 y)
Particle radiation, pure -emitting isotopes
Paul Scherrer Institut • 5232 Villigen PSI lecture: principles of LSC, RISO, September 6, 2013
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Schematic view of radioactive transformation
1 (95.5 %)1
Z = 88
Z = 86222Rn (3.82 d)
2 (4.5 %)
0.0
0.0
0.186
226Ra (1600 y)
88226
86222
24 4 78Ra Rn He MeV .
Paul Scherrer Institut • 5232 Villigen PSI lecture: principles of LSC, RISO, September 6, 2013
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principle of liquid scintillation spectrometry (LSC)
• Sample is in a cocktail with a organic scintillator and homogenously mixed
• Particle radiation ( or ) disturbs the electron configuration (orbital) of the scintillation liquid
• During recombination of the electron structure light (h*) is emitted which is measured in photomultiplier tubes
Paul Scherrer Institut • 5232 Villigen PSI lecture: principles of LSC, RISO, September 6, 2013
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page 7
Liquid Scintillation Counting
Samples are dissolved or suspended in a "cocktail" containing an aromatic solvent and small amounts of other additives known as fluors Beta particles emitted from the sample transfer energy to the solvent molecules, which in turn transfer their energy to the fluors; the excited fluor molecules dissipate the energy by emitting light In this way, each beta emission results in a pulse of light
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Principle of LS Coincidence/Anticoincidence Counting
page 8
log Scale
3H 14C 32P
The counter has two photomultiplier tubes connected in a coincidence circuit. The coincidence circuit assures that genuine light pulses, which reach both photomultiplier tubes, are counted, while other pulses (due to noise, for example), which would only affect one of the tubes, are ignored.
Paul Scherrer Institut • 5232 Villigen PSI lecture: principles of LSC, RISO, September 6, 2013
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PMT 1
COINCI‐DENCE
PMT 2
SUM‐MATION ADCAMPLIFIER
DIGITIZEDSUMMED
COINCIDENCEPULSE
SPECTRALYZERSPECTRUMANALYZER
COINCIDENCE PULSE
Classical two photomultiplier LS electronic set-up
Paul Scherrer Institut • 5232 Villigen PSI lecture: principles of LSC, RISO, September 6, 2013
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principle of LSC coincidene/anticoincidence counting
PMT 1 PMT 2PMT 2
PMT 2PMT 2
sample chamber
PMT 2 PMT 2
sample vial
Paul Scherrer Institut • 5232 Villigen PSI lecture: principles of LSC, RISO, September 6, 2013
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LSC, Perkin Elmer Model TriCarb 3100 TR/SL LSC with BGO detector guard
Paul Scherrer Institut • 5232 Villigen PSI lecture: principles of LSC, RISO, September 6, 2013
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HIDEX Model SL 300 with guard detector
Paul Scherrer Institut • 5232 Villigen PSI lecture: principles of LSC, RISO, September 6, 2013
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LSC: relevant isotopes in the nuclear fuel cycle, radiopharmaceutical
application and environmental analysis• Pure - or ec-emitters Tritium (H-3) and
Radiocarbon (C-14) others, : Cl-36, Fe-55, Ni-63, Sr-90, Biological application: P-32, P-33, etc.
• Alpha-emitters, actinides : Th, U, Pu, Am, Cm• Alpha- and Beta-emitters from the U and Th decay
series: Ra-228, Ra-226, Pb-210, Po-210
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-continuum-spectra: 3H, 14C
1 10 1000
200
400
600
800
1000
1200
LSC: spectrum of 14C und 3H
E max
=18
.6 k
eV
E max
= 1
56 k
eV
3H 14C
inte
nsity
(not
to s
cale
)
energy (keV)
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Calculation of activity concentrations via classical and TDCR measurements
• Direct counting (standardization) and two window counting (e.g. 3H, 14C)
• Use of quench curves• Efficiency tracing methods (CIEMAT/NIST, needs
modeling) • Triple to double coincidence ratio measurements
(TDCR)
Paul Scherrer Institut • 5232 Villigen PSI lecture: principles of LSC, RISO, September 6, 2013
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general relationship between activity and counting rate
N
tIA
)14(.)()3( 14, CcpmcmpcpmcpmHcpm BC
B
AnetAA
Example H-3, C-14, two window countingwindow A: H-3 + C-14, window B: C-14
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Determination of the counting efficiency(a) by adding spike of the same isotope
AN
(b) Automatically via quench curve correctionaddedi
additionbeforeiadditionafterii A
NN
,
,,
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Three window Sr-isotope counting
1 10 100 10000
20
40
60
80
100
120
composite spectrum
90Y
90Sr
85Sr
Region A:85Sr
Region C:89Sr + 90Y
Region B:90Sr + 90Y + 89Sr
-energy [keV] (LS-scale)
coun
ts/c
hann
el (n
ot to
sca
le)
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• Quenching within a sample refers to any mechanism which reduces the amount of light being emitted from the vial. • Reducing the amount of light reaching the PMT’s results in a reduction of the pulse height.• Any factor, which reduces the efficiency of the energy transfer or causes the absorption of photons (light), results in quenching in the sample.
Quenching
page 19
Paul Scherrer Institut • 5232 Villigen PSI lecture: principles of LSC, RISO, September 6, 2013
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Sabine Mayer – 1 Introducion to radiological physics page 20
Chemical Quenching… occurs during the transfer of energy from the solvent to the scintillator.
Chemical agents (e.g. water and other solvents) added to the cocktail with the radioactive sample interfere with the transfer of kinetic energy between the solvent and the fluor(s).
The results are:Reduction and loss of lightReduced counting efficiency
Colour Quenching…is an attenuation of the photon of light.
The photons produced are absorbed or scattered by the colour in the solution, resulting in reduced light output available for measurement by the PMT’s.
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14C spectrum of waste water: examples for not quenched filtrated
water and a quenched spectrum (direct measurement)
1 10 1000
200
400
600
800
1000
1200
E quen
ched
< E
max
E max
= 1
56 k
eV
14Cquenched
14C(not quenched)
rela
tive
inte
nsity
energy (keV)
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Effects of Quenching
page 22
1) A shift in the pulse height spectrum of the particles to lower energy
2) A reduction in the measured CPM of the sample (loss of counting efficiency). This effect occurs especially with low energy particles.
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Quench parameter calculation
k
ii
k
iii
XI
XIXkQPES
1
1
)(
)(
QPES or tSIE = quenching parameter (or center ofgravity or spectral index) of the external standardXi and I(Xi) refer to the channel numbers and the countrates of the external standard in each channel number.
Paul Scherrer Institut • 5232 Villigen PSI lecture: principles of LSC, RISO, September 6, 2013
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3H, 14C quench curves: efficiency in dependency of the spectral index from the external standard
100 150 200 250 3000
20
40
60
14C 3H
% e
ffici
ency
tSIE
Paul Scherrer Institut • 5232 Villigen PSI lecture: principles of LSC, RISO, September 6, 2013
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Alpha/Beta Separation
• Classical: use of spill-over curves and pulse shape analysis (PSA)
• TDCR (Hidex 300 SL): use of pulse length index (PLI) and energy differentiation
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Alpha/Beta spectrum of Pu-isotopes
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(iii) Alpha LSC countingalpha/beta-discrimination, PSA, Pulse
Shape Analysis)
20 40 60 80 100 120 140 1600
200
400
600
800
1000
1200
alpha-pulse
beta-pulserela
tive
inte
nsity
pulse decay time [ns] 100 110 120 130 140 1500
2
4
6
8
10
12
14
in in
spillo
ver [
%]
discriminator setting [ns]
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Pulse Length Index (PLI) discrimination with HIDEX SL 300
27 38 52 72 99 135
185
252
343
466
634
861
1169
1588
2156
2927
3973
5393
7319
9934
1348
1
1829
6
0
4
8
12
16
20
24
28
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Analytical separation of two interfering -peaks
0 200 400 600 800 10000
20
40
60
80
100
120
140
window B:B + Aspill
window A:A + Bspill
AspillBspill
BA
window Bwindow A239+240Pu 236Pu-Tracer
-energy [MeV]
coun
ts/c
hann
el (n
ot to
sca
le)
Paul Scherrer Institut • 5232 Villigen PSI lecture: principles of LSC, RISO, September 6, 2013
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mathematical equations: 2-window counting
AA
V spill1 BB
V spill2
spillA BAN spillB ABN
21
21239 1
1VV
NVNVAAN BAspill
21
12236 1
1VV
NVNVBBN ABspill
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Isotope Spiking
Pu
ss Y
NA )(239
)(239
Pu
tt Y
NA )(236
)(236
)(236)(236
)(239)(239 t
t
ss A
NN
A
Paul Scherrer Institut • 5232 Villigen PSI lecture: principles of LSC, RISO, September 6, 2013
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The triple coincidence to double coincidence ratio (TDCR) counting technique
SAMPLE
PM R
PM S
PM T
Paul Scherrer Institut • 5232 Villigen PSI lecture: principles of LSC, RISO, September 6, 2013
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The theory of TDCR
nx
exnnxP
!),(
1!
:0xnx
x
nenPZ ),0(
neZ 11
In counting statistics the number of events (x) that are detected from a mean number of (n) events follows a discrete probability or Poissondistribution provided that the events occur with a known average rate and independently of the time since the last event i.e.
From equation (9-53) it follows for the extreme case of no detection
Therefore, for case of no detection or zero detection (Z) it follows for 1 photomultiplier, for instance for “R”:
And, for the detection probability or detection efficiency ():
(9-56)
(9-53)
(9-54)
(9-55)
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2111 nnn eee
32 111 nnn eee
31 neRST
nn eeRS 21
Equation (9-56) shows that the value for the detection efficiency varies between 0 (no interaction between the decaying isotopeand the scintillation cocktail) and 1 (i.e. when high energetic beta particles undergo strong interaction with the cocktail medium, i.e. produce a very high number of photons that are detected via LSC). From equation (9-56) it is obvious that for 2 photomultipliers (R+S) connected in coincidence, the total coincidence efficiency is:
And, consequently, for three photomultipliers (R, S, T) connected in a coincidence circuit:
In the following the possible quantity of coincidences is listed for the one case of triple coincidences tubes (R-S-T)and the other three cases of double coincidences, i.e. (R-S, R-T, S-T).
3-coincidences:
Equation (9-60) shows the coincidence probability for the R-S couple with zero detection from the T-tube.In analogy it can be written for the combination of the R-T-tubes (with zero detection from the S-tube):
(9-62)
2-coincidences:
(9-57)
(9-58)
(9-59)
(9-60)
nn eeRT 212-coincidences:
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nn eeST 21
nnn eeeall 23 131
nnn eeeall 311 2
nn eeall 211 2
And, finally for the combination S-T (with zero detection from the R-tube):2-coincidences:
(9-62)The logical sum of these 4 possible combinations, i.e. the sum of all coincidences is:
(9-63)This expression can be rewritten by reducing both terms in equation (9-63) with (1-e-n)2 i.e.,
(9-64)
(9-65)
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32 1213 nn eeall
32
3
12131
nn
n
eee
alltriple
cidencesdoublecoincidencestriplecoinTDCR
1..11: TDCReien n
0...11:0 23 TDCReieen nn
Multiplying these terms and converting the result in binominal expressions yields finally:
Therefore the ratio of triple coincidences to all coincidences, referred in the literature as TDCR, is in reality:
In the following, two extreme cases have to be regarded, i.e. the number of photoelectrons produced in the multiplier (n) tends to a) an unlimited high number and, b) tends to zero value, i.e.
(9-68)
(9-69)
(9-66)
(9-67)
For a high number of events the measured ratio TDCR is a function of the counting probability detection, i.e. the efficiency.With common pure -emitting radionuclides and less quenched cocktail medium (e.g. 14C in organic compounds such as benzenemixed with a high aromatic scintillation liquid) the TDCR value approximates roughly the counting efficiency.For the Hidex 300 SL LS-spectrometer the efficiency is given as linear function of the TDCR-value or,
1 mwithTDCRm (9-73)
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0.0000
0.1000
0.2000
0.3000
0.4000
0.5000
0.6000
0.7000
0.0000 0.1000 0.2000 0.3000 0.4000 0.5000 0.6000 0.7000
TDCR
Eff
The first approximation linear relationship between the counting efficiency and the TDCR
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TDCR vs. Efficiency using high purity radionuclide standard solutions
0.4 0.5 0.6 0.7 0.8 0.9 1.00.4
0.5
0.6
0.7
0.8
0.9
1.0
TDCR = efficiency
226Ra
210Pb
228Ra
TDC
R
efficiency
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TDCR blank correction
2211 MCMCMC mm
00 TDCRrTDCRrTDCRr nnbb
For linear systems the following mass relationship hold for mixtures (m) of two omopnents, M1 and M2 with the concentrations C1 and C2
This relationship can be transferred directly to TDCR measurements and the true or net-TDCR (TDCRn) has to be calculated from the brut-TDCR („mixture“) (TDCRb) and the TDCR-value of a blank measurement (TDCR0) .
with
0rrr bn 000 TDCRrTDCRrrTDCRr nbbb
0
00
rrTDCRrTDCRrTDCR
b
bbn
nnTDCR
n
b
n
n rrrA
0
bbb
b
TDCRrTDCRrrrA
0
20
follows:
for pure beta emittes holds:
with:
follows for the activity calculation
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Terrestrial radioisotopes:
238U-series 235U-series
232Th-series
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238U 234U
230Th
234Pa
234Th
226Ra
222Rn
218Po 214Po 210Po
210Bi
210Pb 206Pb
235U
231Pa
231Th 227Th
227Ac
223Ra
219Rn
232Th 228Th
228Ac
224Ra228Ra
220Rn
215Po
211Pb 207Pb
211Bi 212Bi
216Po 212Po
212Pb 208Pb
207Tl 208Tl
214Bi
214Pb
4.47x109y 2.45x105y
24.1d 7.54x104y
1.17min
4.196MeV
4.776MeV
4.688MeV
4.784MeV
5.490MeV
6.003MeV
1600y
3.825d
3.11min
19.9min
26.8min 22.3y
7.04x108y
6.038MeV
4.395MeV
5.013MeV
3.28x104y
18.7d
21.8y
11.4d
4.010MeV
1.41x1010y 1.91y
5.75y
5.423MeV6.13h
3.66d
5.686MeV
55.6s
6.288MeV
1.6x10-4s
5.01d
7.687MeV
5.304MeV
stable
138.4d
1.06d
5.716MeV
6.819MeV
3.96s
1.8x10-3s
2.14min
36.1min stable
7.386MeV
6.623MeV
4.77min
66.3%
0.15s
6.779MeV 1.01h
33.7%
6.051MeV10.6h
3.05min
stable
8.784MeV
3x10-7s
238U-Series 235U-Series 232Th-Series
UPaThAcRaFrRnAtPoBiPbTl
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Th-Ra relationship in the 232Th and 238U decay series
230 7 54 10 226 1 60 10 222 3 82 2184 3
Th Ra Rn Po daughtersa a d : . : . : .
232 1 40 10 228 5 76 10 228 613 22810 0
Th Ra Ac Th daugthersa a h : . : . : .
228 19110 224 3 66 220 55 6 2160
Th Ra Rn Po daugthersa d s : . : . : .
Paul Scherrer Institut • 5232 Villigen PSI lecture: principles of LSC, RISO, September 6, 2013
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Continental water: relevant isotopes
• Alpha-emitter: U-238, U-234• Beta-emitter: Ra-228 (with fast ingrowing Ac-228)• Alpha-emitter: Ra-226 (with Rn-222 prognies)• Beta-emitter: Pb-210 (with ingrowing Bi-210)• Alpha-emitter: Po-210
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relevant isotopes in continental water and their measurement methods at PSI
radionuclide analytical technique
234U, (235U), 238U U/TEVA separation, electro-deposition, -spectrometry
226Ra, 228Ra, 210Pb filtration (RadDisc), OptiPhase Hisafe3 cocktail, LSC
210Po spontaneous deposition on silver disc, -spectrometry
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Relationship parent / daughterparent isotope
half-life parent
ingrowing daughter
half-life daughter
210Pb () 22.3 years 210Bi () 6.02 days
226Ra () 1602 years 222Rn () 3.82 days
228Ra () 5.76 years 228Ac () 6.13 hours
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Method implementation: low level determination of 210Pb, 226Ra+228Ra in drinking water
• Filtration of the sample (2 liter) through 3 Empore RadDisc (Mn-oxide impregnated) membrane filters
• Elution of Pb with Diammonium Hydrogen Citrate• Elution of Ra with alkaline Na-EDTA solution• Measuring via LSC with optimized -
discrimination
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-spectrum of Radium-226: PERALS-LSC
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-spectrum of 226Ra with ingrowing daughters 2 h and 8 h after separation using HIDEX 300 SL LSC
Alpha
0
20
40
60
80
100
120
140
10 100 1000 10000
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-spectrum of 226Ra with ingrowing daughters obtained 6 days after separation
Alpha
0
20
40
60
80
100
120
140
160
10 100 1000 10000
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-spectrum of 228Ra with ingrowing 228Ac 1 h and 8 h after separation using HIDEX 300 SL LSC
Beta
0
5
10
15
20
25
30
35
40
45
50
1 10 100 1000
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long lived mother – short lived daughter relationship
A t A e e A ey xy
y x
xt yty
yt( ) ( ) ( ) ( )
0 0
A t A e ey xy
y x
xt yt( ) ( ) ( )
0
x yy
y x
1
)1()0()( txy
yeAtA
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LS-spectrum interference correction
228228
AcB
A
AcR
)()( 228228,
228, AcrRrRar B
nAcAmn
Acorn
ARa
cornRa
RarA
228
228,
228
)(
BAc
Bn
AcAcrA228
228
228)(
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Comparison of measured 228Ra and 228Ac activities with calculated decay/ingrowth curves
0 10 20 30 40 50 60 70 800.0
0.5
1.0
1.5
2.0
2.5
228Ac: measured data
228Ra decay curve
228Ra: measured data
228Ac ingrowth curve
rela
tive
activ
ity
time after separation [h]
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Comparison of measured 226Ra and the progeny isotopes 222Rn, 218Po and 214Po with calculated decay/ingrowth curves
0 5 10 15 20 25 300.0
0.5
1.0
1.5
2.0
2.5
3.0
3.5
4.0
222Rn+218Po+214Po: measured data
226Ra decay curve
226Ra: measured data
222Rn+218Po+214Po ingrowth curve
rela
tive
activ
ity
time after separation [d]
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ms tr
VkA 0
1* 21
0 5 10 15 20 250
10
20
30
40
50
226Ra
228Ra
210Pb
low
er li
mit
of d
etec
tion
[mB
q / L
]
counting time [h]
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LSC detection limits, 2 l aliquot, quantitative adsorption on RadDisc filter,
counting time 6 h
• Ra-226: 3 mBq/liter• Ra-228: 20 mBq/liter• Pb-210: 15 mBq/liter
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Conclusions• LSC is a powerful method to detect particle radiation
(alpha / beta) without the need of applying extensive sample preparation procedures
• LSC is highly useful to measure potentially volatile isotopes such as 3H and 14C
• New counter developments allow almost quantitative activity concentration determinations without (internal) standardization, i.e. application of TDCR-measurements using triple to double coincidence ratio measurements
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Thank you for your attention