Currie 1968
Currie 1968
Quantitative Determination
Application to Radiochemistry
Lloyd A. Currie
Analytical Chemistry Division, National Bureau of Standards, Washington, D, C. 20234
alternative procedures, and to optimize given procedures with Figure 1. “Ordered” detection limits—literature definitions
respect to certain experimental parameters. Examination of The detection limit for a specific radioactivity measurement process
the analytical and radiochemical literature for an appropriate is plotted in increasing order, according to commonly-used alterna-
definition of the limit of detection revealed a plethora of tive definitions. Lc, Ld, and Lq are the critical level, detection
mathematical expressions and widely-ranging terminology. limit, and determination limit as derived in the text
One encounters, for example, terms such as lower limit of de-
tection (7), detection sensitivity (2), sensitivity (3), minimum that of the net signal. Some authors apply two-sided confi-
detectable activity (or mass) (4, 5), and limit of guarantee for dence intervals, while others use one-sided intervals. In addi-
purity (6)—all used with approximately equivalent meanings. tion, various “nonstatistical” definitions appear in which the
The nomenclature problem is compounded, however, because detection limit is equated to the background, 10% of the back-
other authors make use of the same, or very similar, terms to ground, 100 dps ( -radioactivity), or 1000 dpm (a-, 3-, -radio-
refer not to the minimum amount that may be detected, but activity). In order to compare some of the more commonly-
rather, to the minimum amount which may be determined with used definitions, “detection limits” have been calculated for a
a given relative standard deviation (such as 10%). Still other Hypothetical radioactivity experiment in which a long-lived
expressions, such as the “detection limit at the 95% confidence 7-emitter was counted for 10 min with an efficiency of 10%,
level” are used without explicit mathematical definition, which using a detector having a background of 20 cpm. The results,
leaves the meaning rather ambiguous. The various mathemati- plotted in increasing order in Figure 1, are obviously unsatis-
cal definitions of detection limit (or its equivalent) range from factory, for they encompass nearly three orders of magnitude!
one to twenty times the standard deviation of the net signal, In what follows, it will be seen that a complete discussion of
with the standard deviation of the blank sometimes replacing the (lower) limits for a measurement process requires the in-
troduction of three specific levels: (1) a “decision limit” at
which one may decide whether or not the result of an analysis
indicates detection, (2) a “detection limit" at which a given
(1) B. Altshuler and B. Pasternack, Health Physics, 9, 293 (1963).
(2) J. Wing and M. A. Wahlgren, Anal. Chem., 39, 85 (1967). analytical procedure may be relied upon to lead to detection,
(3) R. C. Koch, “Activation Analysis Handbook,” Academic and (3) a “determination limit” at which a given procedure will
Press, New York, N. Y., 1960. be sufficiently precise to yield a satisfactory quantitative esti-
(4) D. E. Watt and D. Ramsden, “High Sensitivity Counting mate. Following definition of the three levels, an attempt will
Techniques,” Macmillan Co., New York, N. Y., 1964.
be made to indicate their relations to the various definitions re-
(5) “A Manual of Radioactivity Procedures," Handbook 80,
National Bureau of Standards, Washington, D. C., 1961. ferred to previously, and to give asymptotic expressions which
(6) H. Kaiser, Z. Anal. Chem., 209,1 (1965). may serve as convenient working definitions.
related physical quantity by means of the calibration factor. (correct) decision, “detected.” The detection limit, defined in
Symbols will be defined, in general, as they appear in the this manner, is equivalent to the“limit of guarantee for purity”
text, but it may be helpful initially to list the following: of Kaiser (6) and the “minimum detectable true activity" of
Altshuler and Pasternack (7). The significance of this partic-
Blank: µ limiting mean (or “true” mean)
B observed value ular form for the definition is that it allows one to determine,
standard deviation for a given measurement process, the smallest (true) signal
which will be “detected” with a probability 1 —ß, where the a
Gross Signal: ps+B limiting mean posteriori decision mechanism has a built-in protection-level,
(S + B) observed value a, against falsely concluding that a blank observation repre-
+ b standard deviation sents a “real” signal. True signals, ps, lying between zero
and Ld will have larger values for ß, and therefore, although
Net Signal: ps =
ps+b -
Pb limiting mean
value derived from they may be “detected,” such detection cannot be considered
S = (S + B) —
B an
reliable.
observation pair
Mathematically, the critical level is given as
3 =
( 2+ + |)1/2 standard deviation
Lc —
kaao (1)
The blank is defined as the signal resulting from a sample
which is identical, in principle, to the sample of interest, except and the detection limit,
that the substance sought is absent (or small compared to ). Ld =
Lc -j- kpUD (2)
The blank thus includes the effects of interfering species.
where ka and kp are abscissas of the standardized normal
Qualitative Analysis. It is vital at the outset to distinguish
between two fundamental aspects of the problem of detection:
distribution corresponding to probability levels, 1 a and—
1
—
J/ V
UNRELIABLE DETECTION DETECTION: QUALITATIVE ANALYSIS DETERMINATION: QUANTITATIVE ANALYSIS
H i As = 0
VLc
„
Lc =
kctO< k^cro
NET SIGNAL
H =
://$ Lg
L0 =
Lc+ kg^g
Lc ld
0 Lc Lq Lq
Figure 2. Hypothesis testing
Figure 3. The three principal analytical regions
Errors of the first and second kinds
y. (z 1—7/2 is the critical value for the standardized normal to estimate a limit of detection. In any case, replicates are
distribution such that Prob (z < zi-y2) = 1 y/2.) If the net
—
ployed, Lc is numerically equal to ' -yr. This leads to the to that used by Adams, Passmore, and Campbell who defined
common, mistaken practice of equating \-7 with the “de- a “minimum working concentration” as that for which the
tection limit [(95%) confidence level]." Such a statement relative standard deviation was 10 % (S).
is seriously in error because the detection limit cannot be The Determination Limit so defined is,
characterized by a single “confidence level,” and because it
Lq =
IcqCq (3)
confuses the decision-making quantity ( ' -7 Lc) with LD, =
which is used to assess the a priori detectability. To the where Lq is the true value of the net signal, ps, having a stan-
extent that =
0, which may be satisfactory if is approxi- dard deviation, aQ, and 1 ¡kQ is the requisite relative standard
mately constant in the region between zero and LD, the use of deviation.
z'i-yC (one-sided) to test a given result is exactly equivalent to By way of summary, the levels Lc, LD, and Lq are deter-
the use of Lc for this purpose. mined entirely by the error-structure of the measurement
A second possible mistake is the confusion of an a posteriori process, the risks, a and ß, and the maximum acceptable
upper limit with the a priori detection limit. Here again, the relative standard deviation for quantitative analysis. Lc
two may coincide, if the net signal happens to be Lc, and if is used to test an experimental result, whereas LD and LQ
« cd and the one-sided confidence interval is employed. refer to the capabilities of measurement process itself. The
Such a coincidence is not accidental, for the detection limit relations among the three levels and their significance in
is, by definition, the maximum upper limit. It must be re- physical or chemical analysis appear in Figure 3.
membered, however, that, in general, the upper limit depends Special Cases (numerical results). In order to make the
upon the specific experimental result, S, whereas the detection significance of Equations 1-3 clearer, a number of specific
limit must be independent of S, depending, rather, upon the choices for a, ß, and the various ’$ may be helpful.
measurement process itself.
Finally, the difference between and / j/V« should be
(8) P. B. Adams, W. O. Passmore, and D. E. Campbell, paper No.
discussed. The use of the latter, which depends upon the 14, “Symposium on Trace Characterization—Chemical and
variance estimate resulting from «-observations, is clearly Physical,” National Bureau of Standards (Oct. 1966).
cates detection (a =
0). LD = kgaD, and Lq kQaQ, where =
1. a = =
constant. If the risks of making both aD and aQ now depend upon the net signal only.
ß·,
5. a2s+B = ms + mb· Poisson statistics—to be discussed
kinds of mistake are set equal, then ka-= kg k, and
—
Ld = 2k a = 2 Lc (5b) both risks are set at 50%, then both levels coincide with zero.
Therefore, any positive, net signal will be recognized as “real,”
In this case, the detection limit is just twice the critical level— and any nonzero “true” level in a sample will be “detectable.”
a situation which obtains in the large majority of (That is, the detection limit is in fact zero!) However, such
cases. Assuming that risks of 5% are acceptable, and that fantastic detection capabilities must be viewed with caution,
the random errors are normally-distributed, the constant, for regardless of whether ms 0, or if it is just above the =
k, takes on the value, 1.645. The standard deviation of the limit of detection, the conclusion will be wrong 50% of the
net signal is derived from time, and therefore the experiment could be performed equally
well by the flipping of a coin.
2 =
as+s + ß2 (6)
where <tJ+ b represents the variance of the “gross” (directly- RADIOACTIVITY
observed) signal and ß2 represents the variance of the blank.
If the standard deviation is approximately independent of the Signal Detection. Application of the foregoing considera-
tions to radioactivity involves the fact that the gross “signal”
signal level, then
and “blank” observations are in digital form which in most
2 =
a¿+B + ß2 = 2 ß2 (7) cases may be assumed to be governed by the Poisson dis-
tribution. (Extra, non-Poisson variability of the blank is
Making the additional requirement that kq =
10—i.e., that
discussed below, under “Interference and Background.”)
aQ =o 10%—we find that
If the numbers of counts are sufficiently large, the distribu-
Lq =
kqaQ = 10 a (8) tions are approximately Normal, and we may therefore
readily estimate the variance of the net signal and establish
The above results are summarized in Table I, which may be
approximate levels of confidence and significance. Under
used to provide convenient “working” formulae for the large
such circumstances, the variance of the net signal (number of
majority of problems. The first row is derived assuming
counts) is given by
equivalent observations of sample (plus blank) and blank,
while the second row, which differs by assumes that a l/V^ 2 =
as+b + ß —
(ms -p Mb) + —
(9)
long history of observations of the blank make the second «
term on the right in Equation 6 negligible.
2. Fixed Ld; varying ( ,ß). For a given measurement (B is assumed to have been derived from «-observations of
the blank.) Note that a is not independent of signal level
process specification of a fixes Lc. Similarly, specification
as was assumed in Table I. Its variation over the range
of Lc or a together with the specification of ß fixes LD.
For a given LD, however, an infinite set of combinations Ms
=0 to Ms Ld is trivial if mb is large, however. If
=
0, =
and Lc 0 if µ
=
0, is peculiar to the Poisson distribution,
=
aD =
ao), correspond to ( ,ß) (0.5, 0.0005) and ( ,ß) = = “general” case and that of radioactive decay.
Remembering that 02 is the variance when m.s 0, and =
the magnitude of the background, per se, but only its stan- Lc =
ka 0 =
ka (mb + °~i)112 (10)
dard deviation, there is no change. Such a state of affairs is
reasonable, for a background of any magnitude can be set Ld —
Lq -f- kgao =
Lc + kg (Ld ao2) 1,2
(11)
equal to zero simply by a change of scale; such a change can- Solving Equations 10 and 11 for LD, leads to
not be expected to alter the detection limit.
0. In this case, the effect is profound. Lc is ke2 4¿c 4Lc2 1/2)
4. aB =
j
Ld —
Lc -j- 1 + , ,
(12)
necessarily zero, and any net positive signal definitely indi- kg2 ka2kg2
(| =
“Well-known" blank
µ) 2. 33 \/µ 2.71 + 4.65 V7b 50·
K
(7
Zero blank
=
0) 1.64 V7b 2.71 + 3.29 V7b 50
j +l -r}
(MB 0) = 0 2.71 100
Asymptotic ratio6»'
(S/tb) 1.64 3.29 10
*
Dimensions (counts) apply to the first three rows only.
6
“Well-known” blank case; for paired observations, multiply by /2.
'
Correct to within 10% if µ > 0, 67, 2500 counts, respectively, for each of the three columns. For paired observations, µ > 0, 34,
1250 counts, respectively.
the blank thus allow the calculation of Lc and LD for selected proximately 0.07 instead of the desired 0.05.
values of a and ß by means of Equations 10 and 12. A con- Interference and Background. Thus far, µ and have
siderable simplication takes place if ka k's k. Equation = =
been used to refer to the “blank.” In observations of radio-
12 then reduces to the form, activity one frequently approaches the situation where the
blank is due only to background radiation. When such is
Ld = k2 + 2LC (13) not the case, it may be desirable to decompose the blank into
Equation 13 differs by the term, k2, from that arising in the its separate components: background and interfering ac-
previous discussion in which the “reasonable” assumption tivities. Using b to denote background and I to denote in-
was made that 2 » const. Thus, even if 0 Lc,
—
= terference, the above quantities take the form,
we see that Ld may never be equal to zero. The determination
Ms =
µ» + µ/ (16)
limit, Lq, is given by
2 =
»2 + ,2 (17)
Lq =
kQ<TQ
—
Especially simple “working” expressions may be stated when extra (non-Poisson) component of variance. Such extra
the number of background counts, µ , is “large.” Such variance, which may arise from cosmic ray variations or in-
simplified expressions, presented in terms of the ratio of strument instability, must be included in the estimate of
the net signal to the standard deviation of the background 02 and, hence, in the estimates of Lc, LD, and LQ.
(“signal/noise”), appear in the bottom row of Table II. Limits for the Related Physical Quantities. In order to
Note the correspondence of the asymptotic ratios to the make the decision, “detected” or “not detected," one needs
“working” expressions in Table I. to know only the net number of counts resulting from a
The occurrence of nonintegral values for LD and Lq in specific experiment, and the critical number of counts, Lc.
Table II is not at all inconsistent with integral, Poisson dis- Limits for qualitative and quantitative analysis and upper
tributions, because LD and Lq represent the means of such limits or confidence intervals for actual results, however, are
distributions, and such means may take on any positive value, of value only when expressed in terms of the physical quan-
integral or nonintegral. Lc, on the other hand, represents a tity of interest, such as grams or atoms. The connection is
decision level against which an integral, experimental result simply made by means of the relevant calibration factor. For
must be compared. An exact, Poisson treatment would thus example, the detection limit, Ld, may be related to the mini-
lead to an integer for Lc, but only discrete values for a would mum detectable mass, mD(g), by means of Equation 18,
then be possible. The magnitude of the error in significance
Ld =
KmD (18)
level, due to the assumption of normality, is worth consider-
ing with respect to the data in Table II. For example, LD where K represents an overall calibration factor relating the
is there given as 2.71 counts for the zero blank case, and this is detector response to the mass present. Thus, K would be
supposed to correspond to ß 0.05. Examination of the =
equal to unity for direct (ideal) weighing; it would be equal
correct, Poisson distribution shows that the probability of to the absorbance per gram for spectrophotometry if the
where P =
production rate (nuclei/g-sec) Such a procedure suffers from a number of limitations, when
S =
saturation factor 1 e~Xr = —
compared to the use of Equation 22 (or the analogous equa-
T =
(e_w/X) (1 _ ) (seconds) (a generalized
— tions for mc and mQ). The limitations include: (1) no al-
counting interval relating initial counting rate lowance is made for short-lived radioactivity; (2) inter-
to observed number of counts), ference—especially “decaying” interference—is not con-
e =
detection efficiency (counts/disintegration) (chem- sidered; (3) the formula may not be applied to the comparison
ical yield may be incorporated in e, when of critical levels or detection limits, because a- and ß- type
appropriate). errors have not been included; (4) the approximation, µ5
« µ , is built into the formula. This last factor, which
and X are characteristic of the nuclear reaction being would lead one to conclude that one particular detection
utilized; they represent the reaction cross section (cm2) and system is better than another, may lead to the wrong con-
product decay constant (sec-1), respectively, t, t, and At clusion for mD or mQ. That is, the exact equations, of the
are the times (sec) for activation, delay (decay), and counting, form of Equation 22, can lead to the conclusion that the one
respectively, x represents a variable detection parameter, detection system has the lower limit of detection, but that
such as absorber thickness, discriminator setting, etc. A the other has the lower limit of determination.
similar expression may be written for the mean number of
counts from an interfering radionuclide: ILLUSTRATIONS
µ =
m¡ [P(Xi)S(\i,T)T(X.¡J,At)f-i(x)] (20) In order to make clear the application of the preceding
formulae, three examples will be given, one selected arbi-
the mean number of background counts is given by
trarily from among “standard” methods of chemical analysis,
another dealing with the simple detection of radioactivity,
µ»
=
b(x)At (21)
and a third dealing with a more complex problem in activation
where b(x) is the background rate, which also may depend analysis.
upon the detection parameter, x. The preceding expressions (1) Spectrophotometry
may be incorporated into a single equation for the mass- The fundamental relation governing the absorption of light
detection limit: by matter may be written,
k2 + 2k [µ + + µ + (/;µ/)2]1/2 A =
µ + A (23)
mD = -
(22) o
distribution and if they are determined by “equivalent” ob- because A0 has been set equal to zero.
servations, the radical in the numerator of Equation 22 takes (d) K =
µ/, the calibration factor.
the simpler form: (2µ + 2µ/)1/2. If the variances are negli- (e) as = standard deviation of the net signal, A.
gible, the radical becomes (µ + µ )112.
Experimental observations on the spectrophotometric de-
Systematic errors in calibration factors are not a part of the termination of thorium using thorin, yielded: 0.0020, =
present discussion. Such errors can in no way affect the crit- and K = 58.2 //g (9). The sample standard deviation, as,
ical level, Lc, because Lc refers only to the instrumental re-
was observed to be relatively constant and equal to , over
sponse at which the decision is made—“detected" or “not the concentration range studied. A particular sample an-
detected.” All physical quantities deduced from Ld, Lq,
alyzed was observed to give a response (absorbance) of 0.0060.
or an “observed” net signal, however, contain uncertainties
Using these data and expressions for paired observations from
due to calibration factor errors. Because the calibration
Table I, we find the following:
factor error is here considered systematic, while the observa-
Decision: Lc 2.33 =
0.0047, Thus, the observed re-
=
( ,«) 8SK (93.1 %) 38K (7.7 min) 7.7 X 10-i° 6.0 X 10-7
23Na (100%) 22Na (2.6 yr)
0
Isotopic abundance listed in parentheses.
6
Half-life listed in parentheses
nance).
(For long-lived species, T, the “effective counting interval,"
(c) irradiation time and counting time-103 min or two
reduces to At, the physical counting interval.) Using the
half-lives (potassium product) whichever is less.
fact that µ 20 cpm X 15.4 min, one may calculate Lc,
=
(d)delay time-negligible.
Ld, and LQ directly from the formulae for paired observations nuclear cross sections-taken from the literature.
(e)
given in the first row of Table II. The above value for e
8.33 min, in order to de- (f) interference correction accuracy, f¡-\ %.
may then be combined with T =
We describe a rapid and flexible graphical method for necessary to find the nuclear parameters in the literature
estimating the activity induced in neutron irradiations. Concise summaries of sensitivities for thermal-neutron activa-
This method, applicable to several activation problems,
is applied here to thermal- and fission-neutron irradia- tion have also been published (4, J). These generally apply
tions, which are widely used in activation analysis to selected counting and irradiation conditions.
with reactors. The calculated saturation activities of The techniques described here combine, in compact form,
the products of most activation reactions are repre- the essential nuclear data with a quick and flexible graphical
sented on two activation charts. We develop a graphi- calculation method. The various factors appearing in the
cal technique, using a transparent overlay, to obtain
corrections for the saturation, decay, and counting activity equation, including the saturation, decay, and count-
factors. The principal advantage of this method is ing-time corrections, can easily be determined. Also, quali-
that the corrections due to these factors can be applied tative information of optimal irradiation and decay times,
to any saturation activity of the chart, which already which are often desired in activation analysis, can be obtained
contains all the nuclear information required for
estimation of induced radioactivity. Most simple graphically rather than by using numerical computer tech-
activity calculations can be performed quickly and niques (6).
accurately; the technique is also useful in estimating
the best irradiation and decay times to enhance GRAPHICAL METHOD FOR COMPUTATION
selected activities in composite samples. We give the
numerical values for the construction of charts of The Activation Equation. In calculating induced radio-
saturation activities for thermal- and fission-neutron activity, we assume that the irradiated sample is so small
irradiation and for the overlay. Calculation tech- that it produces no significant attenuation of the flux of in-
niques are explained and clarified with typical ex- cident particles. The total disintegration rate of a radio-
amples.
isotope produced by irradiation of an element of natural
The calculation of induced radioactivity is required in many isotopic composition in a constant flux is then given by
activation problems. Generally, the same mathematical
formalism is applied, with different values of nuclear constants
and time parameters. The search for nuclear constants and
A =
"100^[(1
M
-
the solution of equations for composite samples is often time- AsatSD = N* In 2/7V2 (1)
consuming. We here develop a graphical method for rep-
where m is the mass of the irradiated element, / is the isotopic
resenting nuclear data and solving activation equations; this
method can be successfully applied to several activation abundance (%) of the isotope that undergoes the reaction,
No is Avogadro’s number, is neutron flux, a is the cross
problems, flux monitoring, and radioisotope production with
reactors and accelerators. (The two activation charts and section, M is the atomic weight of the irradiated element,
the transparent overlay are available as a courtesy from 7i/2 is the half-life of the induced activity, is the irradiation
General Radioisotope Processing Corp., 3120 Crow Canyon time, ti is the decay time (between the end of irradiation and
Road, San Ramon, Calif. 94583.) The specific applications the beginning of counting), Asat is the saturation
to thermal- and fission-neutron activation have been chosen 100 M
because of their wide and frequent use in activation analysis activity, S is [(1 —