In discussions of neutron activation one usually assumes that the daughter radionuclide is not affected by the activation particles. However, there are situations in which this assumption does not hold and account must then be taken of the activation of the daughter radionuclide into a granddaughter nuclide. The model that deals with this type of activation is called the “parent depletion–daughter activation” model and this model too, similarly to the saturation and depletion models, can be written in compact format by introducing new parameters (see Sect. T12.6.5), in addition to the ones (x,m,y_P,y_D) used already in saturation and depletion models.
The standard parameters y_P\ and\ y_D of the saturation and depletion models are defined in Prob. 252 and the new parameters \lambda_{\mathrm{D}}^*, \varepsilon^*, m^*, \text { and } y_{\mathrm{D}}^*, used in conjunction with “depletion–activation” model are defined as follows:,
where σ_P\ and\ σ_D are activation cross sections of parent P and daughter D nuclides, respectively, λ_D is the decay constant of the daughter, \lambda^* is the modified decay constant, \dot{φ} is the neutron fluence rate in the nuclear reactor, m is the activation factor, m^∗ is the modified activation factor, \mathcal{A}_{\mathrm{D}}^*(t) is the daughter radionuclide D activity, and N_P(0) is the initial number of parent nuclei.
For the “parent depletion–daughter activation model”:
(a) Transform the equation that describes the number of parent nuclei N_P(t) into a general format given by y_P as a function of normalized time variable x.
(b) Transform the equation that describes the activity of daughter nuclei \mathcal{A}_D(t) of (d) in Prob. 251 into a general format given by y^∗_D(x) as a function of normalized time x and modified activation factor m^∗.
(c) Compare y^∗ _D(x) calculated in (b) with y_D(x) given for the depletion model in (b) of Prob. 252 and derive expressions for \left(x_{\mathrm{D}}^*\right)_{\max } and \left(y_{\mathrm{D}}^*\right)_{\max } as a function of m^∗.
For the saturation and depletion models of neutron activation the general variables x, y_P,\ y_D as well as the activation factor m are defined as follows
x=m \frac{t}{\left(t_{1 / 2}\right)_{\mathrm{D}}} ; (12.92)
y_{\mathrm{P}}=\frac{N_{\mathrm{P}}(t)}{N_{\mathrm{P}}(0)} (12.93)
y_{\mathrm{D}}=\frac{N_{\mathrm{D}}(t)}{m N_{\mathrm{P}}(0)}=\frac{\mathcal{A}_{\mathrm{D}}(t)}{\sigma_{\mathrm{P}} \dot{\varphi} N_{\mathrm{P}}(0)} ; (12.94)
m=\frac{\sigma_{\mathrm{P}} \dot{\varphi}}{\lambda_{\mathrm{D}}} . (12.95)
In the “parent depletion–daughter activation model” we use the following additional parameters:\lambda_{\mathrm{D}}^*, \varepsilon^* \text {, and } m^* \text { as well as variable } y_{\mathrm{D}}^*(x). The additional parameters are defined as follows
\lambda_{\mathrm{D}}^*=\lambda_{\mathrm{D}}+\sigma_{\mathrm{D}} \dot{\varphi} ; (12.96)
\varepsilon^*=\frac{\lambda_{\mathrm{D}}^*}{\lambda_{\mathrm{D}}}=1+\frac{\sigma_{\mathrm{D}} \dot{\varphi}}{\lambda_{\mathrm{D}}} ; (12.97)
m^*=\frac{\sigma_{\mathrm{P}} \dot{\varphi}}{\lambda_{\mathrm{D}}^*}=\frac{m}{\varepsilon^*} ; (12.98)
y_{\mathrm{D}}^*=\frac{\mathcal{A}_{\mathrm{D}}^*(t)}{\sigma_{\mathrm{P}} \dot{\varphi} N_{\mathrm{P}}(0)} . (12.99)
(a) The standard form for the number of parent nuclei N_P(t), undergoing nuclear activation in particle fluence rate \dot{φ}, is expressed by the following equation
N_{\mathrm{P}}(t)=N_{\mathrm{P}}(0) e^{-\sigma _{ \mathrm{P} }\dot{\varphi} t}, (12.100)
that, after incorporating (12.92), (12.93), and (12.95), takes up the following form giving the number of parent nuclei N_P(t) normalized to the initial number of parent nuclei N_P(0) as
y_{\mathrm{P}}=\frac{N_{\mathrm{P}}(t)}{N_{\mathrm{P}}(0)}=e^{-\sigma_{\mathrm{P}} \dot{\varphi} t}=e^{-m \lambda_{\mathrm{D}} t}=e^{-m \frac{t}{\left(t_{1 / 2}\right) \mathrm{D}} \ln 2}=e^{-x \ln 2}=\frac{1}{2^x} \equiv 2^{-x} (12.101)
Equation (12.101) is valid in general irrespective of the activation model used, and is thus valid for the saturation, depletion, as well as depletion–activation model.
(b) The standard equation used for describing the depletion–activation model is in Prob. 251 [see (12.51)] expressed as (T12.47)
N_D(t) = N_P(0) \frac{\sigma_P \dot φ}{\lambda^*_D – \sigma_P \dot φ} [e^{-\sigma_P \dot φ t} – e^{-\lambda^*_D t}] (12.51)
\frac{\mathrm{d} N_{\mathrm{D}}(t)}{\mathrm{d} t}=\sigma_{\mathrm{P}} \dot{\varphi} N_{\mathrm{P}}(t)-\lambda_{\mathrm{D}} N_{\mathrm{D}}(t)-\sigma_{\mathrm{D}} \dot{\varphi} N_{\mathrm{D}}(t)=\sigma_{\mathrm{P}} \dot{\varphi} N_{\mathrm{P}}(t)-\lambda_{\mathrm{D}}^* N_{\mathrm{D}}(t), (12.102)
resulting in the following expression [Prob. 251, see (12.52)] for the daughter activity \mathcal{A}_{\mathrm{D}}^*(t).
\mathcal{A}_{\mathrm{D}} (t) = N_P(0) \frac{\lambda_D \sigma_P \dot φ}{\lambda^*_D – \sigma_P \dot φ}[e^{-\sigma_P \dot φ t} – e^{-\lambda^*_D t} ]= \sigma_{\mathrm{P}} \dot{\varphi} N_{\mathrm{P}}(0) \frac{\frac{\lambda_{\mathrm{D}}}{\lambda_{\mathrm{D}}^*}}{1-\frac{\sigma_{\mathrm{P}} \dot{\varphi}}{\lambda_{\mathrm{D}}^*}}\left[e^{-\sigma_{\mathrm{P}} \dot{\varphi} t}-e^{-\lambda_{\mathrm{D}}^* t}\right] (12.52)
\mathcal{A}_{\mathrm{D}}^*(t)=\lambda_{\mathrm{D}} N_{\mathrm{P}}(t)=\sigma_{\mathrm{P}} \dot{\varphi} N_{\mathrm{P}}(0) \frac{\frac{\lambda_{\mathrm{D}}}{\lambda_{\mathrm{D}}^*}}{1-\frac{\sigma_{\mathrm{P}} \dot{\varphi}}{\lambda_{\mathrm{D}}^*}}\left[e^{-\sigma_{\mathrm{P}} \dot{\varphi} t}-e^{-\lambda_{\mathrm{D}}^* t}\right] (12.103)
where \lambda_{\mathrm{D}}^*=\lambda_{\mathrm{D}}+\sigma_{\mathrm{D}} \dot{\varphi} is the modified decay constant for the daughter accounting for the radioactive daughter decay (through λ_D) as well as the daughter activation \text { (through } \sigma_{\mathrm{D}} \text { and } \dot{\varphi} \text { ). }
Combining (12.103) with (12.96), (12.97), (12.98), and (12.99) as well as recalling that \sigma_{\mathrm{P}} \dot{\varphi} t=x \ln 2 \text { and } \lambda_{\mathrm{D}}^* t=\left(x / m^*\right) \ln 2 we obtain the following expression (T12.57) for the normalized daughter activity y_{\mathrm{D}}^*.
y_{\mathrm{D}}^*(x)=\frac{\mathcal{A}_{\mathrm{D}}(t)}{\sigma_{\mathrm{P}} \dot{\varphi} N_{\mathrm{P}}(0)}=\frac{1}{\varepsilon^*\left(1-m^*\right)}\left[e^{-x \ln 2}-e^{-\frac{x}{m^*} \ln 2}\right]=\frac{1}{\varepsilon^*\left(1-m^*\right)}\left[\frac{1}{2^x}-\frac{1}{2^{\frac{x}{m^*}}}\right] (12.104)
(c) Normalized daughter activity for the depletion model was determined in (12.64) of Prob. 252 as
(1) A comparison of y^∗ _D given by (12.104) for the depletion–activation model with y_D(x) given by (12.105) for the depletion model shows that the two expressions are similar except for the factor ε^∗ which is equal or larger than 1 (ε^∗ ≥ 1) and depends on fluence rate \dot{φ}. A closer look at expressions (12.104) and (12.105) shows that (12.105) of the depletion model actually follows from (12.104) of the depletion– activation model, since, for the depletion model, λ^∗ _D = λ_D\ and\ ε^∗ = 1 as a result of σ_D = 0. We conclude that the depletion model is a special case of the depletion– activation model when the activation cross section σ_D of the daughter nucleus is zero. Thus, we expect the behavior of y^∗ _D(x) of the depletion–activation model to be similar to that of y_D(x) of the depletion model: rise from 0 at x = 0 to reach a maximum \left(y^∗ _D\right)_{max} at x = \left(x^∗ _D\right)_{max}, and then asymptotically decrease to 0 as x → ∞.
(2) The characteristic normalized time \left(x_{\mathrm{D}}^*\right)_{\max } \text { at which } y_{\mathrm{D}}^* exhibits its maximum \left(y_{\mathrm{D}}^*\right)_{\max } can be determined as a function of the activation factor m^* by setting \mathrm{d} y_{\mathrm{D}}^* /\left.\mathrm{d} x\right|_{x=\left(x_{\mathrm{D}}^*\right)_{\max }} \text { and solving for }\left(x_{\mathrm{D}}^*\right)_{\max } as follows
Solving (12.106) for (x^∗_D)_{max} we now get
2^{-(x^*_D)_{max}} = \frac{1}{m^*}2^{-(x^*_D)_{max} / m^*} or -(x^*_D)_{max} \ln 2 = \ln \frac{1}{m^*} – \frac{(x^*_D)_{max}}{m^*} \ln 2 (12.107)
and finally the following expression for \left(x^∗ _D\right)_{max}
\left(x_{\mathrm{D}}^*\right)_{\max }=\frac{m^*}{\left(m^*-1\right)} \frac{\ln m^*}{\ln 2} . (12.108)
For m^*=1 (12.108) is not defined; however, since it gives \left(x_{\mathrm{D}}^*\right)_{\max }=0 / 0, we can apply the l’Hôpital rule to get \left.\left(x_{\mathrm{D}}^*\right)_{\max }\right|_{m \rightarrow 1} as follows
\left.\left(x_{\mathrm{D}}^*\right)_{\max }\right|_{m^* \rightarrow 1}=\lim _{m^* \rightarrow 1} \frac{\frac{\mathrm{d}\left(m^* \ln m^*\right)}{\mathrm{d} m^*}}{\frac{\mathrm{d}\left(m^*-1\right)}{\mathrm{d} m^*} \ln 2}=\lim _{m^* \rightarrow 1} \frac{1+\ln m^*}{\ln 2}=\frac{1}{\ln 2}=1.443 . (12.109)
Thus, \left(x_{\mathrm{D}}^*\right)_{\max } is given by (12.108) for any positive m^* \text { except for } m^*=1 for which \left(x_{\mathrm{D}}^*\right)_{\max }=1.443, as determined in (12.109).
(3) The maximum daughter activity \left(y_{\mathrm{D}}^*\right)_{\max } can be determined by inserting \left(x_{\mathrm{D}}^*\right)_{\max } \text { of }(12.108) \text { into } y_{\mathrm{D}}^*(x) given by (12.104) as follows
Components F_1^* \text { and } F_2^* \text { of }(12.110) \text {, after insertion of }\left(x_{\mathrm{D}}^*\right)_{\max } given by (12.108) and using the following identity e^{z \ln 2}=e^{\ln 2^z}=2^z, yield the following expressions
F_1^*=\frac{1}{2^{\left(x_{\mathrm{D}}^*\right)_{\max} }}=\frac{1}{2^{\frac{m^*}{\left(m^*-1\right)} \frac{\ln m^*}{\ln 2} }}= 2^{\frac{m^*}{(1 – m^*)}\frac{\ln m^*}{\ln 2}} =e^{\ln 2^{\frac{m^*}{\left(1-m^*\right)} \frac{\ln m^*}{\ln 2}}}=e^{\frac{m^*}{1-m^*}} \ln m^* (12.111)
and
F_2^*=\frac{1}{2^{\left(x_{\mathrm{D}}^*\right)_{\max }\left[\frac{1-m^*}{m^*}\right]}}=\frac{1}{2^{\frac{m^*}{\left(m^*-1\right)} \frac{\ln m^*}{\ln 2}\left[\frac{1-m^*}{m^*}\right]}}=2^{\frac{\ln m^*}{\ln 2}}=e^{\ln m^*}=m^* . (12.112)
The maximum normalized daughter activity \left(y^∗ _D\right)_{max} of (12.109) after incorporating F_1^* \text { of (12.111) and } F_2^* of (12.112) can now be written as follows