Theory of Successive Transformation and Radioactive Equilibrium
Any radioactive atom decays to its daughter atom following its characteristics decay constant. The daughter atom, if radioactive, decays to third generation and in this manner a chain of decay propagates, which eventually stops by the formation of a stable nucleus. Let us consider a radioactive nuclide, symbolized by a subscript p (Parent nucleus) to decay into another radioactive nuclide (subscript d: daughter nucleus); which again decays to a stable end product (subscript 3). Let λp, λd be the decay constants of nuclides p and d respectively, and Np, Nd and N3 be the number of atoms of the three kinds at any instant. The second nuclide would be formed at the rate of λpNpby the decay of the parent atom, and would decay at the rate of λdNd. In the same manner, the atoms of the end product will appear at the rate λdNd by the decay of nuclide, but being stable will not decay. Therefore,1 | ||
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Solving Eq. (m4.13), we have | ||
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where, ![]() From (m4.14) using (m4.16), we have | ||
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Multiplying both sides by ![]() | ||
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where, A is the constant of integration. Now, at t =0,Nd = N0d = a constant. So, from Eqn. (m4.17), | ||
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From above equations, | ||
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where, B is the integration constant. Now at t =0,N3 = N03, so that we have from Eqn. 6.17, | ||
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In practical cases, as only the first nuclide is present at t = 0, we can put N0d = N03 and from Eqns. 6.16 to 6.18, we get | ||
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The decay of the parent nuclide and the growth and decay of the daughter nuclide are shown in Fig. m4.2. | ||
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FIGURE m4.2 Decay of the parent nuclide and growth and decay of the first daughter nuclide with time | ||
Example m4.2: Show that if N0p be the number of parent atoms initially and γp and γd the disintegration constants of parent and daughter respectively, the time at which the number of daughter atoms is maximum is given by | ||
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Solution: | ||
From the relation m4.22, we get, ![]() ![]() ![]() ![]() | ||
⇒ ![]() | ||
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Radioactive Equilibrium | ||
When we consider a radioactive series, it is important to understand the equilibrium conditions of all the nuclei in the respective chain. Applying the mathematical condition of equilibrium, i.e., time derivative of any quantity is equal to zero, we can write from | ||
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Where 1, 2, —- n and represents parent, daughter and so on upto nth nucleus. It is clear from Eqn. (m4.25) that the first equation is not valid as it implies λ1 to be zero. Therefore, the mathematical condition of equilibrium cannot be applied here rigorously. However, some conditions can be set in to attain a state very close to equilibrium. Depending on the conditions, two equilibrium states can be defined: | ||
Secular Equilibrium (λ1<< other λ’s) | ||
In this case the first equation of 6.22 can be considered to certain approximation and hence we can write, | ||
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or![]() | ||
As in this case λ1 ![]() ![]() ![]() | ||
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After a long time ![]() | ||
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This is known as secular equilibrium. | ||
Transient Equilibrium (λ1<λ2 but (T1/2)1 is not very long) | ||
In this case λ1 ~ 0 does not hold good. When t becomes large,![]() | ||
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This indicates that daughter decays with the same half life of the parent. This is basically the condition of transient equilibrium. From equations m4.1 and m4.28, we can write | ||
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Example m4.3: Calculate the amount of Ra-226 in secular equilibrium with 5 kg of pure U-238, given the half life of 226Ra and 238U as 1620 years and 4.5 x 109 years respectively. | ||
Solution: | ||
Let x gm be the required amount of 226Ra in secular equilibrium with 5 kg of pure 238U. Now, | ||
5 kg of pure U-238 = ![]() | ||
x gm of Ra-226 = ![]() | ||
From the condition of secular equilibrium | ||
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x = 1.7 mg |