In nuclear physics, secular equilibrium is a situation in which the quantity of a radioactive isotope remains constant because its production rate (e.g., due to decay of a parent isotope) is equal to its decay rate. An example of this is the germanium-68/gallium-68 generator commonly used for the preparation of gallium-68 radiopharmaceuticals for PET imaging.
In radioactive decay Secular equilibrium can occur in a radioactive decay chain only if the half-life of the daughter radionuclide B is much shorter than the half-life of the parent radionuclide A. In such a case, the decay rate of A and hence the production rate of B is approximately constant, because the half-life of A is very long compared to the time scales considered. The quantity of radionuclide B builds up until the number of B atoms decaying per unit time becomes equal to the number being produced per unit time. The quantity of radionuclide B then reaches a constant, equilibrium value. Assuming the initial concentration of radionuclide B is zero, full equilibrium usually takes several half-lives of radionuclide B to establish. The quantity of radionuclide B when secular equilibrium is reached is determined by the quantity of its parent A and the half-lives of the two radionuclide. That can be seen from the time rate of change of the number of atoms of radionuclide B:
d N B d t = λ A N A − λ B N B , {\displaystyle {\frac {dN_{B}}{dt}}=\lambda _{A}N_{A}-\lambda _{B}N_{B},}
where λA and λB are the decay constants of radionuclide A and B, related to their half-lives t1/2 by λ = ln ( 2 ) / t 1 / 2 {\displaystyle \lambda =\ln(2)/t_{1/2}} , and NA and NB are the number of atoms of A and B at a given time. Secular equilibrium occurs when d N B / d t = 0 {\displaystyle dN_{B}/dt=0} , or
N B = λ A λ B N A . {\displaystyle N_{B}={\frac {\lambda _{A}}{\lambda _{B}}}N_{A}.}
Over long enough times, comparable to the half-life of radionuclide A, the secular equilibrium is only approximate; NA decays away according to
N A ( t ) = N A ( 0 ) e − λ A t , {\displaystyle N_{A}(t)=N_{A}(0)e^{-\lambda _{A}t},}
and the "equilibrium" quantity of radionuclide B declines in turn. For times short compared to the half-life of A, λ A t ≪ 1 {\displaystyle \lambda _{A}t\ll 1} and the exponential can be approximated as 1.
See also Bateman equation Transient equilibrium
References
IUPAC definition "secular equilibrium", IUPAC definition (IUPAC Compendium of Chemical Terminology 2nd Edition, 1997) (in English) Radioactive Equilibrium, EPA definition Radioactive Equilibrium. An equilibrium as old as the Earth Archived 2019-07-28 at the Wayback Machine, radioactivity.eu.com, IN2P3, EDP Science
