For every daughter energy level, the total number leaving it must equal direct beta feeding plus cascades entering it. Direct feeding cannot be negative. This nuclear level population balance gives a decisive test without assuming any electromagnetic transition-strength model.
In scheme B, the first excited level is populated by and , with counts . Its only downward transition is , whose count is . Its direct beta feeding would therefore have to bewhich is impossible.
For scheme A the corresponding direct feeding values, in the same arbitrary count normalization, areAll are non-negative. Thus scheme A is the compatible scheme. Under the stipulated complete decay sample and the six-transition model, scheme B is ruled out by population conservation, rather than merely being less probable. This inference assumes that the reported emitted-photon counts account for de-excitation: substantial unreported internal conversion or other decay paths would require additional terms.
Let be the common normalization converting the quoted to photon numbers per parent decay. Apply nuclear level population balance to scheme A, starting with the top level:For example, the transition contributes to the population of level 2; it must be subtracted from the total leaving level 2 to obtain its direct beta feeding. Similarly, a photon in the strong line need not imply a direct beta transition to level 1.
The three equations giveAdding them cancels the internal cascade counts:This also has a simple physical meaning: each decay that initially feeds an excited daughter eventually contributes exactly one of the three transitions into the ground state. The number of all emitted photons is not the correct normalization, because a single cascade can emit several.
Consequently the required formulae are