We examine the ratio of the decay rate of the eta, into light hadrons to th
e decay rate into photons and find that most of the large next-to-leading-o
rder (NLO) correction is associated with running of the strong coupling alp
ha We resum Such contributions by analyzing final-state chains of vacuum-po
larization bubbles. We show that the nonperturbative parts of the bubble ch
ains can be absorbed into a color-octet matrix element, once one has used c
ontour deformations, of the phase-space integrals to cancel certain contrib
utions. We argue that these contributions are incompatible with the uncerta
inty principle, We also argue that perturbation theory is reliable only if
one carries out the phase-space integrations before the perturbation summat
ion. Our results are in good agreement with experiment and differ considera
bly from those that one obtains by applying the scale-setting method of Bro
dsky. Lepage. and Mackenzie to the NLO result.