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In this paper, we consider the reprocessing of high‐frequency photons emitted by He  ii  and He  i  during the epoch of cosmological recombination by He  i  and H  i . We demonstrate that, in comparison to computations which neglect all feedback processes, the number of cosmological recombination photons that are related to the presence of helium in the early Universe could be increased by ∼40–70 per cent. Our computations imply that per helium nucleus ∼3–6 additional photons could be produced. Therefore, a total of ∼12–14 helium‐related photons per helium atom are emitted during cosmological recombination. This is an important addition to cosmological recombination spectrum which in the future may render it slightly easier to determine the primordial abundance of helium using differential measurements of the cosmic microwave background (CMB) energy spectrum. Also, since these photons are the only witnesses of the feedback process at high redshift, observing them in principle offers a way to check our understanding of the recombination physics. Here, most interestingly, the feedback of He  ii  photons on He  i  leads to the appearance of several additional, rather narrow spectral features in the He  i  recombination spectrum at low frequencies. Consequently, the signatures of helium‐related features in the CMB spectral distortion from cosmological recombination at some given frequency can exceed the average level of ∼17 per cent several times. We find that in particular the bands around  ν∼ 10, ∼35, ∼80  and  ∼200 GHz  seem to be affected strongly. In addition, we computed the changes in the cosmological ionization history, finding that only the feedback of primary He  i  photons on the dynamics of He  ii → He  i  recombination has an effect, producing a change of  Δ N  e / N  e ∼+0.17  per cent at   z ∼ 2300 . This result seems to be  ∼2–3  times smaller than the one obtained in earlier computations for this process, however, the difference will not be very important for the analysis of future CMB data.

Cosmological recombination: feedback of helium photons and its effect on the recombination spectrum