Is e+e- pair emission important in the determination of the 3He+4He S factor?

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Hydrostatic Stellar Nucleosynthesis, Radiative Capture, Internal Pair Production, Solar Neutrinos

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We show that the cross section for direct E0 pair emission is related to the cross section for direct E2 photon emission, and is a negligible contribution to the total capture cross section for 3He+4He→7Be. E0 resonance emission, E1 pair emission, and internal conversion are also negligible. Thus there cannot be significant contributions to the 3He+4He→7Be capture cross section at low energies from electromagnetic emission processes other than single photon emission.

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