The $pd$ radiative capture reaction plays a vital role in Big Bang nucleosynthesis and stellar proton-proton chain. The study of the low-energy reaction is challenging in both experiments and theories. Using the framework of potential model, we analyze $pd$ radiative capture below 1 MeV for both electric dipole ($E1$) and magnetic dipole ($M1$) transitions. The obtained astrophysical S factors agree well with recent results, especially at energies relevant to sensitive deuterium abundance. The calculated reaction rate shows good agreement, with less than a 5% difference compared to recent works. The extrapolated value for $S(0)$ including both transitions is determined to be 0.211 ± 0.016 eV b. A comparison with experimental data using the χ² test reveals the sensitivity of the $M1$ cross section at low energies to the scattering potential depth.
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Anh et al. (2024) studied this question.
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