The 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 radiative capture below 1 MeV for both electric dipole () and magnetic dipole () transitions. The obtained astrophysical 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 including both transitions is determined to be eV b. A comparison with experimental data using the test reveals the sensitivity of the cross section at low energies to the scattering potential depth.

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