Bolometric light curve of SN 2024ggi. The bolometric light curve published in Ertini et al. (2025) and their preferred model are plotted in pink dots and line, respectively. Our fitting of Eq. (1) is shown in purple. A new hydrodynamical model with the same parameters as those presented in Ertini et al. (2025), but with a larger ⁵⁶Ni mass of 0.052 M_⊙ is shown in the cyan line. The dashed gray line indicates the decay with a ⁵⁶Ni mass of 0.049 M_⊙ and full-trapping of γ rays.