2025ApJ...995...34L

We consider the question of whether core-collapse supernovae (CCSNe) can produce rapid neutron capture process (r-process) elements and how future MeV gamma-ray observations could address this. Rare types of CCSNe characterized by substantial magnetic fields and rotation, known as magnetorotational supernovae (MR-SNe), are theoretically predicted to produce these elements, although direct observational evidence is lacking. We suggest that this critical question be addressed through the study of some of the 11 CCSN remnants located within 10 kpc, as well as through the detection of gamma-ray emission from a future Galactic supernova. We use a two-dimensional MR-SN model to estimate the expected gamma flux stemming from nuclear decays in the range of a few tens of keV to a few MeV. Our results indicate that an observation of ¹²⁶Sn (¹²⁶Sb) in a remnant stands out as a signature of an r-process-producing supernova. Since the neutron-rich conditions that lead to the production of the r-process could also enhance the production of ⁶⁰Fe, the detection of substantial ⁶⁰Fe (⁶⁰Co) would be indicative of favorable conditions for the r-process. In the case of a future supernova explosion, when the evolution of the spectrum is studied over 10 days to a few years, a rich picture emerges. At various epochs, the second peak r-process isotopes such as ¹²⁵Sn, ¹³¹I, ¹³²Te, ¹³²I, and ¹⁴⁰La produce signals that are not obscured by the gamma emission from explosive burning products and electron-positron annihilation. The weak r-process isotopes ⁹⁵Nb, ¹⁰³Ru, and ¹⁰⁶Rh also have periods of prominence.