Long Gamma Ray Bursts (GRBs) are linked to the core collapse of massive stars, and in many cases Type Ic supernovae. Here, the authors identify that the time-evolving emission line in GRB 221009A is consistent with Doppler-boosted 56Ni decay, providing insights into supernova nucleosynthesis and relativistic jet dynamics.
- Rahim Moradi
- Emre S. Yorgancioglu
- Yu Wang