Strong magnetic fields could exist in the inner region of the supernova. The phase space of the electrons is quantized inside the magnetic field so that the weak interaction rates deviate from the field-free case. This talk focuses on the (anti)neutrinos absorption process. This process is essential since it determines the opacity of the neutrino and the position of the (anti) neutrino sphere. Moreover, we will show that the evolution of the electron fraction 𝑌𝑒 is also affected by the magnetic field since its value depends on the inverse reaction of the neutrino process. Such impact could leave an imprint on the nucleosynthesis yields.
Yudong Luo graduated from the University of Tokyo with a Ph.D. in 2021, and served as a Ph.D. and postdoctoral researcher at the Japan Society for the Promotion of Science (JSPS). He is currently a Boya Postdoctoral Fellow at Peking University. His research interests include big bang cosmology, big bang nucleosynthesis and nucleosynthesis in explosive events.