MAGNETOROTATIONALLY DRIVEN SUPERNOVAE AS THE ORIGIN OF EARLY GALAXY r -PROCESS ELEMENTS?

We examine magnetorotationally driven supernovae as sources of r -process elements in the early Galaxy. On the basis of thermodynamic histories of tracer particles from a three-dimensional magnetohydrodynamical core-collapse supernova model with approximated neutrino transport, we perform nucleosynthesis calculations with and without considering the effects of neutrino absorption reactions on the electron fraction ( Y e ) during post-processing. We find that the peak distribution of Y e in the ejecta is shifted from ∼0.15 to ∼0.17 and broadened toward higher Y e due to neutrino absorption. Nevertheless, in both cases, the second and third peaks of the solar r -process element distribution can be reproduced well. The rare progenitor configuration that was used here, characterized by a high rotation rate and a large magnetic field necessary for the formation of bipolar jets, could naturally provide a site for the strong r -process in agreement with observations of the early Galactic chemical evolution.