C. Winteler

TL;DR: In this paper, the authors explore nucleosynthesis in the dynamic ejecta of compact binary mergers and compare the results with those from two simulations of a neutron star black hole merger.

TL;DR: In this article, the nucleosynthesis in the dynamic ejecta of compact binary mergers is explored and the authors compare the results with those from two simulations of a neutron star black hole merger.

TL;DR: In this paper, the authors examined magnetorotationally driven supernovae as sources of r-process elements in the early Galaxy and found that the peak distribution of Ye in the ejecta is shifted from 0.15 to 0.17 and broadened toward higher Ye due to neutrino absorption.

TL;DR: In this article, the authors examined magnetorotationally driven supernovae as sources of $r$-process elements in the early Galaxy and found that the peak distribution of $Y_{e}$ in the ejecta is shifted from 0.15$ to 0.17$ and broadened toward higher values due to neutrino absorption.

TL;DR: In this paper, three of the four nucleosynthesis processes involved in producing heavy nuclei beyond Fe (with a main focus on the r -process) are identified with explosive Ne/O-burning in outer zones of the progenitor star.