Bradley S. Meyer

TL;DR: In this article, a simulation of a 20 solar mass "delayed" supernova explosion is presented, where the authors follow the detailed evolution of material moving through the bubble at the late times appropiate to r-process nucleosynthesis.

TL;DR: A review of low energy nuclear experiments and theory, stellar modeling over a wide range of mass and composition, and abundance studies of many hundreds of stars can be found in this paper.

TL;DR: In this paper, the steady-state eigenvalue problem of neutrino-driven proto-neutron star winds was solved and the authors derived the entropy, dynamical timescale, and neutron-to-seed ratio in the general relativistic framework.

TL;DR: In this paper, it was shown that the high-temperature, high-entropy evacuated region outside the recent neutron star in a core-collapse supernova may be an ideal r-process site.

TL;DR: Burbidge et al. as discussed by the authors showed that the heavy nuclei were formed in three distinct nucleosynthetic processes, which they termed the r-, s-, and p-processes.