activity
19952026
most citedThe consequences of nuclear electron capture in core collapse supernovae

223 citations · 903 across the 11 of their papers we have counts for

collaborators
Showing astro-phShow all

5 papers · 1 filter

astro-ph2008★ 90 cited

The Effects of the pep Nuclear Reaction and Other Improvements in the Nuclear Reaction Rate Library on Simulations of the Classical Nova Outburst

S. Starrfield, C. Iliadis, W. R. Hix +2

We have continued our studies of the Classical Nova outburst by evolving TNRs on 1.25Msun and 1.35Msun WDs (ONeMg composition) under conditions which produce mass ejection and a ra…

astro-ph2003★ 223 cited

The consequences of nuclear electron capture in core collapse supernovae

W. R. Hix, O. E. B. Messer, A. Mezzacappa +5

The most important weak nuclear interaction to the dynamics of stellar core collapse is electron capture, primarily on nuclei with masses larger than 60. In prior simulations of co…

astro-ph2000★ 156 cited

Explosive Nucleosynthesis in Hypernovae

Takayoshi Nakamura, Hideyuki Umeda, Koichi Iwamoto +4

We examine the characteristics of nucleosynthesis in 'hypernovae', i.e., supernovae with very large explosion energies ($ \gsim 10^{52} $ ergs). We carry out detailed nucleosynthes…

astro-ph1998★ 101 cited

Silicon Burning II: Quasi-Equilibrium and Explosive Burning

W. Raphael Hix, Friedrich-Karl Thielemann

Having examined the application of quasi-equilibrium to hydrostatic silicon burning in Paper I of this series, Hix & Thielemann (1996), we now turn our attention to explosive silic…

astro-ph1995★ 126 cited

Silicon Burning I: Neutronization and the Physics of Quasi-Equilibrium

W. R. Hix, F. -K. Thielemann

As the ultimate stage of stellar nucleosynthesis, and the source of the iron peak nuclei, silicon burning is important to our understanding of the evolution of massive stars and su…