Schramm, D.N. (1973) Explosive r-Process Nucleosynthesis. In: Schramm, D.N. and Arnett, W.D., Eds., Explosive Nucleosynthesis, University of Texas Press, Austin, 84.
https://ui.adsabs.harvard.edu/abs/1973ApJ...185..293S/abstract

has been cited by the following article:

• TITLE: Competition of Electron Capture and Beta Decay Rates in Explosive Astrophysical Scenario of Type II Supernova

  AUTHORS: Rulee Baruah, Kalpana Duorah, Hira Lal Duorah

  KEYWORDS: Protoneutron Star, Weak Interaction Processes, Neutrinos

  JOURNAL NAME: World Journal of Nuclear Science and Technology, Vol.12 No.2, April 29, 2022

  ABSTRACT: Stellar weak interaction processes play a significant role during the supernova explosion condition after collapse leading to the formation of neutron star. In dynamic events like core-collapse supernovae the high entropy wind scenario arises from considerations of the newly born proto-neutron star. Here, the late neutrinos interact with matter of the outermost neutron star layers leading to moderately neutron rich ejecta. We study the electron capture and beta decay rates of Co and Cd isotopes at various temperature and density conditions in an astrophysical environment and found that the beta decay rates are much higher than the corresponding electron capture rates at all the conditions.