Influence of shell-quenching far from stability on the astrophysical r-process
- 27 July 1995
- journal article
- Published by Elsevier in Physics Letters B
- Vol. 355 (1-2), 37-44
- https://doi.org/10.1016/0370-2693(95)00737-6
Abstract
No abstract availableKeywords
This publication has 22 references indexed in Scilit:
- The r-process and neutrino-heated supernova ejectaThe Astrophysical Journal, 1994
- Astrophysics and nuclei far from stabilitysNuclear Physics A, 1994
- Isotopic r-process abundances and nuclear structure far from stability - Implications for the r-process mechanismThe Astrophysical Journal, 1993
- Thomas-Fermi approach to nuclear-mass formulaNuclear Physics A, 1992
- R-process nucleosynthesis in the high-entropy supernova bubbleThe Astrophysical Journal, 1992
- The R-process and nucleochronologyPhysics Reports, 1991
- New developments in the calculation of β-strength functionsNuclear Physics A, 1990
- s-process nucleosynthesis-nuclear physics and the classical modelReports on Progress in Physics, 1989
- Synthesis of the Elements in StarsReviews of Modern Physics, 1957
- Origin of Anomalous Abundances of the Elements in Giant Stars.The Astrophysical Journal, 1955