Analysis of the solar-system r-process abundance pattern with the new ETFSI-Q mass formula
- 1 September 1997
- journal article
- Published by Springer Nature in The European Physical Journal A
- Vol. 357 (3) , 235-238
- https://doi.org/10.1007/s002180050237
Abstract
No abstract availableKeywords
This publication has 19 references indexed in Scilit:
- Nuclear mass formula with Bogolyubov-enhanced shell-quenching: application to r-processPhysics Letters B, 1996
- Beta-Decay Half-Lives and Neutron-Emission Probabilities of Very Neutron-Rich Y to Tc IsotopesPhysical Review Letters, 1996
- Nuclear mass formula via an approximation to the Hartree—Fock methodAtomic Data and Nuclear Data Tables, 1995
- Influence of shell-quenching far from stability on the astrophysical r-processPhysics Letters B, 1995
- Nuclear Ground-State Masses and DeformationsAtomic Data and Nuclear Data Tables, 1995
- Nuclear properties far from stability and the R-processAIP Conference Proceedings, 1995
- Closed shells at drip-line nucleiPhysica Scripta, 1995
- 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
- s-process nucleosynthesis-nuclear physics and the classical modelReports on Progress in Physics, 1989