Nuclear Properties for Astrophysical Applications
Abstract
We tabulate the ground-state odd-proton and odd-neutron spins and parities, proton and neutron pairing gaps, binding energy, one- and two-neutron separation energies, quantities related to beta-delayed one- and two-neutron emission probabilities, beta-decay energy release and half-life with respect to Gamow-Teller decay, one- and two-proton separation energies, and alpha-decay energy release and half-life for 8979 nuclei ranging from oxygen-16 to Z = 136, A = 339 and extending from the proton drip line to the neutron drip line. Single-particle level diagrams and other quantities are also presented in graphical form. The starting point of our present work is a study of nuclear ground-state masses and deformations based on the finite-range droplet model and folded-Yukawa single-particle potential published in a previous issue of Atomic Data and Nuclear Data Tables. The beta-delayed neutron-emission probabilities and Gamow-Teller beta-decay rates are obtained from a quasi-particle random-phase approximation with single-particle levels and wave functions at the calculated nuclear ground-state shapes as input quantities.
Cite
@article{arxiv.nucl-th/9601043,
title = {Nuclear Properties for Astrophysical Applications},
author = {P. Moller and J. R. Nix and K. -L. Kratz},
journal= {arXiv preprint arXiv:nucl-th/9601043},
year = {2007}
}
Comments
42 pages. LaTeX. Submitted to Atomic Data and Nuclear Data Tables. 99 figures and 160-page table not included here. Complete preprint, including device-independent (dvi), PostScript, and LaTeX versions of the text and table, plus PostScript files of the figures, available at http://t2.lanl.gov/pub/publications/publications.html or at ftp://t2.lanl.gov/pub/publications/astro