Nuclei beyond the drip line
核理论
2009-02-06 v1
摘要
In a Thomas-Fermi model, calculations are presented for nuclei beyond the nuclear drip line at zero temperature. These nuclei are in equilibrium by the presence of an external gas, as may be envisaged in the astrophysical scenario. We find that there is a limiting asymmetry beyond which these nuclei can no longer be made stable.
引用
@article{arxiv.nucl-th/0108071,
title = {Nuclei beyond the drip line},
author = {J. N. De and X. Viñas and S. K. Patra and M. Centelles},
journal= {arXiv preprint arXiv:nucl-th/0108071},
year = {2009}
}
备注
Physical Review C (in press), 1 ReVteX file for text, 4 PS-files for figures