Probing Isospin Dynamics in Halo Nuclei
Abstract
Nuclear many-body theory is used to study nuclear matter and finite nuclei at extreme isospin. In-medium interactions in asymmetric nuclear matter are obtained from (Dirac-) Brueckner theory. Neutron skin formation in Ni and Sn isotopes is investigated by relativistic mean-field calculations in DDRH theory with density dependent meson-nucleon vertices. Applications to light nuclei are discussed with special emphasis on pairing and core polarization in weakly bound nuclei. Approaches accounting for continuum coupling in dripline pairing and core polarization are presented. Calculations for the halo nuclei B, Be and C show that shell structures are dissolving when the driplines are approached. Relativistic breakup data are well described by eikonal calculations.
Cite
@article{arxiv.nucl-th/0012082,
title = {Probing Isospin Dynamics in Halo Nuclei},
author = {H. Lenske and F. Hofmann and C. M. Keil},
journal= {arXiv preprint arXiv:nucl-th/0012082},
year = {2009}
}
Comments
10 pages, 8 figures