1999/11/16 by Oe. Elgaroey, T. Engeland, Elgaroey, Oe. +6
Physics and Astronomy · #Atomic and Subatomic Physics Research #FOS: Physical sciences #Nuclear Physics and Applications #Nuclear Theory (nucl-th) #Pulsars and Gravitational Waves Research #nucl-th
paper · pdf · doi:10.48550/arxiv.nucl-th/9911053
9 pages, 2 figs, world-scientific latex style. Proceedings of Many-Body X, Seattle, 10-15 sept 1999
arxiv created 1999/11/16 · openalex publication_date 1999/11/16 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Finite nuclei such as those found in the chain of even tin isotopes from 102Sn to 130Sn, exhibit a near constancy of the 2+1-0+1 excitation energy, a constancy which can be related to strong pairing correlations and the near degeneracy in energy of the relevant single particle orbits. Large shell-model calculations for these isotopes reveal that the major contribution to pairing correlations in the tin isotopes stems from the 1S0 partial wave in the nucleon-nucleon interaction. Omitting this partial wave and the 3P2 wave in the construction of an effective interaction, results in a spectrum which has essentially no correspondence with experiment. These partial wave are also of importance for infinite neutron matter and nuclear matter and give the largest contribution to the pairing interaction and energy gap in neutron star matter.