Abstract
The shell model (SM) is used to calculate the energy levels and transition probabilities B(E2) for 18,19,20 O isotopes. Two interactions (USDA and USDB) are used in the SDPN model space. We assume that all possible many-nucleon configurations are defined by the 0d5/2, 1s1/2, and d3/2 states that are higher than in 16 O doubly magic nucleus. The available empirical data are in a good agreement with theoretical energy levels predictions. Spins and parities were affirmed for new levels, and the transition probabilities B(E2; ↓) are predicted.
Publisher
National Academy of Sciences of Ukraine (Co. LTD Ukrinformnauka)
Subject
General Physics and Astronomy
Reference24 articles.
1. Ab initio shell model with a genuine three-nucleon force for the p-shell nuclei.;Navratil;Nucl Th,2003
2. Effective interactions for sd-shell-model calculations.;Fiase;J Phys G Nucl Phys,1988
3. Level structure of 210Po by means of surface delta interaction.;Hasan;Turk J Phys,2013
4. Systematic study of shell-model effective interaction in sd shell.;Wang,2014
5. Semi-empirical effective interaction for the (1s − 0d).;Brown;Ann Phys,1988
Cited by
6 articles.
订阅此论文施引文献
订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献