Probing the Z = 6 spin-orbit shell gap with (p,2p) quasi-free scattering reactions
arXiv:2008.10126 · doi:10.1016/j.physletb.2020.135748
Abstract
The evolution of the traditional nuclear magic numbers away from the valley of stability is an active field of research. Experimental efforts focus on providing key spectroscopic information that will shed light into the structure of exotic nuclei and understanding the driving mechanism behind the shell evolution. In this work, we investigate the Z = 6 spin-orbit shell gap towards the neutron dripline. To do so, we employed N(p,2p)C quasi-free scattering reactions to measure the proton component of the 2 state of C. The experimental findings support the notion of a moderate reduction of the proton 1p-1p spin-orbit splitting, at variance to recent claims for a prevalent Z = 6 magic number towards the neutron dripline.
arXiv comment27 pages, 5 figures, 2 tables. Submitted to Physics Letter B
References in corpus (9)
- Nuclear magic numbers: new features far from stability
- Tables of E2 Transition Probabilities from the first States in Even-Even Nuclei
- Systematics of intermediate-energy single-nucleon removal cross sections
- Role of Long-Range Correlations on the Quenching of Spectroscopic Factors
- Quasi-free (p,2p) and (p,pn) reactions with unstable nuclei
- Quenching of spectroscopic factors for proton removal in oxygen isotopes
- Evidence for Z=6 `magic number' in neutron-rich carbon isotopes
- Spectroscopic Factors in 16O and Nucleon Asymmetry
- Nucleon-nucleon correlations and the single-particle strength in atomic nuclei