Abstract

We analyze the evolution of the spin-orbit splittings in the Ca isotopes and in the $N=28$ isotones. We also focus on the reduction of the spin-orbit splittings associated with $f$ and $p$ orbits from $^{48}\mathrm{Ca}$ to $^{46}\mathrm{Ar}$. We conclude that adding the tensor contribution can qualitatively explain in most cases the empirical trends, whereas this is not the case if one simply employs existing Skyrme parametrizations without the tensor force.

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.