Abstract
A study is made on such halo states that are isobaric analogues of the neutron-halo states confirmed in the neutron drip-line nuclei. A simple formula enables us to predict the excitation energies of the analogue halos. A semi-quantitative estimate of their decay widths encourages us to pursue both experimental and theoretical investigation, for example, in the A=11 isobars.
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 callDisclaimer: 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.
