Abstract
The nuclei below lead but with more than 126 neutrons are crucial to an understanding of the astrophysical process in producing nuclei heavier than . Despite their importance, the structure and properties of these nuclei remain experimentally untested as they are difficult to produce in nuclear reactions with stable beams. In a first exploration of the shell structure of this region, neutron excitations in have been probed using the neutron-adding (,) reaction in inverse kinematics. The radioactive beam of was delivered to the new ISOLDE Solenoidal Spectrometer at an energy above the Coulomb barrier. The spectroscopy of marks a first step in improving our understanding of the relevant structural properties of nuclei involved in a key part of the path of the process.
- Received 6 November 2019
- Revised 12 December 2019
- Accepted 2 January 2020
DOI:https://doi.org/10.1103/PhysRevLett.124.062502
Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI.
Published by the American Physical Society