First Exploration of Neutron Shell Structure Below Lead and Beyond
arXiv:2001.00976 · doi:10.1103/PhysRevLett.124.062502
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 Hg have been probed using the neutron-adding (,) reaction in inverse kinematics. The radioactive beam of Hg was delivered to the new ISOLDE Solenoidal Spectrometer at an energy above the Coulomb barrier. The spectroscopy of Hg 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.
arXiv comment6 pages, 5 figures
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- Charge radii, moments and masses of mercury isotopes across the N = 126 shell closure
- Systematic shell-model study of Rn isotopes with 207 to 216 and isomeric states
- Isochronic evolution and the radioactive decay of r-process nuclei
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