Abstract

The nuclei below lead but with more than 126 neutrons are crucial to an understanding of the astrophysical rr-process in producing nuclei heavier than A∼190A\sim190. 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 207^{207}Hg have been probed using the neutron-adding (dd,pp) reaction in inverse kinematics. The radioactive beam of 206^{206}Hg was delivered to the new ISOLDE Solenoidal Spectrometer at an energy above the Coulomb barrier. The spectroscopy of 207^{207}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 rr-process.

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