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Tang, T L; Kay, B P; Hoffman, C R; Schiffer, J P; Sharp, D K; Gaffney, L P; Freeman, S J; Mumpower, M R; Arokiaraj, A; Baader, E F; Butler, P A; Catford, W N; de Angelis, G; Flavigny, F; Gott, M D; Gregor, E T; Konki, J; Labiche, M; Lazarus, I H; MacGregor, P T; Martel, I; Page, R D; Podolyák, Zs; Poleshchuk, O; Raabe, R; Recchia, F; Smith, J F; Szwec, S V; Yang, J
Physical review letters, 2020-Feb-14, Volume: 124, Issue: 6Journal Article
The nuclei below lead but with more than 126 neutrons are crucial to an understanding of the astrophysical r process in producing nuclei heavier than A∼190. 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}Hg have been probed using the neutron-adding (d,p) reaction in inverse kinematics. The radioactive beam of ^{206}Hg was delivered to the new ISOLDE Solenoidal Spectrometer at an energy above the Coulomb barrier. The spectroscopy of ^{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 r process.
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