Precision masses of neutron-rich platinum and gold nuclei reveal enhanced shell strength below doubly-magic Pb
Through precision mass measurements of neutron-rich platinum and gold isotopes at GSI, an international collaboration of experimentalists and theorists discovered that the shell strength fades less rapidly than expected below doubly-magic lead-208. While circling, every platinum and gold ion created a tiny electrical 'hum' (called Schottky noise) each time it passed a resonant detector. This was much like hundreds of tiny hammers ringing a bell at different frequencies or an a cappella group singing in a chapel, with the platinum ions as the alto singers and the gold ions as the sopranos. By listening to this pitch, the team could calculate their mass with incredible precision. Specifically, platinum-204 and gold-205 were found to be lighter than predicted, suggesting a bifurcation that separates the gold–mercury trend from the thallium–lead trend near , though further mass measurements are required to determine if this bifurcation also exists in platinum. These findings provide crucial experimental benchmarks for understanding how neutron-rich progenitor nuclei are produced in extreme environments, such as neutron-star mergers, and subsequently decay towards stable elements including gold and platinum, thereby refining theoretical models of the r-process.