Origin of the rare-earth abundance peak
In plain words
The solar system has a small extra bump in the abundances of rare-earth elements near mass 160. Whether it comes from nuclear deformation (nuclei becoming non-spherical) late in the r-process or from fission fragments is not known.
Precise statement
Determine whether the r-process rare-earth peak at $A$ about 160 forms by trapping of material at deformed nuclei near $N$ about 104 during freeze-out (Surman et al., 1997) or by deposition of fission fragments, and identify the nuclear properties (masses and half-lives for $Z = 60\ \text{to}\ 66, N = 100\ \text{to}\ 110$) that control it. Answer: the mechanism and the specific nuclei whose properties set the peak.
What would settle it
Mass and half-life measurements across the neutron-rich lanthanides at FRIB and CARIBU, fed into network calculations for merger and collapsar conditions.
Status in the literature
Unverified note: it names recent work and was partly written without a live literature search; it awaits a check by an editor.
Mass measurements of neutron-rich lanthanides at Argonne since about 2016 began to test the deformation mechanism without deciding between the two pictures as of 2026.
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