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Table 3.
Comparison of the rms deviations between simulated abundances from various nuclear physics models and observed abundances in r-process-enhanced metal-poor stars.
| Model | σ(Y) |
|---|---|
| FRDM2012 | 0.456 |
| HFB27 | 0.380 |
| DZ31 | 0.372 |
| WS4 | 0.347 |
Notes. Average abundances from six astrophysical models for neutron star mergers with the average abundances observed in eight r-process-enhanced metal-poor stars.
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