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The impact of global nuclear mass model uncertainties on r-process abundance predictions

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Figure

Figure 1. Distributions used to sample nuclear masses for ourrepresents a hypothetical improved model with a reduced rms er-ror of 100 keV,monte carlo studies
Figure 3. Variance in isotopic abundance patterns from three uncertain nuclear mass model predictions (HFB-17, DZ, and FRDM1995)compared to the solar r-process residuals (dots)

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