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- W4385220452 endingPage "138092" @default.
- W4385220452 startingPage "138092" @default.
- W4385220452 abstract "The sensitivity of the r-process rare-earth peak abundances to nuclear masses has been studied in different astrophysical scenarios. The most impactful nuclei lie along the r-process paths at r-process freeze-out and at the time when the neutron-capture timescale is approximately 3 times of the β-decay timescale (τnγ≈3τβ), corresponding to the onset and completion of rare-earth peak formation, respectively. In astrophysical scenario with fission involved, the sensitivities for nuclei lying along the r-process path at freeze-out are masked by the large contribution of fission products to the rare-earth peak abundances. This work provides recommended targets for future researches and thus helps to increase the understanding of rare-earth peak formation mechanism and the efficacy of the rare-earth peak as an r-process site diagnostic." @default.
- W4385220452 created "2023-07-25" @default.
- W4385220452 creator A5001678665 @default.
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- W4385220452 date "2023-09-01" @default.
- W4385220452 modified "2023-10-14" @default.
- W4385220452 title "Sensitivity of the r-process rare-earth peak abundances to nuclear masses" @default.
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- W4385220452 doi "https://doi.org/10.1016/j.physletb.2023.138092" @default.
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