Implications of a weakening N=126 shell closure away from stability for r-process astrophysical conditions
The formation of the third r-process abundance peak near A ∼ 195 is highly sensitive to both nuclear structure far from stability and the astrophysical conditions that produce the heaviest elements. In particular, the N=126 shell closure plays a crucial role in shaping this peak. Experimental data h...
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| Auteurs principaux: | , , |
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| Format: | Artigo |
| Langue: | Inglês |
| Publié: |
Elsevier
2026-01-01
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| Collection: | Physics Letters B |
| Sujets: | |
| Accès en ligne: | http://www.sciencedirect.com/science/article/pii/S0370269325008664 |
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