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The Stellar 72Ge(n, γ) Cross Section for weak s-process: A First Measurement at n_TOF
The slow neutron capture process (s-process) is responsible for producing about half of the elemental abundances heavier than iron in the universe. Neutron capture cross sections on stable isotopes are a key nuclear physics input for s-process studies. The 72Ge(n, γ) Maxwellian-Averaged Cross Sectio...
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| הוצא לאור ב: | EPJ Web of Conferences |
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| Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
| פורמט: | Artigo |
| יצא לאור: |
EDP Sciences
2023-01-01
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| גישה מקוונת: | https://www.epj-conferences.org/articles/epjconf/pdf/2023/10/epjconf_nd2023_01017.pdf |
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