First direct limit on the 395 keV resonance of the 22Ne(α, γ)26Mg reaction
The 22Ne(α, γ)26Mg reaction (Q = 10614.74 keV) competes with the 22Ne(α, n)25Mg reaction (Q = −478.34 keV) which is the main source of neutrons for the s-process in low-mass Asymptotic Giant Branch and massive stars. The cross sections of these reactions are crucial to fix the cross over temperature...
Збережено в:
| Автор: | |
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| Формат: | Artigo |
| Мова: | Inglês |
| Опубліковано: |
EDP Sciences
2022-01-01
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| Серія: | EPJ Web of Conferences |
| Онлайн доступ: | https://www.epj-conferences.org/articles/epjconf/pdf/2022/04/epjconf_nic16th2022_11017.pdf |
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