High-resolution study of levels in the astrophysically important nucleus Mg26 and resulting updated level assignments-Reference-Cited by-同舟云学术

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High-resolution study of levels in the astrophysically important nucleus Mg26 and resulting updated level assignments

Published:2018-04-30 Issue:4 Volume:97 Page:
ISSN:2469-9985
Container-title:Physical Review C
language:en
Short-container-title:Phys. Rev. C

Author:

Adsley P.,Brümmer J. W.,Faestermann T.,Fox S. P.,Hammache F.,Hertenberger R.,Meyer A.,Neveling R.,Seiler D.,de Séréville N.,Wirth H.-F.

Funder

National Research Foundation

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevC.97.045807/fulltext

Reference25 articles.

1. Thesprocess: Nuclear physics, stellar models, and observations

2. Reaction rates for thes-process neutron source22Ne+α

3. N22e(α,n)M25g: The Key Neutron Source in Massive Stars

4. Reaction rates of the s-process neutron sources Ne-22(alpha, n)Mg-25 and C-13(alpha, n)O-16

5. Helium burning of22Ne

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4. The resonances in the $$^{22}$$Ne+$$\alpha $$ fusion reactions;The European Physical Journal A;2023-01-30

5. <sup>22</sup>Ne(α, n)<sup>25</sup>Mg: The key neutron source in massive stars;Chinese Science Bulletin;2022-05-24

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