Direct measurement of the low-energy resonances in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Ne</mml:mi><mml:mprescripts /><mml:none /><mml:mn>22</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><mml:mi>α</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi>Mg</mml:mi><mml:mprescripts /><mml:none /><mml:mn>26</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> reaction-Reference-Cited by-同舟云学术

Direct measurement of the low-energy resonances in Ne22(α,γ)Mg26 reaction

Published:2022-08-22 Issue:2 Volume:106 Page:
ISSN:2469-9985
Container-title:Physical Review C
language:en
Short-container-title:Phys. Rev. C

Author:

Shahina ^ORCID,Görres J.,Robertson D.^ORCID,Couder M.^ORCID,Gomez O.^ORCID,Gula A.,Hanhardt M.^ORCID,Kadlecek T.,Kelmar R.^ORCID,Scholz P.^ORCID,Simon A.^ORCID,Stech E.,Strieder F.^ORCID,Wiescher M.^ORCID

Funder

National Science Foundation

University of Notre Dame

Sanford Underground Research Facility

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevC.106.025805/fulltext

Reference28 articles.

1. Cauldrons in the Cosmos

2. The branchings of the main s-process: their sensitivity to α-induced reactions on 13C and 22Ne and to the uncertainties of the nuclear network

3. Reaction rates for O-18(alpha, gamma)Ne-22, Ne-22(alpha, gamma)Mg-26, and Ne-22(alpha, n)Mg-25 in stellar helium burning and s-process nucleosynthesis in massive stars

4. Probing astrophysically important states in theMg26nucleus to study neutron sources for thesprocess

5. Helium burning of22Ne

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