Constraining the 22Ne(α,γ)26Mg and 22Ne(α,n)25Mg reaction rates using sub-Coulomb α-transfer reactions-Reference-Cited by-同舟云学术

Constraining the 22Ne(α,γ)26Mg and 22Ne(α,n)25Mg reaction rates using sub-Coulomb α-transfer reactions

Published:2020-03 Issue: Volume:802 Page:135267
ISSN:0370-2693
Container-title:Physics Letters B
language:en
Short-container-title:Physics Letters B

Author:

Jayatissa H.,Rogachev G.V.^ORCID,Goldberg V.Z.,Koshchiy E.,Christian G.,Hooker J.,Ota S.^ORCID,Roeder B.T.,Saastamoinen A.,Trippella O.,Upadhyayula S.^ORCID,Uberseder E.

Funder

National Nuclear Security Administration

U.S. Department of Energy

Publisher

Elsevier BV

Subject

Nuclear and High Energy Physics

Reference36 articles.

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

2. Neutron-Capture Elements in the Early Galaxy

3. The astrophysical implications of low-energy resonances in 22Ne + α

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

5. Study of the 22Ne(α, n)25Mg reaction: a possible source of stellar neutronS

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