Constraining the 22Ne(α,γ)26Mg and 22Ne(α,n)25Mg reaction rates using sub-Coulomb α-transfer reactions
The 22Ne(α,γ)26Mg and 22Ne(α,n)25Mg reactions play an important role in astrophysics because they have significant influence on the neutron flux during the weak branch of the s-process. We constrain the astrophysical rates for these reactions by measuring partial α-widths of resonances in 26Mg locat...
Main Authors: | H. Jayatissa, G.V. Rogachev, V.Z. Goldberg, E. Koshchiy, G. Christian, J. Hooker, S. Ota, B.T. Roeder, A. Saastamoinen, O. Trippella, S. Upadhyayula, E. Uberseder |
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Format: | Article |
Language: | English |
Published: |
Elsevier
2020-03-01
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Series: | Physics Letters B |
Online Access: | http://www.sciencedirect.com/science/article/pii/S037026932030071X |
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