Cross sections of the 21Ne(α, n)24Mg and 22Ne(α, n)25Mg reactions at low energies of astrophysical interest☆
References (14)
Nucl. Phys.
(1969)Nucl. Phys.
(1965)- et al.
Rev. Mod. Phys.
(1957) Astronom. J.
(1960)- et al.
Phys. Rev.
(1973) - et al.
Astrophys. J.
(1957) - et al.
Astrophys. J.
(1972)
There are more references available in the full text version of this article.
Cited by (17)
Charged particle reaction cross sections and nucleosynthesis
1982, Physics ReportsTotal cross-section measurements for the production of nuclear gamma rays from light nuclei by low-energy deuterons
1982, Nuclear Physics, Section ACompetition cusps in (α, γ) reactions
1979, Nuclear Physics, Section ARemeasurement of the low-energy cross section for the <sup>15</sup>N(p, α<inf>0</inf>)<sup>12</sup>C reaction
1979, Nuclear Physics, Section AEnergy levels of A = 21-44 nuclei (VI)
1978, Nuclear Physics, Section A
- ☆
Supported in part by the National Science Foundation [GP-28027].
- ††
Present address: Physics Department, Queens's University, Kingston, Ontario, Canada.
- †††
Present address: Physics Department, Tel Aviv University, Ramat Aviv, Tel Aviv, Israel.
Copyright © 1974 Published by Elsevier B.V.