16O(p,α0)13N cross-section measurements
References (11)
- et al.
Phys. Lett.
(1972) Nucl. Phys.
(1970)- et al.
Nucl. Phys.
(1961) Nucl. Phys.
(1971)- et al.
Phys. Rev.
(1964)
There are more references available in the full text version of this article.
Cited by (12)
Possible solution to the triple alpha fine-tuning problem: Spallation reactions during planet formation
2022, Astroparticle PhysicsProduction yields at the distal fall-off of the β<sup>+</sup> emitters <sup>11</sup>C and <sup>13</sup>N for in-vivo range verification in proton therapy
2022, Radiation Physics and ChemistryCitation Excerpt :In this case, the evaluation is based in ten of the fourteen data sets available up to 35 MeV. The evaluation included the data of Whitehead and Foster (1958), Furukawa et al. (1960), Hille et al. (1961), Maxson (1961), Dangle et al. (1964), McCamis et al. (1973), Nero and Howard (1973), Gruhle and Kober (1977), Sajjad et al. (1986) and Kitwanga et al. (1989). The deviations of the selected data from the evaluation are on average about 19%.
Investigation of (α, p) reactions using a radioactive beam
1999, Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated EquipmentAnalysis of oxygen by charged particle bombardment
1992, Nuclear Inst. and Methods in Physics Research, BThe reactions <sup>16</sup>O(p, α), <sup>20</sup>Ne(p, α) and <sup>24</sup>Mg(p, α)
1977, Nuclear Physics, Section A
- †††
Work supported in part by the National Science Foundation [GP-28027].
- †
Present address: Princeton university, Princeton, New Jersey 08540.
- ††
Oresent address: Trinity College, Hartford, Connecticut 06106.
Copyright © 1973 Published by Elsevier B.V.