S-factor of 14N(α,γ)18F reaction at low-energies
The astrophysical S-factor of the 14N(α,γ)18F reaction has been studied at range of bombarding energy 1–1.30 MeV. The 14N(α,γ)18F process is important in low energy astrophysics so that a possible source of energy in massive stars which have spent their hydrogen cycle. Using the Wood-saxon potential...
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| Format: | Article |
| Language: | English |
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Elsevier
2018-06-01
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| Series: | Results in Physics |
| Online Access: | http://www.sciencedirect.com/science/article/pii/S2211379718303905 |