The ²⁶Mg(p,n)²⁶Al and ²³Na(α,n)²⁶Al Reactions

<p>Cross sections for the <sup>26</sup>Mg (p ,n)<sup>26</sup>AI reaction have been measured from threshold at E<sub>p</sub> = 4.988 MeV to E<sub>p</sub> = 5.820 MeV. Cross sections for the <sup>23</sup>Na (α,n)<sup>26</sup>...

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Bibliographic Details
Main Author: Skelton, Robert Thomas
Format: Others
Language:en
Published: 1985
Online Access:https://thesis.library.caltech.edu/11377/2/Skelton_RT_1985.pdf
Skelton, Robert Thomas (1985) The ²⁶Mg(p,n)²⁶Al and ²³Na(α,n)²⁶Al Reactions. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/z85k-2k90. https://resolver.caltech.edu/CaltechTHESIS:02012019-083752423 <https://resolver.caltech.edu/CaltechTHESIS:02012019-083752423>
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Summary:<p>Cross sections for the <sup>26</sup>Mg (p ,n)<sup>26</sup>AI reaction have been measured from threshold at E<sub>p</sub> = 4.988 MeV to E<sub>p</sub> = 5.820 MeV. Cross sections for the <sup>23</sup>Na (α,n)<sup>26</sup>AI reaction have been measured from threshold at E<sub>α</sub> = 3.483 MeV to E<sub>α</sub> = 4.597 MeV. In each case separate measurements have been to the ground state and to the first and second excited states of <sup>26</sup>AI. Cross sections for the inverse reactions have been calculated and reaction rate factors relating to the destruction of <sup>26</sup>AI in a supernova environment have been determined. Astrophysical implications relating to the observation of live and extinct <sup>26</sup>AI are discussed. Excitation functions for several additional exit channels for the <sup>26</sup>Mg + p and <sup>26</sup>Na + α reactions are reported.</p>