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The Beta-Delayed Proton and Gamma Decay of 27P for Nuclear Astrophysics
2013
Journal of Physics, Conference Series
The creation site of 26 Al is still under debate. It is thought to be produced in hydrogen burning and in explosive helium burning in novae and supernovae, and possibly also in the H-burning in outer shells of red giant stars. Also, the reactions for its creation or destruction are not completely known. When 26 Al is created in novae, the reaction chain is: 24 M g(p, γ) 25 Al(β + ν) 25 M g(p, γ) 26 Al, but this chain can be by-passed by another chain, 25 Al(p, γ) 26 Si(p, γ) 27 P and it can
doi:10.1088/1742-6596/420/1/012152
fatcat:6fxtktbjvfcoxg4rwlbxsnyi2e