Analysis of Al25 energy levels observed in the Si28(p,α)Al25 reaction

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Transfer Reactions, Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments, 20&Lt, =A&Lt, =38, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, Transfer Reactions, Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments, 20<=A<=38, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages

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The level structure of Al25 has been studied at the ORNL Holifield Radioactive Ion Beam Facility by measuring the angular and energy distributions of α particles from the Si28(p,α)Al25 reaction. Proton beams (~10nA) at laboratory energies of 40 and 42 MeV were generated by the 25 MV tandem accelerator and bombarded a natural silicon target (50μg/cm2). Seventeen levels were observed and spins for several were constrained through a distorted-wave Born approximation analysis of the angular distributions.

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