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Proton threshold states in /sup 26/Al and their role in astrophysics

Thesis/Dissertation ·
OSTI ID:5571355

The energy levels of /sup 26/Al between E/sub x/ = 6.3 and 6.5 MeV, corresponding to proton threshold energies in the /sup 25/Mg + p reaction from E/sub p/ = 0 to 200 keV, have been investigated using the reactions /sup 27/Al(/sup 3/He,..cap alpha..)/sup 26/Al and /sup 24/Mg(/sup 3/He,p)/sup 26/Al. Despite early work reporting a doublet at E/sub x/ 6346 keV and E/sub x/ = 6362 keV, most subsequent work reported a single state with conflicting spin and parity assignments. By measuring the spectroscopic factors of these states from the /sup 25/Mg(/sup 3/He,d)/sup 26/Al reaction, resonance strengths, omega..gamma.., of the proton threshold states in /sup 26/Al corresponding to the /sup 25/Mg(p,..gamma..)/sup 26/Al reaction have been deduced. The limits on the branching ratios from these states to the ground state of /sup 26/Al have been obtained by using the reaction /sup 27/Al(/sup 3/He,..cap alpha gamma..)/sup 26/Al. Finally by combining the results of the above experiments, stellar reaction rates of the /sup 25/Mg(p,..gamma..)/sup 26/Al reaction have been calculated. The results conclude that the production rate of /sup 26/Al in stellar environments from the reaction /sup 25/Mg(p,..gamma..)/sup 26/Al is substantially higher than what was calculated from other work.

Research Organization:
Ohio State Univ., Columbus (USA)
OSTI ID:
5571355
Country of Publication:
United States
Language:
English

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