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4. 26gAl(p,γ)27Si at Stellar Temperatures

26gAl(p,γ)27Si at Stellar Temperatures

Published: May 2015 Bardayan

Lead Author(s): S.D. Pain

The rate of the ^26gAl(p,γ)²⁷Si reaction at stellar temperatures determines, in part, the contributions that various stellar events make to the observed ^26gAl g-ray flux from the Galactic center.  The rate has been constrained via an ^26gAl(d,p)²⁷Al study at the ORNL Holifield Radioactive Ion Beam Facility. Learn more

Publication: Constraint of the Astrophysical ^26gAl(p,γ)²⁷Si Destruction Rate at Stellar Temperatures