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

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