Longland, RIliadis, CKarakas, Amanda2015-12-100556-2813http://hdl.handle.net/1885/68040The 22Ne(α,n)25Mg reaction is an important source of neutrons for the s-process. In massive stars responsible for the weak component of the s-process, 22Ne(α,n)25Mg is the dominant source of neutrons, both during core helium burning and in carbon-shell201210.1103/PhysRevC.85.0658092015-12-10