Low-energy measurement of the 25Mg(α,n)28Si reaction via neutron spectroscopy

Published: March 2026 Wiescher

Lead Author(s): Shahina

During core helium and carbon burning in massive stars, neutrons are produced by the 22Ne(α,n)25Mg reaction. However, the rates of neutron poison and recycling reactions must also be well determined. One such critical reaction is 25Mg(α,n)28Si, where past attempts to measure the cross section using neutron moderator counters have been greatly hindered by lower-Z background reactions. In this work, neutron spectroscopy with deuterated liquid scintillator detectors has been used to improve the background discrimination. Learn more

Publication: Low energy measurement of the 25Mg(α,n)28Si reaction via neutron spectroscopy