On April 2, Scott Carmichael successfully defended his Ph.D. thesis on “An experimentally constrained reaction rate fo57Ni(p,γ)58Cu” at the University of Notre Dame. Scott constrained the amount of observable 44Ti produced in supernovae by understanding the 57Ni(p,γ)58Cu reaction rate that had never previously been experimentally determined, combining two measurements. One used GODDESS for a high-resolution study of 58Cu through gamma-ray spectroscopy, and the other used high-resolution charged-particle spectroscopy using the newly-installed Enge spectrometer at the Notre Dame (previously ORNL). Scott worked closely with Prof. Rebecca Surman on nucleosynthesis calculations showing the dramatic reduction in uncertainties related to 44Ti nucleosynthesis – a major target of gamma-ray astronomy.

