New inverse-kinematics measurements of spectroscopic factors in 57Cu/57Ni update the 56Ni(p,γ)57Cu reaction rate for explosive astrophysical burning.
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Single-particle shell strengths near the doubly magic nucleus $^{56}$Ni and the $^{56}$Ni(p,$\gamma$)$^{57}$Cu reaction rate in explosive astrophysical burning
New inverse-kinematics measurements of spectroscopic factors in 57Cu/57Ni update the 56Ni(p,γ)57Cu reaction rate for explosive astrophysical burning.