The Nucleus Resolved, Ch Neutrons: the reagent with no barrier
Problem
Stable 86Sr (N=48) and 88Sr (N=50, a closed neutron shell) both capture neutrons in a stellar neutron flux at kBT=30keV. Neutron capture on 86Sr forms 87Sr with neutron separation energy Sn(87Sr)=8.43MeV; capture on 88Sr forms 89Sr with Sn(89Sr)=6.36MeV. Take the level-density parameter of each compound nucleus as ald=A/8MeV−1 and the level density as ρlev(U)∝exp(2aldU).
((a)) State, with a one-sentence reason, which target is predicted to have the larger 30keV capture cross section.
((b)) Estimate the ratio of the two capture cross sections from the level densities at Sn.