β-decay Measurements Near the N=40 Island of Inversion to Quantify Cooling of Accreted Neutron Star Crusts
Abstract
Understanding the thermal structure of the outer crust of accreting neutron stars is important to interpret astronomical X-ray observations. Ground-state to ground-state β-decay transitions of neutron-rich nuclei comprising the crust enable Urca neutrino cooling processes that affect this thermal structure. Here we constrain the ground-state to ground-state transition strengths for the decays of 57Sc, 57Ti, and 59Ti based on experimental data. The data were obtained by combining total absorption γ-spectroscopy data from the SuN detection system with β-delayed neutron emission data from the NERO detection system at Michigan State University's National Superconducting Cyclotron Laboratory. We find ft=5.8+0.3-0.2 and ft=5.34+0.08-0.24 for the decays of 57Ti and 59Ti, respectively, and find no evidence for ground-state feeding in the decay of 57Sc. The results indicate weaker transitions than predicted by theory and indicated by previous measurements, resulting in reduced efficiency of neutrino cooling in accreted neutron star crusts in systems that exhibit X-ray superbursts.
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