Nuclear Mass Measurements Map the Structure of Atomic Nuclei and Accreting Neutron Stars
Z. Meisel🇺🇸 · S. George🇩🇪 · S. Ahn🇺🇸 · D. Bazin🇺🇸 · B. A. Brown🇺🇸 · J. Browne🇺🇸 · J. F. Carpino · H. Chung · R. H. Cyburt · A. Estradé🇺🇸 · M. Famiano🇺🇸 · A. Gade🇺🇸 and 19 other authors
We present mass excesses (ME) of neutron-rich isotopes of Ar through Fe, obtained via TOF- mass spectrometry at the National Superconducting Cyclotron Laboratory. Our new results have significantly reduced systematic uncertainties relative to a prior analysis, enabling the first determination of ME for , , , , and . Our results show the subshell weaken at Sc and vanish at Ti, along with the absence of an subshell at Mn. This leads to a cooler accreted neutron star crust, highlighting the connection between the structure of nuclei and neutron stars.