Time-of-flight mass measurements of neutron-rich chromium isotopes up to N=40 and implications for the accreted neutron star crust We present the mass excesses of 59−64 Cr, obtained from recent time-of-flight nuclear mass measurements at the National Superconducting Cyclotron Laboratory at Michigan State University. The mass of 64 Cr was determined for the first time with an atomic mass excess of −33.48(44) MeV. We find a significantly different two-neutron separation energy S2n trend for neutron-rich isotopes of chromium, removing the previously observed enhancement in binding at N = 38. Additionally, we extend the S2n trend for chromium to N = 40, revealing behavior consistent with the previously identified island of inversion in this region. We compare our results to state-of-the-art shell-model calculations performed with a modified Lenzi-Nowacki-Poves-Sieja interaction in the f p-shell, including the g 9/2 and d 5/2 orbits for the neutron valence space. We employ our result for the mass of 64 Cr in accreted neutron star crust network calculations and find a reduction in the strength and depth of electron capture heating from the A = 64 isobaric chain, resulting in a cooler than expected accreted neutron star crust. This reduced heating is found to be due to the over 1 MeV reduction in binding for 64 Cr with respect to values from commonly used global mass models.
I. INTRODUCTION
22The evolution of nuclear structure away from the val- production of more neutron-rich nuclides of interest were 106 used alternately, keeping Bρ of the A1900 and S800 fixed.
107Fragments were transmitted through the A1900 fragment spectively.
124The relationship between TOF and nuclear rest mass 125 m rest is obtained from the equation of motion for a 126 charged massive particle through a magnetic system.
127Equating the two counteracting forces, the Lorentz force 128 F L and the centripetal force F c , results in the followingwhere the Lorentz factor γ is a function of velocity v, the Bρ-corrected data were fit with a Gaussian distribu-158 tion in order to determine a mean TOF for each nuclide.
159The relationship between mass over charge m rest /q and
160TOF was fit to the data of reference nuclides in order to