Abstract

The neutron total cross sections σtotσ_{tot} of 16,18^{16,18}O, 58,64^{58,64}Ni, 103^{103}Rh, and 112,124^{112,124}Sn have been measured at the Los Alamos Neutron Science Center (LANSCE) from low to intermediate energies (3 ≤Elab≤\leq E_{lab} \leq 450 MeV) by leveraging waveform-digitizer technology. The σtotσ_{tot} relative differences between isotopes are presented, revealing additional information about the isovector components needed for an accurate optical-model description away from stability. Digitizer-enabled σtotσ_{tot}-measurement techniques are discussed and a series of uncertainty-quantified dispersive optical model (DOM) analyses using these new data is presented, validating the use of the DOM for modeling light systems (16,18^{16,18}O) and systems with open neutron shells (58,64^{58,64}Ni and 112,124^{112,124}Sn). The valence-nucleon spectroscopic factors extracted for each isotope reaffirm the usefulness of high-energy proton reaction cross sections for characterizing depletion from the mean-field expectation.

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