Nuclear Physics Experiment Helps Identify Conditions for a New Astrophysical Process

Credit: Facility for Rare Isotope Beams

A simulation of a rapidly accreting white dwarf showing a proposed site for the intermediate (i) process and the Summing NaI (SuN) detector. The research studied the 139Ba+n reaction, constrained by the beta decay of 140Cs into 140Ba.

« Nuclear Physics Experiment Helps Identify Conditions for a New Astrophysical Process

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