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We present the first ab initio calculations for open-shell nuclei past thetin isotopic line, focusing on Xe isotopes as well as doubly-magic Sn isotopes.We show that, even for moderately hard interactions, it is possible to obtainmeaningful predictions and that the NNLOsat chiral interaction predicts radiiand charge density distributions close to the experiment. We then make a newprediction for ${}^{100}$Sn. This paves the way for ab initio studies of exoticcharge density distributions at the limit of the present ab initio mass domain,where experimental data is becoming available. The present study closes the gapbetween the largest isotopes reachable by ab initio methods and the smallestexotic nuclei accessible to electron scattering experiments.

Ab initio computation of charge densities for Sn and Xe isotopes