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Ab Initio Computation of Charge Densities for Sn and Xe Isotopes

2020/02/29 by P. Arthuis, C. Barbieri, Matteo Vorabbi +3
Physics and Astronomy · #Ab initio #Ab initio quantum chemistry methods #Astronomical and nuclear sciences #Atomic physics #Charge (physics) #Charge density #Computation #Computer science #Isotope #Materials science #Molecule #Nuclear Physics and Applications #Nuclear physics #Nuclear physics research studies #Physics #Quantum mechanics #nucl-ex #nucl-th

paper · pdf · doi:10.1103/physrevlett.125.182501

published as Phys. Rev. Lett. 125, 182501 (2020) · 6 pages, 4 figures and 2 tables

openalex created_date 2020/02/14 · arxiv created 2020/07/09 · openalex publication_date 2020/10/28 · arxiv updated 2020/11/04 · openalex updated_date 2026/08/06

Abstract

We present the first ab initio calculations for open-shell nuclei past the tin 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 obtain meaningful predictions and that the NNLOsat chiral interaction predicts radii and charge density distributions close to the experiment. We then make a new prediction for 100Sn. This paves the way for ab initio studies of exotic charge density distributions at the limit of the present ab initio mass domain, where experimental data is becoming available. The present study closes the gap between the largest isotopes reachable by ab initio methods and the smallest exotic nuclei accessible to electron scattering experiments.

Citations