6533b7d2fe1ef96bd125f5d9

RESEARCH PRODUCT

Ab initio limits of atomic nuclei

J. D. HoltJ. D. HoltS. R. StrobergS. R. StrobergAchim SchwenkAchim SchwenkJ. SimonisJ. Simonis

subject

ProtonNuclear TheoryNuclear TheoryAb initioGeneral Physics and Astronomychemistry.chemical_elementFOS: Physical sciences01 natural sciences7. Clean energyNuclear Theory (nucl-th)0103 physical sciencesPhysics::Atomic and Molecular ClustersNeutronNuclear drip linePhysics::Atomic PhysicsNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentNuclear ExperimentHeliumPhysicsIsotopeStarke Wechselwirkung und exotische Kerne – Abteilung BlaumRenormalization groupchemistryAtomic nucleusAtomic physics

description

We predict the limits of existence of atomic nuclei, the proton and neutron drip lines, from the light through medium-mass regions. Starting from a chiral two- and three-nucleon interaction with good saturation properties, we use the valence-space in-medium similarity renormalization group to calculate ground-state and separation energies from helium to iron, nearly 700 isotopes in total. We use the available experimental data to quantify the theoretical uncertainties for our ab initio calculations towards the drip lines. Where the drip lines are known experimentally, our predictions are consistent within the estimated uncertainty. For the neutron-rich sodium to chromium isotopes, we provide predictions to be tested at rare-isotope beam facilities.

https://dx.doi.org/10.48550/arxiv.1905.10475