Electron-scattering form factors for 6Li in the ab initio symmetry-guided framework
arXiv:1502.03066 · doi:10.1103/PhysRevC.91.024326
Abstract
We present an ab initio symmetry-adapted no-core shell-model description for Li. We study the structure of the ground state of Li and the impact of the symmetry-guided space selection on the charge density components for this state in momentum space, including the effect of higher shells. We accomplish this by investigating the electron scattering charge form factor for momentum transfers up to fm. We demonstrate that this symmetry-adapted framework can achieve significantly reduced dimensions for equivalent large shell-model spaces while retaining the accuracy of the form factor for any momentum transfer. These new results confirm the previous outcomes for selected spectroscopy observables in light nuclei, such as binding energies, excitation energies, electromagnetic moments, E2 and M1 reduced transition probabilities, as well as point-nucleon matter rms radii.
arXiv comment10 pages, 7 figures; accepted to Physical Review C
References in corpus (25)
- An accurate nucleon-nucleon potential with charge-independence breaking
- Accurate Charge-Dependent Nucleon-Nucleon Potential at Fourth Order of Chiral Perturbation Theory
- Quantum Monte Carlo calculations of nuclei with A \leq 7
- Quantum Monte Carlo Calculations of Nuclei
- Properties of C in the {\it ab initio} nuclear shell-model
- Ab initio calculation of the Hoyle state
- An optimized chiral nucleon-nucleon interaction at next-to-next-to-leading order
- Structure and rotations of the Hoyle state
- Evolution of Nuclear Spectra with Nuclear Forces
- Similarity-Transformed Chiral NN+3N Interactions for the Ab Initio Description of 12-C and 16-O
- Ab Initio Many-Body Calculations of n-3H, n-4He, p-{3,4}He, and n-10Be Scattering
- Many-body nuclear Hamiltonian: Ab exitu approach
- Origin of the anomalous long lifetime of 14C
- Medium-mass nuclei from chiral nucleon-nucleon interactions
- Collective Modes in Light Nuclei from First Principles
- Convergence in the no-core shell model with low-momentum two-nucleon interactions
- Evidence for Symplectic Symmetry in Ab Initio No-Core Shell Model Results for Light Nuclei
- SU(3) quasi-dynamical symmetry as an organizational mechanism for generating nuclear rotational motions
- Lithium isotopes within the ab intio no-core full configuration approach
- Ab initio nuclear structure simulations: the speculative F nucleus
- Microscopic calculation of 6Li elastic and transition form factors
- Neutrino-12C scattering in the ab initio shell model with a realistic three-body interaction
- Structure of A = 7 - 8 nuclei with two- plus three-nucleon interactions from chiral effective field theory
- Quasi-SU(3) truncation scheme for even-even sd-shell nuclei
- Structure of the Particle-Hole Amplitudes in No-core Shell Model Wave Functions
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- Symmetry-guided large-scale shell-model theory
- Symmetry restoration in mean-field approaches
- From bound states to the continuum
- Angular-momentum projection in coupled-cluster theory: structure of Mg
- Nuclear Dynamics and Reactions in the Ab Initio Symmetry-Adapted Framework
- Ab initio Folding Potentials for Nucleon-Nucleus Scattering based on NCSM One-Body Densities
- Large-scale exact diagonalizations reveal low-momentum scales of nuclei
- Efficacy of the SU(3) scheme for ab initio large-scale calculations beyond the lightest nuclei
- Emergent symplectic symmetry in atomic nuclei: Ab initio symmetry-adapted no-core shell model
- Emergent Sp(3,R) dynamical symmetry in the nuclear many-body system from an ab initio description
- Benchmark calculations of electromagnetic sum rules with a symmetry-adapted basis and hyperspherical harmonics
- Ab initio Translationally Invariant Nonlocal One-body Densities from No-core Shell-model Theory
- Efficacy of the symmetry-adapted basis for ab initio nucleon-nucleus interactions for light- and intermediate-mass nuclei
- Ab initio single-neutron spectroscopic overlaps in lithium isotopes
- Ab Initio No Core Shell Model with Leadership-Class Supercomputers