Isoscalar Hamiltonians for light atomic nuclei

Abstract

The charge-dependent realistic nuclear Hamiltonian for a nucleus, composed of neutrons and protons, can be successfully approximated by a charge-independent one. The parameters of such a Hamiltonian, i.e., the nucleon mass and the NN potential, depend upon the mass number A, charge Z and isospin quantum number T of state of the studied nucleus.

REVTeX, 22 pages, 3 eps figures, to appear in PRC

References in corpus (2)

• Quantum Monte Carlo calculations of nuclei with A \leq 7
• Large-basis shell-model calculations for p-shell nuclei

Cited by in corpus (14)

• Unified ab initio approaches to nuclear structure and reactions
• Uncertainty analysis and order-by-order optimization of chiral nuclear interactions
• Quantum Monte Carlo calculations of electromagnetic moments and transitions in A <= 9 nuclei with meson-exchange currents derived from chiral effective field theory
• Spectra and binding energy predictions of chiral interactions for 7Li
• Rigorous constraints on three-nucleon forces in chiral effective field theory from fast and accurate calculations of few-body observables
• Quantum Monte Carlo calculations of electroweak transition matrix elements in A = 6,7 nuclei
• Ab initio many-body calculations of nucleon-4He scattering with three-nucleon forces
• Quantum Monte Carlo calculations of electromagnetic transitions in 8Be with meson-exchange currents derived from chiral effective field theory
• Charge-symmetry breaking forces and isospin mixing in 8Be
• Jacobi no-core shell model for p-shell nuclei
• Quadrupole moments and proton-neutron structure in p-shell mirror nuclei
• Intrinsic operators for the translationally-invariant many-body problem
• Perturbative $\chi$EFT calculations of the deuteron and triton up to N${}^2$LO
• Challenges for Modeling Nuclear Structure: Are the Proton and Neutron Masses and A-body Interactions Relevant?