The effect of three-body nucleon-nucleon interaction on the ground state binding energy of the light nuclei
arXiv:2502.16323 · doi:10.1016/j.nuclphysa.2025.123056
Abstract
We calculate the ground state binding energies of the light nuclei such as 4He, 6Li, 12C and 14N by considering the effect of three-body nucleon-nucleon interaction. We use the effective twobody potential obtained from the lowest order constrained variational (LOCV) calculations of the nuclear matter for the Reid68, AV14, UV14, and AV18 nuclear potentials in different channels. To calculate the ground state binding energy, we implement the local density approximation by using the harmonic oscillator wave functions while the effect of three-body interaction is considered by employing the UIX potential. We compare the obtained two-body ground state binding energy with the energy related to the three-body effect. We also compare the obtained values with the experimental data and also work of others, and show that the results are relatively acceptable. We compute the root mean-square radius Rrms of the above nuclei for the Reid68, AV14, UV14, and AV18 potentials and compare the results with the experiment. We also obtain the contribution of different channels by matching to the experimental values of the quadrupole moments and magnetic dipole moments. Furthermore, we calculate the three-body cluster energy of the above nuclei and compare the results with that of nuclear matter. According to the obtained results, we see that the three-body cluster energy contribution is small. For example, for 4He nuclide, this value is 0.079 MeV with the Reid68 potential.
arXiv comment12 pages, 8 figures, 4 tables (Nuclear Physics A (2025) accepted for publication)
References in corpus (14)
- An accurate nucleon-nucleon potential with charge-independence breaking
- Quantum Monte Carlo calculations of nuclei with A \leq 7
- Quantum Monte Carlo methods for nuclear physics
- Quantum Monte Carlo Calculations of Nuclei
- Modern nuclear force predictions for the alpha particle
- Nuclear Structure based on Correlated Realistic Nucleon-Nucleon Potentials
- Properties of nuclei up to using local chiral interactions
- Spin Polarized Asymmetric Nuclear Matter and Neutron Star Matter Within the Lowest Order Constrained Variational Method
- Nuclear Structure Calculations and Modern Nucleon-Nucleon Potentials
- Magnetized hot neutron matter: lowest order constrained variational calculations
- Influence of spin polarizability on liquid gas phase transition in the nuclear matter
- Hot magnetized nuclear matter: Thermodynamic and Saturation Properties
- Nuclear matter calculations with the phenomenological three-nucleon interaction
- Neutron star calculations with the phenomenological three-nucleon force