Repulsive potentials in dense neutron star matter and binding energy of in hypernuclei
arXiv:2306.17452 · doi:10.1103/PhysRevC.108.065803
Abstract
The repulsive three-body force between the lambda () hyperon and medium nucleons is a key element in solving the hyperon puzzle in neutron stars. We investigate the binding energies of hyperon in hypernuclei to verify the repulsive potentials from the chiral effective field theory (EFT) employing the Skyrme Hartree-Fock method. We find that the EFT potential with the three-body forces reproduces the existing hypernuclear binding energy data, whereas the binding energies are overestimated without the three-body force. Additionally, we search for the parameter space of the potentials by varying the Taylor coefficients of the potential and the effective mass of at the saturation density. Our analysis demonstrates that the parameter region consistent with the binding energy data spans a wide range of the parameter space, including even more repulsive potentials than the EFT prediction. We confirm that these strong repulsive potentials suppress the presence of in the neutron star matter. We found that the potentials repulsive at high densities are favored when the depth of the potential at the saturation density, , is , while attractive ones are favored when . This suggests that the future high-resolution data of hypernuclei could rule out the scenario in which s appear through the precise determination of within the accuracy of .
15 pages, 11 figures, 3 tables, figures updated and extended, (Published in Physical Review C)
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