Effects of finite nucleon size, vacuum polarization, and electromagnetic spin-orbit interaction on nuclear binding energies and radii in spherical nuclei
Abstract:The finite-light-speed correction to the Coulomb interaction called the Breit correction is discussed with Skyrme Hartree-Fock calculations. It is found that the correction to the total energy is about 800 keV for 208 Pb, while proton and neutron radii do not change significantly. Effects of the Breit correction are also compared to the correction due to the vacuum polarization. It is shown that the two contributions to the total energy are comparable in light nuclei, but the latter dominates in heavy nuclei. … Show more
In this suppelemental material, we show results for 16 O, 40 Ca, and 48 Ni, together with those for 48 Ca and 208 Pb. We also discuss the effects of the Coulomb interaction.
In this suppelemental material, we show results for 16 O, 40 Ca, and 48 Ni, together with those for 48 Ca and 208 Pb. We also discuss the effects of the Coulomb interaction.
“…An additional contribution may come from the vacuum polarization effect [79,83,84]. The effect to r 2 ch is extracted as the difference of r 2 ch calculated with and without the vacuum polarization.…”
Section: A Derivation Of Master Equationmentioning
confidence: 99%
“…The former changes ρp and accordingly, ρ ch , while the latter does not change any density distribution, but single-particle energies of electrons change. Here, we discuss the former [79,83,84]. The latter is usually discussed in the context of the laser spectroscopy [85,86].…”
Section: A Derivation Of Master Equationmentioning
confidence: 99%
“…The Skyrme Hartree-Fock calculation [91] is performed under the assumption of the spherical symmetry using a calculation code named skyrme_rpa [92]. The electric form factors of nucleons are considered selfconsistently [79].…”
Section: B Benchmark Calculationmentioning
confidence: 99%
“…To extract r 2 n from r 2 ch and r 4 ch , we will show that the key issue is how to accurately determine r 4 p . In this paper, we analyze the corresponding sensitivity by using one of the state-of-the-art Skyrme Hartree-Fock calculations that we developed in a series of works [77][78][79], where the finite-size effects of nucleons are implemented to the self-consistent steps of the calculation.…”
A method to extract the neutron-skin thickness of atomic nuclei from the second and fourth moments of the charge density distribution is discussed. To reduce the error in the estimation of the neutron root-mean-square radius due to small effects like the magnetic form factors of nucleons, two neighbouring even-even isotopes are used. It is found that uncertainty of the neutron radius strongly depends on the accuracy of estimation of the fourth moment of the proton density distribution. Consequently, extracting the neutron-skin thickness from the charge second and fourth moments is hardly feasible.
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