Neutron density distributions for atomic parity nonconservation experiments
arXiv:nucl-th/0004018 · doi:10.1103/PhysRevC.62.045502
Abstract
The neutron distributions of Cs, Ba, Yb and Pb isotopes are described in the framework of relativistic mean-field theory. The self-consistent ground state proton and neutron density distributions are calculated with the relativistic Hartree-Bogoliubov model. The binding energies, the proton and neutron radii, and the quadrupole deformations are compared with available experimental data, as well as with recent theoretical studies of the nuclear structure corrections to the weak charge in atomic parity nonconservation experiments.
16 pages, RevTex, 11 eps figs, submitted to Phys. Rev. C
References in corpus (5)
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- Ground-state properties of deformed proton emitters in the relativistic Hartree-Bogoliubov model
- Effects of Neutron Spatial Distributions on Atomic Parity Nonconservation in Cesium
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Cited by in corpus (16)
- Search for New Physics with Atoms and Molecules
- Violations of fundamental symmetries in atoms and tests of unification theories of elementary particles
- Neutron Radii in Mean-Field Models
- Relativistic Hartree-Bogoliubov model with density-dependent meson-nucleon couplings
- The Weak Charge of the Proton and New Physics
- New relativistic effective interaction for finite nuclei, infinite nuclear matter and neutron stars
- High accuracy calculation of 6s -> 7s parity nonconserving amplitude in Cs
- Correlated many-body treatment of Breit interaction with application to cesium atomic properties and parity violation
- Atomic Parity Non-Conservation, Neutron Radii, and Effective Field Theories of Nuclei
- High-precision determination of transition amplitudes of principal transitions in Cs from van der Waals coefficient C_6
- Dispelling the curse of the neutron skin in atomic parity violation
- Spin-Isospin Resonances and Neutron Skin of Nuclei
- Nuclear and Neutron Star Radii
- Dependence of atomic parity-violation effects on neutron skins and new physics
- Influence of the single-particle structure on the nuclear surface and the neutron skin
- Implications of nuclear interaction for nuclear structure and astrophysics within the relativistic mean-field model