Descriptions of Carbon isotopes within relativistic Hartree-Fock-Bogoliubov theory
arXiv:1210.5388 · doi:10.1103/PhysRevC.87.034311
Abstract
Within the relativistic Hartree-Fock-Bogoliubov (RHFB) theory, the structure properties of Carbon isotopes are systematically studied. In order to reproduce the experiment data, we take the finite-range Gogny D1S with a strength factor as the pairing force. The self-consistent RHFB calculations with density-dependent meson-nucleon couplings indicate the single-neutron halo structures in both C and C, whereas the two-neutron halo in C is not well supported. It is also found that close to the neutron drip line there exists distinct odd-even staggering on neutron radii, which is tightly related with the blocking effects and correspondingly the blocking effect plays a significant role in halo formation.
8 pages, 5 figures, 5 table
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Cited by in corpus (15)
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- Angular momentum projection in the deformed relativistic Hartree-Bogoliubov theory in continuum
- Nuclear fourth-order symmetry energy and its effects on neutron star properties in the relativistic Hartree-Fock theory
- Relativistic Hartree-Fock-Bogoliubov model for axially deformed nuclei
- Isospin coupling-channel decomposition of nuclear symmetry energy in covariant density functional theory
- Odd-even staggerings on nuclear binding energy described by the covariant density functional theory
- Nuclear matter distributions in the neutron-rich carbon isotopes C from intermediate-energy proton elastic scattering in inverse kinematics
- Critical parameters of liquid-gas phase transition in thermal symmetric and asymmetric nuclear matter
- Continuum Skyrme-Hartree-Fock-Bogoliubov theory with Green's function method for odd- nuclei
- Quenched Λ spin-orbit splitting by relativistic Fock diagram in single-Λ hypernuclei
- Unified mechanism behind the even-parity ground state and neutron halo of Be
- Moments of inertia of neutron stars in relativistic mean field theory: the role of the isovector scalar channel
- Impact of pion tensor force on alpha clustering in Ne