Compressibility and equation of state of finite nuclei
arXiv:0706.1960 · doi:10.1103/PhysRevC.76.024316
Abstract
We present a new approach for calculating the nuclear equation of state and compressibility for finite nuclei using the density-constrained Hartree-Fock method.
arXiv comment4 pages, 3 figures
References in corpus (11)
- Isospin Asymmetry in Nuclei and Neutron Stars
- Reaction Dynamics with Exotic Beams
- Linear response theory in the continuum for deformed nuclei: Green's function vs. time-dependent Hartree-Fock with the absorbing-boundary condition
- 3-D unrestricted TDHF fusion calculations using the full Skyrme interaction
- Heavy-ion interaction potential deduced from density-constrained TDHF calculation
- On the nuclear symmetry energy and the neutron skin in neutron-rich nuclei
- From finite nuclei to the nuclear liquid drop: leptodermous expansion based on the self-consistent mean-field theory
- Time-Dependent Response Calculations of Nuclear Resonances
- Global properties of the Skyrme-force-induced nuclear symmetry energy
- Nuclear Giant Resonances and Linear Response
- Expansion and evaporation of hot nuclei: Comparison between semi-classical and quantal mean-field approaches