The nuclear symmetry energy and the breaking of the isospin symmetry: how do they reconcile with each other?
arXiv:1803.09120 · doi:10.1103/PhysRevLett.120.202501
Abstract
We analyze and propose a solution to the apparent inconsistency between our current knowledge of the Equation of State of asymmetric nuclear matter, the energy of the Isobaric Analog State (IAS) in a heavy nucleus such as 208Pb, and the isospin symmetry breaking forces in the nuclear medium. This is achieved by performing state-of-the-art Hartree-Fock plus Random Phase Approximation calculations of the IAS that include all isospin symmetry breaking contributions. To this aim, we propose a new effective interaction that is successful in reproducing the IAS excitation energy without compromising other properties of finite nuclei.
Accepted for publication in Phys. Rev. Lett. Supplemental material available
References in corpus (6)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Origin of the heavy elements in binary neutron-star mergers from a gravitational wave event
- Nuclear symmetry energy probed by neutron skin thickness of nuclei
- Neutron skin of 208Pb, nuclear symmetry energy, and the parity radius experiment
- Giant Quadrupole Resonances in 208Pb, the nuclear symmetry energy and the neutron skin thickness
- A new Skyrme interaction with improved spin-isospin properties
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