Mean field approaches for hypernuclei and current experimental data
arXiv:1611.03661 · doi:10.1103/PhysRevC.94.064319
Abstract
Motivated by the recently observed hypernucleus (Kiso event) C (N), we identify the state of this system theoretically within the framework of the relativistic-mean-field and Skyrme-Hartree-Fock models. The interactions are constructed to reproduce the two possibly observed removal energies, MeV or MeV. The present result is preferable to be , corresponding to the latter value.
8 pages, 3 figures, 1 table
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- Strangeness and resonance in compact stars with relativistic-mean-field models
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- Massive neutron stars and -hypernuclei in relativistic mean field models
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- Searching for single-particle resonances with the Green's function method
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- Charmed hypernuclei within density-dependent relativistic mean-field theory
- Effects of mixing in the decay of hypernuclei
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- Ground-state properties of light kaonic nuclei signaling symmetry energy at high densities