Empirical information on nuclear matter fourth-order symmetry energy from an extended nuclear mass formula
arXiv:1705.05122 · doi:10.1016/j.physletb.2017.08.007
Abstract
We establish a relation between the equation of state (EOS) of nuclear matter and the fourth-order symmetry energy of finite nuclei in a semi-empirical nuclear mass formula by self-consistently considering the bulk, surface and Coulomb contributions to the nuclear mass. Such a relation allows us to extract information on nuclear matter fourth-order symmetry energy at normal nuclear density from analyzing nuclear mass data. Based on the recent precise extraction of via the double difference of the "experimental" symmetry energy extracted from nuclear masses, for the first time, we estimate a value of MeV. Such a value of is significantly larger than the predictions from mean-field models and thus suggests the importance of considering the effects of beyond the mean-field approximation in nuclear matter calculations.
7 pages, 1 figure. Presentation improved and discussions added. Accepted version to appear in PLB
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Cited by in corpus (9)
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- Nuclear fourth-order symmetry energy and its effects on neutron star properties in the relativistic Hartree-Fock theory
- Nuclear matter fourth-order symmetry energy in non-relativistic mean-field models
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- High-order isospin-dependent surface tension contribution to the fourth-order symmetry energy of finite nuclei