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Nuclear Symmetry Energy Effects on the Bulk Properties of Neutron-rich Finite Nuclei

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Nuclear Symmetry Energy Effects on the Bulk Properties of Neutron-rich Finite Nuclei (EN)
Moustakidis, Charalampos
Divaris, Manolis
info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
Theoretical (EN)
2020-04-17
We systematically study the effect of the nuclear symmetry energy in the basic properties of finite, neutron-rich, heavy nuclei where symmetry energy plays a dominant role. We employ a variational method, in the framework of the Thomas-Fermi approximation, to study the effect of the symmetry energy on the neutron skin thickness and symmetry energy coefficients of various nuclei. The isospin asymmetry function a(r) is directly related to the symmetry energy as a consequence of the variational principle. In addition to this, the Coulomb interaction is included in a self-consistent way. The energy density of the asymmetric nuclear matter that is used, has its origins in a momentum-dependent interaction. (EN)
symmetry energy (EN)
neutron-skin (EN)
neutron-rich nuclei (EN)
Annual Symposium of the Hellenic Nuclear Physics Society
English
Hellenic Nuclear Physics Society (HNPS) (EN)
2654-0088
2654-007X
Annual Symposium of the Hellenic Nuclear Physics Society; Τόμ. 27 (2019): HNPS2019; 91-94 (EL)
HNPS Advances in Nuclear Physics; Vol. 27 (2019): HNPS2019; 91-94 (EN)
Πνευματική ιδιοκτησία (c) 2020 Manolis Divaris, Charalampos Moustakidis (EL)
Hellenic Nuclear Physics Society
Annual Symposium of the Hellenic Nuclear Physics Society
Oral contributions



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