{ "id": "nucl-th/9608005", "version": "v1", "published": "1996-08-02T15:44:37.000Z", "updated": "1996-08-02T15:44:37.000Z", "title": "Superheavy Nuclei in the Relativistic Mean Field Theory", "authors": [ "G. A. Lalazissis", "M. M. Sharma", "P. Ring", "Y. K. Gambhir" ], "comment": "29 pages Latex, 13 ps figures, to appear in Nucl. Phys. A", "journal": "Nucl.Phys. A608 (1996) 202-226", "doi": "10.1016/0375-9474(96)00273-4", "categories": [ "nucl-th" ], "abstract": "We have carried out a study of superheavy nuclei in the framework of the Relativistic Mean-Field theory. Relativistic Hartree-Bogoliubov (RHB) calculations have been performed for nuclei with large proton and neutron numbers. A finite-range pairing force of Gogny type has been used in the RHB calculations. The ground-state properties of very heavy nuclei with atomic numbers Z=100-114 and neutron numbers N=154-190 have been obtained. The results show that in addition to N=184 the neutron numbers N=160 and N=166 exhibit an extra stability as compared to their neighbors. For the case of protons the atomic number Z=106 is shown to demonstrate a closed-shell behavior in the region of well deformed nuclei about N=160. The proton number Z=114 also indicates a shell closure. Indications for a doubly magic character at Z=106 and N=160 are observed. Implications of shell closures on a possible synthesis of superheavy nuclei are discussed.", "revisions": [ { "version": "v1", "updated": "1996-08-02T15:44:37.000Z" } ], "analyses": { "subjects": [ "21.10.Dr", "21.60.cs", "27.90.+b" ], "keywords": [ "relativistic mean field theory", "superheavy nuclei", "neutron numbers", "shell closure", "atomic number" ], "tags": [ "journal article" ], "publication": { "publisher": "Elsevier", "journal": "Nucl. Phys. A" }, "note": { "typesetting": "LaTeX", "pages": 29, "language": "en", "license": "arXiv", "status": "editable", "inspire": 421578 } } }