Reactions of exotic nuclei with the quark-meson coupling model

dc.contributor.authorMcRae, Ellen
dc.contributor.authorSimenel, Cedric
dc.contributor.authorSimpson, Edward
dc.contributor.authorThomas, Anthony
dc.coverage.spatialXi'an, China
dc.date.accessioned2020-05-19T04:26:18Z
dc.date.available2020-05-19T04:26:18Z
dc.date.created10 July 2017 through 13 July 2017
dc.date.issued2017
dc.date.updated2019-12-19T06:13:07Z
dc.description.abstractThe nucleon-nucleon interaction is an important requirement for investigations of nuclear structure and reactions, as well as for astrophysical models such as r-process nucleosynthesis and neutron stars. The traditional approach to low-energy nuclear physics is to treat nucleons as immutable objects interacting via phenomenological forces. The use of phenomenological interactions, rather than one derived from a microscopic theory, raises questions as to the reliability of predictions for exotic regions of the nuclear chart. The quark-meson coupling (QMC) model uses a relativistic mean-field approach to provide a microscopically derived nucleon-nucleon interaction, which takes into account the quark structure of the nucleon. The Skyrme energy density functional is a popular phenomenological tool in studies of nuclear structure and reactions. In this work, the QMC density functional was used to produce a set of Skyrme parameterisations, in the hopes that they will give more reliable predictions for exotic nuclei. In conjunction with Hartree-Fock-Bogoliubov (HFB) calculations, the Skyrme-QMC (SQMC) parameterisations have been used to model the ground-state properties of individual nuclei and nucleus-nucleus potentials for Ca + Sn reactions. The SQMC parameterisation performs with an accuracy comparable to modern phenomenological functionals. From this, one can investigate the importance of the isovector terms of the nucleon-nucleon interaction, which are particularly significant for exotic, neutron-rich regions of the nuclear chart. One of the notable successes of the QMC model is its derivation of nuclear spin-orbit coupling. The isovector dependence of the spin-orbit equation of state is remarkably similar to that of the modern UNEDF1 phenomenological density functional. HFB calculations along the Sn isotopic chain reveal that the isovector properties of the spin-orbit term impact binding energies to a level that will be significant for astrophysical r-process modelling.en_AU
dc.description.sponsorshipThis research is supported by an Australian Government Research Training Program (RTP) Scholarship and ARC Grants FT120100760 and DP160101254.en_AU
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.isbn9780996452700en_AU
dc.identifier.urihttp://hdl.handle.net/1885/204447
dc.language.isoen_AUen_AU
dc.provenance© The Authors, published by EDP Sciences. This is an open access article distributed under the terms of the Creative Commons Attribution License 4.0 (http://creativecommons.org/licenses/by/4.0/).en_AU
dc.publisherEDP Sciencesen_AU
dc.relationhttp://purl.org/au-research/grants/arc/FT120100760en_AU
dc.relationhttp://purl.org/au-research/grants/arc/DP160101254en_AU
dc.relation.ispartofseries2017 20th International Conference on Information Fusion
dc.rights© The Authors, published by EDP Sciences.en_AU
dc.rights.licenseCreative Commons Attribution License 4.0en_AU
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/en_AU
dc.sourceEPJ Web of Conferencesen_AU
dc.titleReactions of exotic nuclei with the quark-meson coupling modelen_AU
dc.typeConference paperen_AU
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.lastpage5en_AU
local.bibliographicCitation.startpage1en_AU
local.contributor.affiliationMcRae, Ellen, College of Science, ANUen_AU
local.contributor.affiliationSimenel, Cedric, College of Science, ANUen_AU
local.contributor.affiliationSimpson, Edward, College of Science, ANUen_AU
local.contributor.affiliationThomas, Anthony, The University of Adelaideen_AU
local.contributor.authoruidMcRae, Ellen, u5178470en_AU
local.contributor.authoruidSimenel, Cedric, u4787848en_AU
local.contributor.authoruidSimpson, Edward, u5633413en_AU
local.description.notesImported from ARIESen_AU
local.description.refereedYes
local.identifier.absfor020202 - Nuclear Physicsen_AU
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciencesen_AU
local.identifier.ariespublicationa383154xPUB9142en_AU
local.identifier.doi10.1051/epjconf/201716300036en_AU
local.identifier.scopusID2-s2.0-85036657243
local.publisher.urlhttps://www.epj.org/en_AU
local.type.statusPublished Versionen_AU

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