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Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/124699
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dc.contributor.authorMotta, T.F.-
dc.contributor.authorThomas, A.W.-
dc.contributor.authorGuichon, P.A.M.-
dc.date.issued2020-
dc.identifier.citationPhysics Letters B: Nuclear Physics and Particle Physics, 2020; 802:1-5-
dc.identifier.issn0370-2693-
dc.identifier.issn1873-2445-
dc.identifier.urihttp://hdl.handle.net/2440/124699-
dc.description.abstractThe presence of exotic hadrons, such as hyperons and isobars, in the dense nuclear matter in their cores has been shown to produce important changes in the properties of neutron stars. Within the quark-meson coupling model, we show that the many-body forces generated by the change in the internal quark structure of the baryons in the strong scalar mean fields generated in dense nuclear matter prohibit the appearance of Δ isobars-
dc.description.statementofresponsibilityT.F. Motta, A.W. Thomas, P.A.M. Guichon-
dc.language.isoen-
dc.publisherElsevier-
dc.rights© 2020 The Authors. Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/). Funded by SCOAP3-
dc.source.urihttp://dx.doi.org/10.1016/j.physletb.2020.135266-
dc.titleDo Delta baryons play a role in neutron stars?-
dc.typeJournal article-
dc.identifier.doi10.1016/j.physletb.2020.135266-
dc.relation.granthttp://purl.org/au-research/grants/arc/DP150103101-
dc.relation.granthttp://purl.org/au-research/grants/arc/DP18010049-
pubs.publication-statusPublished-
dc.identifier.orcidThomas, A.W. [0000-0003-0026-499X]-
Appears in Collections:Aurora harvest 8
Physics publications

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