Dataset Open Access
Ayriyan, Alexander;
Blaschke, David;
Pablo Carlomagno, Juan;
Contrera, Gustavo A.;
Gabriela Grunfeld, Ana
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<identifier identifierType="DOI">10.14278/rodare.3855</identifier>
<creators>
<creator>
<creatorName>Ayriyan, Alexander</creatorName>
<givenName>Alexander</givenName>
<familyName>Ayriyan</familyName>
</creator>
<creator>
<creatorName>Blaschke, David</creatorName>
<givenName>David</givenName>
<familyName>Blaschke</familyName>
<nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0002-8399-5183</nameIdentifier>
</creator>
<creator>
<creatorName>Pablo Carlomagno, Juan</creatorName>
<givenName>Juan</givenName>
<familyName>Pablo Carlomagno</familyName>
</creator>
<creator>
<creatorName>Contrera, Gustavo A.</creatorName>
<givenName>Gustavo A.</givenName>
<familyName>Contrera</familyName>
</creator>
<creator>
<creatorName>Gabriela Grunfeld, Ana</creatorName>
<givenName>Ana</givenName>
<familyName>Gabriela Grunfeld</familyName>
</creator>
</creators>
<titles>
<title>Data publication: Bayesian Analysis of Hybrid Neutron Star EOS Constraints within an Instantaneous Nonlocal Chiral Quark Matter Model</title>
</titles>
<publisher>Rodare</publisher>
<publicationYear>2025</publicationYear>
<subjects>
<subject>Bayesian analysis</subject>
<subject>hybrid neutron stars</subject>
<subject>color superconductivity</subject>
<subject>quark deconfinement</subject>
</subjects>
<dates>
<date dateType="Issued">2025-07-05</date>
</dates>
<resourceType resourceTypeGeneral="Dataset"/>
<alternateIdentifiers>
<alternateIdentifier alternateIdentifierType="url">https://rodare.hzdr.de/record/3855</alternateIdentifier>
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<relatedIdentifiers>
<relatedIdentifier relatedIdentifierType="DOI" relationType="IsReferencedBy">10.3390/universe11050141</relatedIdentifier>
<relatedIdentifier relatedIdentifierType="URL" relationType="IsIdenticalTo">https://www.hzdr.de/publications/Publ-41590</relatedIdentifier>
<relatedIdentifier relatedIdentifierType="URL" relationType="IsReferencedBy">https://www.hzdr.de/publications/Publ-41519</relatedIdentifier>
<relatedIdentifier relatedIdentifierType="DOI" relationType="IsVersionOf">10.14278/rodare.3854</relatedIdentifier>
<relatedIdentifier relatedIdentifierType="URL" relationType="IsPartOf">https://rodare.hzdr.de/communities/matter</relatedIdentifier>
<relatedIdentifier relatedIdentifierType="URL" relationType="IsPartOf">https://rodare.hzdr.de/communities/rodare</relatedIdentifier>
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<rightsList>
<rights rightsURI="https://creativecommons.org/licenses/by/4.0/legalcode">Creative Commons Attribution 4.0 International</rights>
<rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
</rightsList>
<descriptions>
<description descriptionType="Abstract"><p>This dataset contains tabulated hybrid Equations of State (EOS) for neutron star matter, with a phase transition generated by a Maxwell construction between an instantaneous nonlocal chiral quark model for the quark matter phase and the relativistic mean field model &quot;DD2&quot; for the nuclear matter phase. The Bayesian analysis explores the EOS parameter space characterized by the coupling constants \eta_D and \eta_V, which govern diquark and vector interactions, respectively. The provided data includes EOS tables for selected parameter sets. The coupling parameters were selected from the 60% Bayesian credibility region for physically significant cases (see figure Hybrid_EoS_Bayesian_Analysis.png), such as: &bull; the maximum and minimum neutron star masses &bull; the maximum and minimum neutron star onset &bull; the most probable EOS from the Bayesian posterior This dataset enables further analysis of neutron star properties, supporting transparency and reproducibility of the published results.</p></description>
<description descriptionType="Other">The research was supported by the Polish National Science Center (NCN) under the Polonez-BIS program with grant number 2021/43/P/ST2/03319 and by the Argentinian organizations CONICET, ANPCyT and UNLP under grants Numbers PIP 2022-2024 GI-11220210100150CO, PICT19-00792, PICT22-03-00799 and X960, respectively.</description>
</descriptions>
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