July 16, 2025 Dataset Open Access

Gärtlein, Christoph; Sagun, Violetta; Ivanytskyi, Oleksii; Blaschke, David; Lopes, Ilido

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  <identifier identifierType="DOI">10.14278/rodare.3879</identifier>
  <creators>
    <creator>
      <creatorName>Gärtlein, Christoph</creatorName>
      <givenName>Christoph</givenName>
      <familyName>Gärtlein</familyName>
    </creator>
    <creator>
      <creatorName>Sagun, Violetta</creatorName>
      <givenName>Violetta</givenName>
      <familyName>Sagun</familyName>
    </creator>
    <creator>
      <creatorName>Ivanytskyi, Oleksii</creatorName>
      <givenName>Oleksii</givenName>
      <familyName>Ivanytskyi</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>Lopes, Ilido</creatorName>
      <givenName>Ilido</givenName>
      <familyName>Lopes</familyName>
    </creator>
  </creators>
  <titles>
    <title>Data publication: Fastest spinning millisecond pulsars: Indicators for quark matter in neutron stars?</title>
  </titles>
  <publisher>Rodare</publisher>
  <publicationYear>2025</publicationYear>
  <subjects>
    <subject>millisecond pulsars</subject>
    <subject>quark matter</subject>
    <subject>deconfinement phase transition</subject>
    <subject>hypernuclear matter</subject>
    <subject>black widow pulsar</subject>
    <subject>accretion induced spin-up</subject>
    <subject>Kepler frequency</subject>
    <subject>color superconductivity</subject>
    <subject>oblateness</subject>
  </subjects>
  <dates>
    <date dateType="Issued">2025-07-16</date>
  </dates>
  <language>en</language>
  <resourceType resourceTypeGeneral="Dataset"/>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://rodare.hzdr.de/record/3879</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsReferencedBy">10.1103/PhysRevD.111.123021</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="URL" relationType="IsIdenticalTo">https://www.hzdr.de/publications/Publ-41631</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="URL" relationType="IsReferencedBy">https://www.hzdr.de/publications/Publ-41503</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsVersionOf">10.14278/rodare.3878</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>
  </relatedIdentifiers>
  <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">&lt;p&gt;This data publication contains the following selected sets of data: 1) hybrid equations of state (EoSs) obtained via Maxwell construction of a first-order phase transition from hadronic to quark matter (hadronic matter: DD2npY-T, quark matter: NJL-model -&amp;gt; parameters: vector coupling $\eta_V$ and diquark coupling $\eta_D$) 2) files containing outcomes from calculations of compact star configurations with the RNS-code (static configuration, rotation at Kepler frequency, rotation at constant frequency, rotation for fixed rest mass) 3) accretion model (magnetic field + mass accretion)&lt;/p&gt;</description>
  </descriptions>
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