Dataset Open Access

Data publication: Bayesian Analysis of Hybrid Neutron Star EOS Constraints within an Instantaneous Nonlocal Chiral Quark Matter Model

Ayriyan, Alexander; Blaschke, David; Pablo Carlomagno, Juan; Contrera, Gustavo A.; Gabriela Grunfeld, Ana


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{
  "description": "<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>", 
  "datePublished": "2025-07-05", 
  "@id": "https://doi.org/10.14278/rodare.3855", 
  "name": "Data publication: Bayesian Analysis of Hybrid Neutron Star EOS Constraints within an Instantaneous Nonlocal Chiral Quark Matter Model", 
  "identifier": "https://doi.org/10.14278/rodare.3855", 
  "@type": "Dataset", 
  "distribution": [
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      "fileFormat": "dat", 
      "contentUrl": "https://rodare.hzdr.de/api/files/194aa2c6-90df-496a-b897-eaaec1d88b98/DD2p00_2FCSC3DFF_etaD=1.04_etaV=0.44_css_EOS.dat"
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    }, 
    {
      "@type": "DataDownload", 
      "fileFormat": "png", 
      "contentUrl": "https://rodare.hzdr.de/api/files/194aa2c6-90df-496a-b897-eaaec1d88b98/Hybrid_EoS_Bayesian_Analysis.png"
    }, 
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      "fileFormat": "png", 
      "contentUrl": "https://rodare.hzdr.de/api/files/194aa2c6-90df-496a-b897-eaaec1d88b98/Pressure_vs_EnergyDensity.png"
    }, 
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      "fileFormat": "txt", 
      "contentUrl": "https://rodare.hzdr.de/api/files/194aa2c6-90df-496a-b897-eaaec1d88b98/README.txt"
    }
  ], 
  "creator": [
    {
      "@type": "Person", 
      "name": "Ayriyan, Alexander"
    }, 
    {
      "@id": "https://orcid.org/0000-0002-8399-5183", 
      "@type": "Person", 
      "name": "Blaschke, David"
    }, 
    {
      "@type": "Person", 
      "name": "Pablo Carlomagno, Juan"
    }, 
    {
      "@type": "Person", 
      "name": "Contrera, Gustavo A."
    }, 
    {
      "@type": "Person", 
      "name": "Gabriela Grunfeld, Ana"
    }
  ], 
  "license": "https://creativecommons.org/licenses/by/4.0/legalcode", 
  "@context": "https://schema.org/", 
  "url": "https://rodare.hzdr.de/record/3855", 
  "sameAs": [
    "https://www.hzdr.de/publications/Publ-41590"
  ], 
  "keywords": [
    "Bayesian analysis", 
    "hybrid neutron stars", 
    "color superconductivity", 
    "quark deconfinement"
  ]
}
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