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Data publication: Hybrid star phenomenology from the properties of the special point

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


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    <dct:title>Data publication: Hybrid star phenomenology from the properties of the special point</dct:title>
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    <dcat:keyword>Quark matter in neutron stars</dcat:keyword>
    <dcat:keyword>Quark-gluon plasma</dcat:keyword>
    <dcat:keyword>Dense nuclear matter</dcat:keyword>
    <dcat:keyword>High-mass pulsars</dcat:keyword>
    <dcat:keyword>PSR J0952-0607</dcat:keyword>
    <dcat:keyword>PSR J0740+6620</dcat:keyword>
    <dcat:keyword>PSR J0030+0451</dcat:keyword>
    <dcat:keyword>GW170817</dcat:keyword>
    <dct:issued rdf:datatype="http://www.w3.org/2001/XMLSchema#date">2024-01-19</dct:issued>
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    <dct:description>&lt;p&gt;The columns of files EOS_TOV_etaV_etaD.TXT include central values of the baryonic chemical potential [MeV], pressure [MeV/fm^3], baryonic density [1/fm^3], radius [km] and mass [M_solar] of neutron stars modelled with hybrid quark-hadron equations of state constructed for the vector and diquark couplings etaV and etaD specified in the titles. The corresponding mass-radius diagrams are presented in Figs. 6-8 of the paper. The columns of the file etaV-etaD.TXT include diquark coupling and values of the vector coupling corresponding to the boundaries of the region providing the conditions of having the onset of deconfinement above the saturation density and stability of the quark branch of the mass-radius curve obtained as a solution of the TOV equation (see Fig. 7 of the paper).&lt;/p&gt;</dct:description>
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