Hypermassive quark cores
Using a quantum hadrodynamics (QHD) and MIT based models we construct hybrid stars within the Maxwell criteria of hadron-quark phase transition. We are able to produce a hybrid star with maximum mass of 2.15\(M_\odot\). Furthermore, a 2.03\(M_\odot\) star with a quark core corresponding to more than...
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Veröffentlicht in: | arXiv.org 2021-11 |
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Hauptverfasser: | , , |
Format: | Artikel |
Sprache: | eng |
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Online-Zugang: | Volltext |
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Zusammenfassung: | Using a quantum hadrodynamics (QHD) and MIT based models we construct hybrid stars within the Maxwell criteria of hadron-quark phase transition. We are able to produce a hybrid star with maximum mass of 2.15\(M_\odot\). Furthermore, a 2.03\(M_\odot\) star with a quark core corresponding to more than \(80\%\) of both, its total mass and radius, is also possible. |
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ISSN: | 2331-8422 |