Strange matter in core-collapse supernovae
We discuss the possible impact of strange quark matter on the evolution of core-collapse supernovae with emphasis on low critical densities for the quark-hadron phase transition. For such cases the hot proto-neutron star can collapse to a more compact hybrid star configuration hundreds of millisecon...
Gespeichert in:
| Hauptverfasser: | , , |
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| Dokumenttyp: | Article (Journal) Konferenzschrift |
| Sprache: | Englisch |
| Veröffentlicht: |
2012
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| In: |
Acta physica Polonica. B, Particle physics and field theory, nuclear physics, theory of relativity
Year: 2011, Jahrgang: 43, Heft: 4, Pages: 741-748 |
| ISSN: | 1509-5770 |
| DOI: | 10.5506/APhysPolB.43.741 |
| Schlagworte: | |
| Online-Zugang: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.5506/APhysPolB.43.741 Verlag, kostenfrei, Volltext: https://www.actaphys.uj.edu.pl/fulltext?series=Reg&vol=43&page=741 
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| Verfasserangaben: | I. Sagert, T. Fischer, M. Hempel, G. Pagliara, J. Schaffner-Bielich, F.-K. Thielemann, M. Liebendörfer |
| Zusammenfassung: | We discuss the possible impact of strange quark matter on the evolution of core-collapse supernovae with emphasis on low critical densities for the quark-hadron phase transition. For such cases the hot proto-neutron star can collapse to a more compact hybrid star configuration hundreds of milliseconds after core-bounce. The collapse triggers the formation of a second shock wave. The latter leads to a successful supernova explosion and leaves an imprint on the neutrino signal. These dynamical features are discussed with respect to their compatibility with recent neutron star mass measurements which indicate a stiff high density nuclear matter equation of state. |
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| Beschreibung: | Online: 29 Dec 2011 Gesehen am 12.06.2018 |
| Beschreibung: | Online Resource |
| ISSN: | 1509-5770 |
| DOI: | 10.5506/APhysPolB.43.741 |