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Medium modifications for light and heavy nuclear clusters in simulations of core collapse supernovae: Impact on equation of state and weak interactions

Fischer, Tobias ; Typel, Stefan ; Röpke, Gerd ; Bastian, Niels-Uwe F. ; Martínez-Pinedo, Gabriel (2020)
Medium modifications for light and heavy nuclear clusters in simulations of core collapse supernovae: Impact on equation of state and weak interactions.
In: Physical Review C, 102 (5)
doi: 10.1103/PhysRevC.102.055807
Artikel, Bibliographie

Kurzbeschreibung (Abstract)

The present article investigates the role of heavy nuclear clusters and weakly bound light nuclear clusters based on a newly developed equation of state for core collapse supernova studies. A novel approach is brought forward for the description of nuclear clusters, taking into account the quasiparticle approach and continuum correlations. It demonstrates that the commonly employed nuclear statistical equilibrium approach, based on noninteracting particles, for the description of light and heavy clusters becomes invalid for warm nuclear matter near the saturation density. This has important consequences for studies of core collapse supernovae. To this end, we implement this nuclear equation of state provided for arbitrary temperature, baryon density, and isospin asymmetry, to spherically symmetric core collapse supernova simulations to study the impact on the dynamics as well as on the neutrino emission. For the inclusion of a set of weak processes involving light clusters the rate expressions are derived, including medium modifications at the mean-field level. A substantial impact from the inclusion of a variety of weak reactions involving light clusters on the post bounce dynamics and on the neutrino emission could not be found.

Typ des Eintrags: Artikel
Erschienen: 2020
Autor(en): Fischer, Tobias ; Typel, Stefan ; Röpke, Gerd ; Bastian, Niels-Uwe F. ; Martínez-Pinedo, Gabriel
Art des Eintrags: Bibliographie
Titel: Medium modifications for light and heavy nuclear clusters in simulations of core collapse supernovae: Impact on equation of state and weak interactions
Sprache: Englisch
Publikationsjahr: 25 November 2020
Verlag: APS physics
Titel der Zeitschrift, Zeitung oder Schriftenreihe: Physical Review C
Jahrgang/Volume einer Zeitschrift: 102
(Heft-)Nummer: 5
DOI: 10.1103/PhysRevC.102.055807
Kurzbeschreibung (Abstract):

The present article investigates the role of heavy nuclear clusters and weakly bound light nuclear clusters based on a newly developed equation of state for core collapse supernova studies. A novel approach is brought forward for the description of nuclear clusters, taking into account the quasiparticle approach and continuum correlations. It demonstrates that the commonly employed nuclear statistical equilibrium approach, based on noninteracting particles, for the description of light and heavy clusters becomes invalid for warm nuclear matter near the saturation density. This has important consequences for studies of core collapse supernovae. To this end, we implement this nuclear equation of state provided for arbitrary temperature, baryon density, and isospin asymmetry, to spherically symmetric core collapse supernova simulations to study the impact on the dynamics as well as on the neutrino emission. For the inclusion of a set of weak processes involving light clusters the rate expressions are derived, including medium modifications at the mean-field level. A substantial impact from the inclusion of a variety of weak reactions involving light clusters on the post bounce dynamics and on the neutrino emission could not be found.

Zusätzliche Informationen:

Art.No.: 055807

Fachbereich(e)/-gebiet(e): 05 Fachbereich Physik
05 Fachbereich Physik > Institut für Kernphysik
05 Fachbereich Physik > Institut für Kernphysik > Theoretische Kernphysik
05 Fachbereich Physik > Institut für Kernphysik > Theoretische Kernphysik > Kernphysik und Nukleare Astrophysik
05 Fachbereich Physik > Institut für Kernphysik > Theoretische Kernphysik > Kern- und Vielteilchenphysik
05 Fachbereich Physik > Institut für Kernphysik > Theoretische Kernphysik > Theoretische nukleare Astrophysik
Hinterlegungsdatum: 13 Jul 2022 07:45
Letzte Änderung: 27 Dez 2022 09:44
PPN: 503198056
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