Martínez-Pinedo, Gabriel ; Langanke, Karlheinz (2022)
Shell Model Applications in Nuclear Astrophysics.
In: Physics, 4 (2)
doi: 10.3390/physics4020046
Artikel, Bibliographie
Dies ist die neueste Version dieses Eintrags.
Kurzbeschreibung (Abstract)
In recent years, shell model studies have significantly contributed in improving the nuclear input, required in simulations of the dynamics of astrophysical objects and their associated nucleosynthesis. This review highlights a few examples such as electron capture rates and neutrino-nucleus cross sections, important for the evolution and nucleosynthesis of supernovae. For simulations of rapid neutron-capture (r-process) nucleosynthesis, shell model studies have contributed to an improved understanding of half lives of neutron-rich nuclei with magic neutron numbers and of the nuclear level densities and γ-strength functions that are both relevant for neutron capture rates.
| Typ des Eintrags: | Artikel |
|---|---|
| Erschienen: | 2022 |
| Autor(en): | Martínez-Pinedo, Gabriel ; Langanke, Karlheinz |
| Art des Eintrags: | Bibliographie |
| Titel: | Shell Model Applications in Nuclear Astrophysics |
| Sprache: | Englisch |
| Publikationsjahr: | 2022 |
| Ort: | Darmstadt |
| Verlag: | MDPI |
| Titel der Zeitschrift, Zeitung oder Schriftenreihe: | Physics |
| Jahrgang/Volume einer Zeitschrift: | 4 |
| (Heft-)Nummer: | 2 |
| DOI: | 10.3390/physics4020046 |
| Zugehörige Links: | |
| Kurzbeschreibung (Abstract): | In recent years, shell model studies have significantly contributed in improving the nuclear input, required in simulations of the dynamics of astrophysical objects and their associated nucleosynthesis. This review highlights a few examples such as electron capture rates and neutrino-nucleus cross sections, important for the evolution and nucleosynthesis of supernovae. For simulations of rapid neutron-capture (r-process) nucleosynthesis, shell model studies have contributed to an improved understanding of half lives of neutron-rich nuclei with magic neutron numbers and of the nuclear level densities and γ-strength functions that are both relevant for neutron capture rates. |
| Freie Schlagworte: | shell model, core-collapse supernova, r-process nucleosynthesis, neutrino–nucleus reactions, electron capture |
| Zusätzliche Informationen: | This paper is an extended and updated version of the contribution to the 11th International Spring Seminar on Nuclear Physics: Shell Model and Nuclear Structure—Achievements of the Past Two Decades, Ischia, Italy, 12–16 May 2014. |
| Sachgruppe der Dewey Dezimalklassifikatin (DDC): | 500 Naturwissenschaften und Mathematik > 530 Physik |
| Fachbereich(e)/-gebiet(e): | 05 Fachbereich Physik 05 Fachbereich Physik > Institut für Kernphysik 05 Fachbereich Physik > Institut für Kernphysik > Theoretische Kernphysik |
| Hinterlegungsdatum: | 02 Jul 2024 23:13 |
| Letzte Änderung: | 02 Jul 2024 23:13 |
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| Suche nach Titel in: | TUfind oder in Google |
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Shell Model Applications in Nuclear Astrophysics. (deposited 05 Sep 2022 13:06)
- Shell Model Applications in Nuclear Astrophysics. (deposited 02 Jul 2024 23:13) [Gegenwärtig angezeigt]
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