- Weitere Titel
-
Schnelle Neutrino Flavor Umwandlungen in Kernkollaps-Supernova Simulationen
- Standort
-
Deutsche Nationalbibliothek Frankfurt am Main
- Umfang
-
Online-Ressource
- Sprache
-
Englisch
- Anmerkungen
-
München, Technische Universität München, Dissertation, 2024
- Schlagwort
-
Supernova
Neutrinooszillation
Neutrino
Flavour
- Ereignis
-
Veröffentlichung
- (wo)
-
München
- (wer)
-
Universitätsbibliothek der TU München
- (wann)
-
2024
- Urheber
-
Ehring, Jakob Christoph
- Beteiligte Personen und Organisationen
- URN
-
urn:nbn:de:bvb:91-diss-20240223-1729708-1-2
- Rechteinformation
-
Der Zugriff auf das Objekt ist unbeschränkt möglich.
- Letzte Aktualisierung
-
25.03.2025, 13:43 MEZ
Datenpartner
Dieses Objekt wird bereitgestellt von:
Deutsche Nationalbibliothek. Bei Fragen zum Objekt wenden Sie sich bitte an den Datenpartner.
Deutsche Nationalbibliothek. Bei Fragen zum Objekt wenden Sie sich bitte an den Datenpartner.
Beteiligte
- Ehring, Jakob Christoph
- Janka, Hans-Thomas
- Weiler, Andreas
- Universitätsbibliothek der TU München
Entstanden
- 2024
Ähnliche Objekte (12)
Neutrino nucleosynthesis in core-collapse Supernova explosions
Supernova neutrino spectra and applications to flavor oscillations
Supernova neutrino spectra and applications to flavor oscillations
Modeling neutrino-driven core-collapse supernova explosions in three dimensions
Two- and three-dimensional simulations of core-collapse supernova explosions of massive stars applying neutrino hydrodynamics
Two- and Three-Dimensional Simulations of Core-Collapse Supernova Explosions of Massive Stars Applying Neutrino Hydrodynamics
Correlated Signatures of Gravitational-wave and Neutrino Emission in Three-dimensional General-relativistic Core-collapse Supernova Simulations
Explosion dynamics of parametrized spherically symmetric core-collapse supernova simulations
Applications of Different Neutrino-Transport Methods in Three-Dimensional Supernova Simulations
Neutrino Interactions with Supernova Matter
Towards Energy Saturation in Three-dimensional Simulations of Core-collapse Supernova Explosions
Neutrinos in Core-Collapse Supernova Nucleosynthesis
Neutrino nucleosynthesis in core-collapse Supernova explosions
Supernova neutrino spectra and applications to flavor oscillations
Supernova neutrino spectra and applications to flavor oscillations
Modeling neutrino-driven core-collapse supernova explosions in three dimensions
Two- and three-dimensional simulations of core-collapse supernova explosions of massive stars applying neutrino hydrodynamics
Two- and Three-Dimensional Simulations of Core-Collapse Supernova Explosions of Massive Stars Applying Neutrino Hydrodynamics
Correlated Signatures of Gravitational-wave and Neutrino Emission in Three-dimensional General-relativistic Core-collapse Supernova Simulations
Explosion dynamics of parametrized spherically symmetric core-collapse supernova simulations
Applications of Different Neutrino-Transport Methods in Three-Dimensional Supernova Simulations
Neutrino Interactions with Supernova Matter
Towards Energy Saturation in Three-dimensional Simulations of Core-collapse Supernova Explosions
Neutrinos in Core-Collapse Supernova Nucleosynthesis
Neutrino nucleosynthesis in core-collapse Supernova explosions
Supernova neutrino spectra and applications to flavor oscillations
Supernova neutrino spectra and applications to flavor oscillations
Modeling neutrino-driven core-collapse supernova explosions in three dimensions
Two- and three-dimensional simulations of core-collapse supernova explosions of massive stars applying neutrino hydrodynamics
Two- and Three-Dimensional Simulations of Core-Collapse Supernova Explosions of Massive Stars Applying Neutrino Hydrodynamics
Correlated Signatures of Gravitational-wave and Neutrino Emission in Three-dimensional General-relativistic Core-collapse Supernova Simulations
Explosion dynamics of parametrized spherically symmetric core-collapse supernova simulations
Applications of Different Neutrino-Transport Methods in Three-Dimensional Supernova Simulations
Neutrino Interactions with Supernova Matter
Towards Energy Saturation in Three-dimensional Simulations of Core-collapse Supernova Explosions