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Original title:
Towards Energy Saturation in Three-dimensional Simulations of Core-collapse Supernova Explosions
Translated title:
Dreidimensionale Simulationen von Kernkollaps-Supernova-Explosionen bis zur Energiesaturation
Author:
Kresse, Daniel
Year:
2023
Document type:
Dissertation
Faculty/School:
TUM School of Natural Sciences
Advisor:
Janka, Hans-Thomas (Prof. Dr.)
Referee:
Janka, Hans-Thomas (Prof. Dr.); Ibarra, Alejandro (Prof. Dr.)
Language:
en
Subject group:
PHY Physik
TUM classification:
PHY 900
Abstract:
Core-collapse supernovae (CCSNe) are the violent explosions of massive stars. Yet, their detailed explosion mechanism is still a matter of intense research. By performing three-dimensional (3D) hydrodynamics simulations, including a newly developed scheme for neutrino heating and cooling effects, we demonstrate that self-consistent 3D models of neutrino-driven CCSNe can yield explosion properties in agreement with observations on relevant timescales of several seconds.
Translated abstract:
Kernkollaps-Supernovae (KKSNe) sind gewaltige Explosionen massereicher Sterne. Ihr detaillierter Explosionsmechanismus ist bis heute Gegenstand intensiver Forschung. Mittels dreidimensionaler (3D) hydrodynamischer Simulationen einschließlich eines neu entwickelten Schemas für Neutrino-Heiz- und Kühleffekte zeigen wir, dass selbstkonsistente 3D-Modelle neutrinogetriebener KKSNe über Zeitskalen von mehreren Sekunden Explosionseigenschaften in Übereinstimmung mit Beobachtungen liefern können.
WWW:
https://mediatum.ub.tum.de/?id=1707410
Date of submission:
03.05.2023
Oral examination:
27.06.2023
File size:
22487886 bytes
Pages:
174
Urn (citeable URL):
https://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:91-diss-20230627-1707410-1-6
Last change:
26.06.2024
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