Janka, Hans-Thomas
2018-06-09
First three-dimensional, first-principle simulations of
core-collapse supernovae have become possible in the recent past.
They demonstrate the basic viability of the neutrino-driven mechanism
for powering the explosions of the majority of supernova progenitors.
However, important questions still remain to be settled. These include
basic technical aspects such as the influence of the numerical
resolution or the method of the neutrino-transport treatment,
as well as important physics aspects such as the initial stellar
conditions and still missing physics, for example effects of muon
formation and neutrino oscillations. The talk will review the current
status of 3D supernova modeling and of our understanding of
neutrino-driven explosions. It will also provide an outlook
on current progress for answering the open questions mentioned.
https://doi.org/10.5281/zenodo.1287036
oai:zenodo.org:1287036
Zenodo
https://zenodo.org/communities/neutrino2018
https://doi.org/10.5281/zenodo.1287035
info:eu-repo/semantics/openAccess
Creative Commons Attribution 4.0 International
https://creativecommons.org/licenses/by/4.0/legalcode
Neutrino 2018, XXVIII International Conference on Neutrino Physics and Astrophysics, Heidelberg, Germany, 4-9 June 2018
Neutrino-driven Explosions in 3D Supernova Simulations
info:eu-repo/semantics/lecture