Physics of core-collapse supernovae in three dimensions: a sneak preview

HT Janka, T Melson, A Summa - Annual Review of Nuclear and …, 2016 - annualreviews.org
Nonspherical mass motions are a generic feature of core-collapse supernovae, and
hydrodynamic instabilities play a crucial role in the explosion mechanism. The first …

Nucleosynthesis in stars and the chemical enrichment of galaxies

K Nomoto, C Kobayashi… - Annual Review of …, 2013 - annualreviews.org
After the Big Bang, production of heavy elements in the early Universe takes place starting
from the formation of the first stars, their evolution, and explosion. The first supernova …

The origin of elements from carbon to uranium

C Kobayashi, AI Karakas, M Lugaro - The Astrophysical Journal, 2020 - iopscience.iop.org
To reach a deeper understanding of the origin of elements in the periodic table, we construct
Galactic chemical evolution (GCE) models for all stable elements from C (A= 12) to U (A …

[HTML][HTML] Supernova neutrinos: production, oscillations and detection

A Mirizzi, I Tamborra, HT Janka, N Saviano… - La Rivista del Nuovo …, 2016 - Springer
Neutrinos play a crucial role in the collapse and explosion of massive stars, governing the
infall dynamics of the stellar core, triggering and fueling the explosion and driving the …

Hydrodynamics of core-collapse supernovae and their progenitors

B Müller - Living Reviews in Computational Astrophysics, 2020 - Springer
Multi-dimensional fluid flow plays a paramount role in the explosions of massive stars as
core-collapse supernovae. In recent years, three-dimensional (3D) simulations of these …

A two-parameter criterion for classifying the explodability of massive stars by the neutrino-driven mechanism

T Ertl, HT Janka, SE Woosley, T Sukhbold… - The Astrophysical …, 2016 - iopscience.iop.org
Thus far, judging the fate of a massive star (either a neutron star [NS] or a black hole) solely
by its structure prior to core collapse has been ambiguous. Our work and previous attempts …

Supernova simulations from a 3D progenitor model–Impact of perturbations and evolution of explosion properties

B Müller, T Melson, A Heger… - Monthly Notices of the …, 2017 - academic.oup.com
We study the impact of large-scale perturbations from convective shell burning on the core-
collapse supernova explosion mechanism using 3D multigroup neutrino hydrodynamics …

THREE-DIMENSIONAL CORE-COLLAPSE SUPERNOVA SIMULATED USING A 15 M☉ PROGENITOR

EJ Lentz, SW Bruenn, WR Hix… - The Astrophysical …, 2015 - iopscience.iop.org
We have performed ab initio neutrino radiation hydrodynamics simulations in three and two
spatial dimensions (3D and 2D) of core-collapse supernovae from the same 15 M☉ …

The status of multi-dimensional core-collapse supernova models

B Müller - Publications of the Astronomical Society of Australia, 2016 - cambridge.org
Models of neutrino-driven core-collapse supernova explosions have matured considerably
in recent years. Explosions of low-mass progenitors can routinely be simulated in 1D, 2D …

[图书][B] Supernova explosions

D Branch, JC Wheeler - 2017 - Springer
JCW had long wanted to write a new monograph on supernovae. Despite an immense
explosion in the literature and many review articles, there had not been one since that of …