[HTML][HTML] New developments in flavor evolution of a dense neutrino gas
I Tamborra, S Shalgar - Annual Review of Nuclear and Particle …, 2021 - annualreviews.org
Neutrino–neutrino refraction dominates the flavor evolution in core-collapse supernovae,
neutron star mergers, and the early Universe. Ordinary neutrino flavor conversions develop …
neutron star mergers, and the early Universe. Ordinary neutrino flavor conversions develop …
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 …
hydrodynamic instabilities play a crucial role in the explosion mechanism. The first …
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 …
Galactic chemical evolution (GCE) models for all stable elements from C (A= 12) to U (A …
Formation of double neutron star systems
Double neutron star (DNS) systems represent extreme physical objects and the endpoint of
an exotic journey of stellar evolution and binary interactions. Large numbers of DNS systems …
an exotic journey of stellar evolution and binary interactions. Large numbers of DNS systems …
The overarching framework of core-collapse supernova explosions as revealed by 3D fornax simulations
A Burrows, D Radice, D Vartanyan… - Monthly Notices of …, 2020 - academic.oup.com
We have conducted 19 state-of-the-art 3D core-collapse supernova simulations spanning a
broad range of progenitor masses. This is the largest collection of sophisticated 3D …
broad range of progenitor masses. This is the largest collection of sophisticated 3D …
Self-consistent 3D supernova models from− 7 minutes to+ 7 s: A 1-bethe explosion of a∼ 19 M⊙ progenitor
R Bollig, N Yadav, D Kresse, HT Janka… - The Astrophysical …, 2021 - iopscience.iop.org
To date, modern three-dimensional (3D) supernova (SN) simulations have not demonstrated
that explosion energies of 10 51 erg (= 1 bethe= 1 B) or more are possible for neutrino …
that explosion energies of 10 51 erg (= 1 bethe= 1 B) or more are possible for neutrino …
[HTML][HTML] 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 …
core-collapse supernovae. In recent years, three-dimensional (3D) simulations of these …
The explosion of helium stars evolved with mass loss
T Ertl, SE Woosley, T Sukhbold… - The Astrophysical …, 2020 - iopscience.iop.org
Light curves, explosion energies, and remnant masses are calculated for a grid of
supernovae resulting from massive helium stars that have been evolved including mass …
supernovae resulting from massive helium stars that have been evolved including mass …
Three-dimensional simulations of neutrino-driven core-collapse supernovae from low-mass single and binary star progenitors
We present a suite of seven 3D supernova simulations of non-rotating low-mass progenitors
using multigroup neutrino transport. Our simulations cover single star progenitors with zero …
using multigroup neutrino transport. Our simulations cover single star progenitors with zero …
Supernova simulations from a 3D progenitor model–Impact of perturbations and evolution of explosion properties
We study the impact of large-scale perturbations from convective shell burning on the core-
collapse supernova explosion mechanism using 3D multigroup neutrino hydrodynamics …
collapse supernova explosion mechanism using 3D multigroup neutrino hydrodynamics …