Explosion mechanisms of core-collapse supernovae
HT Janka - Annual Review of Nuclear and Particle Science, 2012 - annualreviews.org
Supernova theory, numerical and analytic, has made remarkable progress in the past
decade. This progress was made possible by more sophisticated simulation tools, especially …
decade. This progress was made possible by more sophisticated simulation tools, especially …
The supernova–gamma-ray burst connection
SE Woosley, JS Bloom - Annu. Rev. Astron. Astrophys., 2006 - annualreviews.org
Observations show that at least some gamma-ray bursts (GRBs) happen simultaneously
with core-collapse supernovae (SNe), thus linking by a common thread nature's two …
with core-collapse supernovae (SNe), thus linking by a common thread nature's two …
Mind the gap: the location of the lower edge of the pair-instability supernova black hole mass gap
Detections of gravitational waves are now starting to probe the mass distribution of stellar
mass black holes (BHs). Robust predictions from stellar models are needed to interpret …
mass black holes (BHs). Robust predictions from stellar models are needed to interpret …
Compact remnant mass function: dependence on the explosion mechanism and metallicity
The mass distribution of neutron stars and stellar-mass black holes provides vital clues into
the nature of stellar core collapse and the physical engine responsible for supernova …
the nature of stellar core collapse and the physical engine responsible for supernova …
Supernova neutrinos: production, oscillations and detection
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 …
infall dynamics of the stellar core, triggering and fueling the explosion and driving the …
The r-process of stellar nucleosynthesis: Astrophysics and nuclear physics achievements and mysteries
M Arnould, S Goriely, K Takahashi - Physics Reports, 2007 - Elsevier
The r-process, or the rapid neutron-capture process, of stellar nucleosynthesis is called for to
explain the production of the stable (and some long-lived radioactive) neutron-rich nuclides …
explain the production of the stable (and some long-lived radioactive) neutron-rich nuclides …
Theory of core-collapse supernovae
Advances in our understanding and the modeling of stellar core-collapse and supernova
explosions over the past 15 years are reviewed, concentrating on the evolution of …
explosions over the past 15 years are reviewed, concentrating on the evolution of …
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 …
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 …
Constraints from gravitational-wave detections of binary black hole mergers on the 12C (α, γ) 16O rate
Gravitational-wave detections are starting to allow us to probe the physical processes in the
evolution of very massive stars through the imprints they leave on their final remnants …
evolution of very massive stars through the imprints they leave on their final remnants …