The physics of core-collapse supernovae

The physics of core-collapse supernovae is …
instance of (P31):
scholarly articleQ13442814

External links are
P818arXiv IDastro-ph/0601261
P356DOI10.1038/NPHYS172
P8608Fatcat IDrelease_u2rdukh4azbifl4m4liqvhe2lq
P5875ResearchGate publication ID1778244

P50authorStanford E. WoosleyQ1243485
P2093author name stringThomas Janka
P2860cites workThe evolution and explosion of massive starsQ21563879
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Supernova Simulations with Boltzmann Neutrino Transport: A Comparison of MethodsQ57589100
Toward Gravitational Wave Signals from Realistic Core‐Collapse Supernova ModelsQ57589105
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Asymmetric supernovae, pulsars, magnetars, and gamma-ray burstsQ68275242
Some properties of r-process accretion disks and jetsQ68313444
The velocity distribution of isolated radio pulsarsQ68326332
Stability of standing accretion shocks, with an eye toward core-collapse supernovaeQ68346964
Magnetic protoneutron star winds and r-process nucleosynthesisQ68347091
The collapse of rotating massive stars in three dimensionsQ68369773
Pulsar recoil by large-scale anisotropies in supernova explosionsQ68370761
Anisotropies in the neutrino fluxes and heating profiles in two-dimensional, time-dependent, multigroup radiation hydrodynamics simulations of rotating core-collapse supernovaeQ68458723
Presupernova evolution of differentially rotating massive stars including magnetic fieldsQ68458728
Alfven wave-driven proto-neutron star winds and r-process nucleosynthesisQ68459515
A numerical example of the collapse of a rotating magnetized starQ68580184
On the metallicity dependence of Wolf-Rayet windsQ68590876
Evolution of rapidly rotating metal-poor massive stars towards gamma-ray burstsQ68591012
Isotopic r-process abundances and nuclear structure far from stability: implications for the r-process mechanismQ68794764
On the nature of core-collapse supernova explosionsQ68808234
Nucleosynthesis in neutrino-driven winds. I. The physical conditionsQ68817628
Dynamo action by differential rotation in a stably stratified stellar interiorQ68843065
Non-radial instabilities of isothermal Bondi accretion with a shock: Vortical-acoustic cycle vs. post-shock accelerationQ68844373
Neutron star mergers versus core-collapse supernovae as dominant r-process sites in the early GalaxyQ68847324
An investigation of neutrino-driven convection and the core collapse supernova mechanism using multigroup neutrino transportQ68869338
The magnetorotational instability in core-collapse supernova explosionsQ68884327
A systematic analysis of supernova light in gamma-ray burst afterglowsQ68888258
P433issue3
P304page(s)147-154
P577publication date2005-12-01
P1433published inNature PhysicsQ2108381
P1476titleThe physics of core-collapse supernovae
P478volume1

Reverse relations

cites work (P2860)
Q50236782Constraining the axion-photon coupling with massive stars
Q104756762Core-collapse supernova explosion theory
Q57431979Cross-section measurement of9Be(γ,n)8Be and implications forα+α+n→9Be in therprocess
Q30364009Numerical hydrodynamics and magnetohydrodynamics in general relativity
Q57834650Quasiequilibrium models for triaxially deformed rotating compact stars
Q85079138Self-Refraction of Supernova Neutrinos: Mixed Spectra and Three-Flavor Instabilities
Q59062981Two populations of X-ray pulsars produced by two types of supernova

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