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Numerical simulations of the random angular momentum in convection: Implications for supergiant collapse to form black holes
Andrea Antoni,
Eliot Quataert
Astrophysical Sciences
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Article
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peer-review
31
Scopus citations
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Dive into the research topics of 'Numerical simulations of the random angular momentum in convection: Implications for supergiant collapse to form black holes'. Together they form a unique fingerprint.
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Keyphrases
Accrete
33%
Angular Momentum
100%
Angular Momentum Vector
33%
ATHENA
33%
Black Hole Spin
33%
Circularization
33%
Convection
100%
Convective Flow
66%
Core-collapse
33%
Hydrodynamic Simulation
33%
Idealized Models
33%
Infall
66%
Innermost Stable Circular Orbit
33%
Massive Stars
33%
Non-rotating
66%
Numerical Simulation
100%
Optically Thick
33%
PERFORM-3D
33%
Polytropic Model
33%
Red Supergiants
66%
Slowly Varying
33%
Small Radius
33%
Spin Parameter
66%
Stellar Radii
33%
Supergiants
100%
Support Material
33%
Physics
Angular Momentum
100%
Black Holes
100%
Circular Orbit
16%
Convective Envelopes
16%
Convective Flow
33%
Energetics
16%
Hydrodynamical Simulations
16%
Idealized Model
16%
Massive Star
16%
Red Supergiant Stars
33%
Stellar Radii
16%
Supergiant
100%
Transients
33%