Gravitational waves from 3D core-collapse supernova models: The impact of moderate progenitor rotation
- Resource Type
- Authors
- H.-Th. Janka; Kiranjyot Gill; Ewald Müller; Alexander Summa; Michele Zanolin; H. Andresen
- Source
- Monthly Notices of the Royal Astronomical Society. 486:2238-2253
- Subject
- Physics
010308 nuclear & particles physics
Astrophysics::High Energy Astrophysical Phenomena
Astronomy and Astrophysics
Angular velocity
Astrophysics
Rotation
Type II supernova
01 natural sciences
Specific relative angular momentum
Instability
Supernova
Amplitude
13. Climate action
Space and Planetary Science
0103 physical sciences
Astrophysics::Solar and Stellar Astrophysics
010303 astronomy & astrophysics
Stellar evolution
Astrophysics::Galaxy Astrophysics
- Language
- ISSN
- 1365-2966
0035-8711
We present predictions for the gravitational-wave (GW) emission of three-dimensional supernova (SN) simulations performed for a 15 solar-mass progenitor with the Prometheus-Vertex code using energy-dependent, three-flavor neutrino transport. The progenitor adopted from stellar evolution calculations including magnetic fields had a fairly low specific angular momentum (j_Fe