A New Kilohertz Gravitational-wave Feature from Rapidly Rotating Core-collapse Supernovae

A New Kilohertz Gravitational-wave Feature from Rapidly Rotating Core-collapse Supernovae

We present self-consistent three-dimensional core-collapse supernova simulations of a rotating 20 M _⊙ progenitor model with various initial angular velocities from 0.0 to 4.0 rad s ^−1 using the smoothed particle hydrodynamics code SPHYNX and the grid-based hydrodynamics code FLASH . We identify tw...

Full description

Bibliographic Details
Main Authors: He-Feng Hsieh, Rubén Cabezón, Li-Ting Ma, Kuo-Chuan Pan
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Core-collapse supernovae
Gravitational wave astronomy
Hydrodynamical simulations
Neutron stars
Online Access:https://doi.org/10.3847/1538-4357/ad08c2

Internet

https://doi.org/10.3847/1538-4357/ad08c2

Similar Items