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Stochastic Gravitational Wave Background from Cosmological Neutrino-dominated Accretion Flows

We investigate the stochastic gravitational wave background (SGWB) from neutrino-dominated accretion flows (NDAFs) based on the results of our fallback core-collapse supernova (CCSN) simulations. We find that the predicted SGWB is mainly determined by the typical CCSN initial explosion energy and pr...

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Principais autores: Yun-Feng Wei, Tong Liu
פורמט: Artigo
שפה:Inglês
יצא לאור: IOP Publishing 2024-01-01
סדרה:The Astrophysical Journal
נושאים:
Accretion
Black holes
Core-collapse supernovae
Massive stars
Gravitational wave astronomy
גישה מקוונת:https://doi.org/10.3847/1538-4357/ad6b0b
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