End-to-end Kilonova Models of Neutron Star Mergers with Delayed Black Hole Formation

End-to-end Kilonova Models of Neutron Star Mergers with Delayed Black Hole Formation

We investigate the nucleosynthesis and kilonova properties of binary neutron star (NS) merger models that lead to intermediate remnant lifetimes of ∼0.1–1 s until black hole (BH) formation and describe all components of the material ejected during the dynamical merger phase, NS remnant evolution, an...

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Bibliographic Details
Main Authors: O. Just, V. Vijayan, Z. Xiong, S. Goriely, T. Soultanis, A. Bauswein, J. Guilet, H.-Th. Janka, G. Martínez-Pinedo
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal Letters
Subjects:
Hydrodynamical simulations
Compact objects
Gravitational wave astronomy
Transient sources
R-process
Nuclear astrophysics
Online Access:https://doi.org/10.3847/2041-8213/acdad2

Internet

https://doi.org/10.3847/2041-8213/acdad2

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