Three dimensional end-to-end simulation for kilonova emission from a black hole neutron star merger

We study long-term evolution of the matter ejected in a black hole neutron star (BH–NS) merger employing the results of a long-term numerical-relativity simulation and nucleosynthesis calculation, in which both dynamical and post-merger ejecta formation is consistently followed. In particular, we em...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2024-12, Vol.535 (4), p.3711-3731
Hauptverfasser:	Kawaguchi, Kyohei, Domoto, Nanae, Fujibayashi, Sho, Hamidani, Hamid, Hayashi, Kota, Shibata, Masaru, Tanaka, Masaomi, Wanajo, Shinya
Format:	Artikel
Sprache:	eng
Online-Zugang:	Volltext
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