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Jet–Environment Interaction after Delayed Collapse in Binary Neutron Star Mergers

We present general relativistic magnetohydrodynamic simulations of binary neutron star mergers, where the collapse of the metastable massive neutron star (MNS) remnant leads to the production of an incipient jet having terminal Lorentz factor and Poynting-flux luminosity compatible with a short gamm...

Ausführliche Beschreibung

Gespeichert in:
Hauptverfasser: Jay V. Kalinani, Riccardo Ciolfi, Manuela Campanelli, Bruno Giacomazzo, Andrea Pavan, Allen Wen, Yosef Zlochower
Format: Artigo
Sprache:Inglês
Veröffentlicht: IOP Publishing 2026-01-01
Schriftenreihe:The Astrophysical Journal Letters
Schlagworte:
Neutron stars
Black holes
Relativistic jets
Gamma-ray bursts
Magnetohydrodynamics
Gravitational wave sources
Online-Zugang:https://doi.org/10.3847/2041-8213/ae402a
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