Magnetized Outflows from Short-lived Neutron Star Merger Remnants Can Produce a Blue Kilonova

Magnetized Outflows from Short-lived Neutron Star Merger Remnants Can Produce a Blue Kilonova

We present a 3D general-relativistic magnetohydrodynamic simulation of a short-lived neutron star remnant formed in the aftermath of a binary neutron star merger. The simulation uses an M1 neutrino transport scheme to track neutrino–matter interactions and is well suited to studying the resulting nu...

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Bibliographic Details
Main Authors: Sanjana Curtis, Pablo Bosch, Philipp Mösta, David Radice, Sebastiano Bernuzzi, Albino Perego, Roland Haas, Erik Schnetter
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal Letters
Subjects:
Transient sources
Compact objects
Neutron stars
Online Access:https://doi.org/10.3847/2041-8213/ad0fe1

Internet

https://doi.org/10.3847/2041-8213/ad0fe1

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