Striped Jets in Post–Neutron Star Merger Systems
Models invoking magnetic reconnection as the particle acceleration mechanism within relativistic jets often adopt a gradual energy dissipation profile within the jet. However, such a profile has yet to be reproduced in first-principles simulations. Here we perform a suite of 3D general relativistic...
Main Authors: | Emma Kaufman, I. M. Christie, A. Lalakos, A. Tchekhovskoy, D. Giannios |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2023-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/ace894 |
Similar Items
-
Propagation of a Realistic Magnetar Jet through a Binary Neutron Star Merger Medium and Implications for Short Gamma-Ray Bursts
by: Gustavo Soares, et al.
Published: (2023-01-01) -
The Collimation of Relativistic Jets in Post–Neutron Star Binary Merger Simulations
by: Matteo Pais, et al.
Published: (2023-01-01) -
Flares, Jets, and Quasiperiodic Outbursts from Neutron Star Merger Remnants
by: Elias R. Most, et al.
Published: (2023-01-01) -
Inhomogeneous Jets from Neutron Star Mergers: One Jet to Rule Them All
by: Gavin P. Lamb, et al.
Published: (2022-11-01) -
Hours-long Near-UV/Optical Emission from Mildly Relativistic Outflows in Black Hole–Neutron Star Mergers
by: Ore Gottlieb, et al.
Published: (2023-01-01)