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Title: Electromagnetic Precursors to Black Hole–Neutron Star Gravitational Wave Events: Flares and Reconnection-powered Fast Radio Transients from the Late Inspiral
Abstract

The presence of magnetic fields in the late inspiral of black hole–neutron star binaries could lead to potentially detectable electromagnetic precursor transients. Using general-relativistic force-free electrodynamics simulations, we investigate premerger interactions of the common magnetosphere of black hole–neutron star systems. We demonstrate that these systems can feature copious electromagnetic flaring activity, which we find depends on the magnetic field orientation but not on black hole spin. Due to interactions with the surrounding magnetosphere, these flares could lead to fast-radio-burst-like transients and X-ray emission, withEM1041B*/1012G2ergs1as an upper bound on the luminosity, whereB*is the magnetic field strength on the surface of the neutron star.

 
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Award ID(s):
2307394 2307395
NSF-PAR ID:
10469384
Author(s) / Creator(s):
;
Publisher / Repository:
DOI PREFIX: 10.3847
Date Published:
Journal Name:
The Astrophysical Journal Letters
Volume:
956
Issue:
2
ISSN:
2041-8205
Format(s):
Medium: X Size: Article No. L33
Size(s):
["Article No. L33"]
Sponsoring Org:
National Science Foundation
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