NS-SN Interaction
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| Category | Progenitor | Type | Energy Mechanism | Emission Mechanism | Counterparts | References | Brief Comments | ||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| LF Radio | HF Radio | Microwave | Terahertz | Optical/IR | X-rays | Gamma-rays | Gravitational Waves | Neutrinos | |||||||
| Shock Interaction | NS-SN Interaction | Single | Mag. reconnect. | -- | Yes | -- | -- | -- | Supernova | -- | -- | -- | -- | http://adsabs.harvard.edu/abs/2009AstL...35..241E | |
Definitions: LF Radio (3 MHz to 3 GHz); HF Radio (3 GHz to 30 GHz); Microwave (30 to 300 GHz)
Model Description
A supernova explosion in a neutron star binary can lead to the shock wave interacting with the companion neutron star's magnetosphere, leading to a FRB.
Observational Constraints
A core-collapse supernova is expected to be coincident with the FRB.