NS-BH Merger: Difference between revisions
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Emma Platts (talk | contribs) No edit summary |
Jake Gordin (talk | contribs) No edit summary |
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|GWCounterpart = Yes | |GWCounterpart = Yes | ||
|NeutrinoCounterpart = -- | |NeutrinoCounterpart = -- | ||
|References = | |References = http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1511.02870 | ||
|Comments = None | |Comments = None | ||
}} | }} | ||
Latest revision as of 04:50, 11 October 2018
| 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 | |||||||
| Merger | NS-BH | Single | BH battery | -- | -- | -- | -- | -- | -- | Yes | Yes | Yes | -- | http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1511.02870 | None |
Definitions: LF Radio (3 MHz to 3 GHz); HF Radio (3 GHz to 30 GHz); Microwave (30 to 300 GHz)
Model Description
During the inspiral of a NS-BH merger, the magnetic field lines of the NS may thread around the BH event horizon in a way similar to a battery powering a circuit, and produce a single FRB.
Observational Constraints
The FRB emission would have a precursor burst and a double peak.