NS-BH Merger - Revision history

Jake Gordin at 09:50, 11 October 2018

2018-10-11T09:50:59Z

← Older revision		Revision as of 05:50, 11 October 2018
Line 18:		Line 18:
	\|GWCounterpart = Yes		\|GWCounterpart = Yes
	\|NeutrinoCounterpart = --		\|NeutrinoCounterpart = --
	\|References = ~~https~~://~~arxiv~~.~~org~~/~~abs~~/1511.02870		\|References = http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1511.02870
	\|Comments = None		\|Comments = None
	}}		}}

Emma Platts at 12:08, 26 September 2018

2018-09-26T12:08:28Z

← Older revision		Revision as of 08:08, 26 September 2018
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	== Model Description ==		== Model Description ==

	~~--To be updated--~~
	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.		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 ==		== Observational Constraints ==
	The FRB emission would have a precursor burst and a double peak.		The FRB emission would have a precursor burst and a double peak.

Emma Platts: Created page with " {{FRBTableTemplate |Category = Merger |Pr..."

2018-09-26T12:05:54Z

Created page with "   {{FRBTableTemplate |Category = Merger |Pr..."

New page

{{FRBTableTemplate
|Category = Merger
|Progenitor = NS-BH
|Type = Single
|EnergyMechanism = BH battery
|EmissionMechanism = --
|LFRadioCounterpart = --
|HFRadioCounterpart = --
|MicrowaveCounterpart = --
|THzCounterpart = --
|OIRCounterpart = --
|XrayCounterpart = Yes
|GammarayCounterpart = Yes
|GWCounterpart = Yes
|NeutrinoCounterpart = --
|References = https://arxiv.org/abs/1511.02870
|Comments = None
}}

== Model Description ==

--To be updated--
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.