Jake Gordin at 09:55, 11 October 2018

2018-10-11T09:55:24Z

← Older revision		Revision as of 05:55, 11 October 2018
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	\|GWCounterpart = Yes		\|GWCounterpart = Yes
	\|NeutrinoCounterpart = --		\|NeutrinoCounterpart = --
	\|References = ~~https~~://~~arxiv~~.~~org~~/~~abs~~/1711.09083		\|References = http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1711.09083
	\|Comments =		\|Comments =
	}}		}}

Emma Platts at 14:28, 26 September 2018

2018-09-26T14:28:39Z

← Older revision		Revision as of 10:28, 26 September 2018
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	\|EnergyMechanism = --		\|EnergyMechanism = --
	\|EmissionMechanism = --		\|EmissionMechanism = --
	\|LFRadioCounterpart = ?		\|LFRadioCounterpart = Yes
	\|HFRadioCounterpart = ?		\|HFRadioCounterpart = ?
	\|MicrowaveCounterpart = --		\|MicrowaveCounterpart = --

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

2018-09-26T12:27:28Z

Created page with "   {{FRBTableTemplate |Category = Interactio..."

New page

{{FRBTableTemplate
|Category = Interaction
|Progenitor = Pulsar-BH
|Type = Single
|EnergyMechanism = --
|EmissionMechanism = --
|LFRadioCounterpart = ?
|HFRadioCounterpart = ?
|MicrowaveCounterpart = --
|THzCounterpart = --
|OIRCounterpart = --
|XrayCounterpart = --
|GammarayCounterpart = --
|GWCounterpart = Yes
|NeutrinoCounterpart = --
|References = https://arxiv.org/abs/1711.09083
|Comments =
}}

== Model Description ==

An enhanced giant pulse generated by a rapidly spun-up neutron star near a spinning black hole could produce a single FRB. A gyroscope is used to model the pulsar's spin-precession, which has been shown to increase rapidly near the event horizon of a Kerr BH. Eventually the spin precession exceeds the pulsar's spin, and the latter can be neglected. As such, the pulsar magnetosphere is essentially rotating around the spin-precession axis. The rapid spin-up causes a giant pulse, whose emission is consistent with an FRB.

== Observational Constraints ==

If two or more bursts are released during the rapid spin-up, the event duration is expected to be >1 ms for an unresolved burst and a double peaked profile is expected if the burst is partially resolved.

Pulsar-BH Interaction - Revision history

Jake Gordin at 09:55, 11 October 2018

Emma Platts at 14:28, 26 September 2018

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