NS to KNBH - Revision history

Emma Platts at 09:54, 17 October 2018

2018-10-17T09:54:10Z

← Older revision		Revision as of 05:54, 17 October 2018
Line 14:		Line 14:
	\|THzCounterpart = --		\|THzCounterpart = --
	\|OIRCounterpart = --		\|OIRCounterpart = --
	\|XrayCounterpart = Possible		\|XrayCounterpart = Possible afterglow
	\|GammarayCounterpart = Possible		\|GammarayCounterpart = Possible GRB
	\|GWCounterpart = Yes		\|GWCounterpart = Yes
	\|NeutrinoCounterpart = --		\|NeutrinoCounterpart = --

Emma Platts at 09:52, 17 October 2018

2018-10-17T09:52:51Z

← Older revision		Revision as of 05:52, 17 October 2018
Line 14:		Line 14:
	\|THzCounterpart = --		\|THzCounterpart = --
	\|OIRCounterpart = --		\|OIRCounterpart = --
	\|XrayCounterpart = --		\|XrayCounterpart = Possible
	\|GammarayCounterpart = --		\|GammarayCounterpart = Possible
	\|GWCounterpart = Yes		\|GWCounterpart = Yes
	\|NeutrinoCounterpart = --		\|NeutrinoCounterpart = --

Emma Platts at 09:48, 17 October 2018

2018-10-17T09:48:29Z

← Older revision		Revision as of 05:48, 17 October 2018
Line 18:		Line 18:
	\|GWCounterpart = Yes		\|GWCounterpart = Yes
	\|NeutrinoCounterpart = --		\|NeutrinoCounterpart = --
	\|References = http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1307.1409, http://adsabs.harvard.edu/~~cgi-bin~~/~~bib_query?arXiv:1603~~.~~05509~~, http://adsabs.harvard.edu/~~abs~~/~~2014ApJ~~.~~..780L..21Z~~		\|References = http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1307.1409, http://adsabs.harvard.edu/abs/2014ApJ...780L..21Z, http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1603.05509
	\|Comments = Possible X-ray afterglow and a short/long GRB created in NS birth prior to the FRB.		\|Comments = Possible X-ray afterglow and a short/long GRB created in NS birth prior to the FRB.
	}}		}}

Emma Platts at 09:47, 17 October 2018

2018-10-17T09:47:55Z

← Older revision		Revision as of 05:47, 17 October 2018
Line 18:		Line 18:
	\|GWCounterpart = Yes		\|GWCounterpart = Yes
	\|NeutrinoCounterpart = --		\|NeutrinoCounterpart = --
	\|References = http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1307.1409, http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1603.05509		\|References = http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1307.1409, http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1603.05509, http://adsabs.harvard.edu/abs/2014ApJ...780L..21Z
	\|Comments = Possible X-ray afterglow and a short/long GRB created in NS birth prior to the FRB.		\|Comments = Possible X-ray afterglow and a short/long GRB created in NS birth prior to the FRB.
	}}		}}

Jake Gordin: /* Observational Constraints */

2018-10-11T11:26:39Z

Observational Constraints

← Older revision		Revision as of 07:26, 11 October 2018
Line 27:		Line 27:

	== Observational Constraints ==		== Observational Constraints ==

			--

Jake Gordin at 09:44, 11 October 2018

2018-10-11T09:44:16Z

← Older revision		Revision as of 05:44, 11 October 2018
Line 18:		Line 18:
	\|GWCounterpart = Yes		\|GWCounterpart = Yes
	\|NeutrinoCounterpart = --		\|NeutrinoCounterpart = --
	\|References = ~~https~~://~~arxiv~~.~~org~~/~~abs~~/1307.1409~~.pdf~~, ~~https~~://~~arxiv~~.~~org~~/~~abs~~/1603.05509		\|References = http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1307.1409, http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1603.05509
	\|Comments = Possible X-ray afterglow and a short/long GRB created in NS birth prior to the FRB.		\|Comments = Possible X-ray afterglow and a short/long GRB created in NS birth prior to the FRB.
	}}		}}

Emma Platts at 19:07, 26 September 2018

2018-09-26T19:07:00Z

← Older revision		Revision as of 15:07, 26 September 2018
Line 18:		Line 18:
	\|GWCounterpart = Yes		\|GWCounterpart = Yes
	\|NeutrinoCounterpart = --		\|NeutrinoCounterpart = --
	\|References = https://arxiv.org/~~pdf~~/1307.1409.pdf,		\|References = https://arxiv.org/abs/1307.1409.pdf, https://arxiv.org/abs/1603.05509
	\|Comments = Possible X-ray afterglow and a short/long GRB created in NS birth prior to the FRB.		\|Comments = Possible X-ray afterglow and a short/long GRB created in NS birth prior to the FRB.
	}}		}}

Emma Platts at 19:03, 26 September 2018

2018-09-26T19:03:35Z

← Older revision		Revision as of 15:03, 26 September 2018
Line 19:		Line 19:
	\|NeutrinoCounterpart = --		\|NeutrinoCounterpart = --
	\|References = https://arxiv.org/pdf/1307.1409.pdf,		\|References = https://arxiv.org/pdf/1307.1409.pdf,
	\|Comments = ~~If NS collapses into KNBH shortly after its birth, an~~ X-ray afterglow and short/long GRB ~~may be observable~~ prior to the FRB.		\|Comments = Possible X-ray afterglow and a short/long GRB created in NS birth prior to the FRB.
	}}		}}

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

2018-09-26T19:01:33Z

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

New page

{{FRBTableTemplate
|Category = Collapse
|Progenitor = NS to KNBH
|Type = Single
|EnergyMechanism = Mag. reconnection
|EmissionMechanism = Curv.
|LFRadioCounterpart = Yes
|HFRadioCounterpart = --
|MicrowaveCounterpart = --
|THzCounterpart = --
|OIRCounterpart = --
|XrayCounterpart = --
|GammarayCounterpart = --
|GWCounterpart = Yes
|NeutrinoCounterpart = --
|References = https://arxiv.org/pdf/1307.1409.pdf,
|Comments = If NS collapses into KNBH shortly after its birth, an X-ray afterglow and short/long GRB may be observable prior to the FRB.
}}

== Model Description ==

Upon the collapse of a supramassive NS into a NKBH, an event horizon will likely form before most of the mass and radiation can escape. By the no-hair theorem, magnetic fields are forbidden from piercing the event horizon, and so the magnetosphere will be left behind. Alternatively, if a NS collapses into a metastable KNBH, its electric discharge can cause the magnetosphere to be shed. Violent magnetic reconnection outside the horizon would then induce a strong magnetic shock wave that moves through the remaining plasma at the speed of light, resulting in a single FRB.

== Observational Constraints ==