Superconducting Cosmic Strings - Revision history

Sulona: /* Observational Constraints */

2018-10-11T11:30:04Z

Observational Constraints

← Older revision		Revision as of 07:30, 11 October 2018
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	== Observational Constraints ==		== Observational Constraints ==

	~~To be filled in with updated draft~~		-

Sulona: /* Model Description */

2018-10-11T10:22:52Z

Model Description

← Older revision		Revision as of 06:22, 11 October 2018
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	== Model Description ==		== Model Description ==

	~~To be filled~~ in with ~~updated draft~~		A cosmic string becomes superconducting when coupled with electromagnetism; achievable through the unbroken symmetry of an extra Higgs field in the formation of the string. Various mechanisms have been considered in which superconducting cosmic strings may produce an FRB, such as: string oscillations, the collisions of string structures (cusps and kinks), and the interaction of a current-carrying loop in the magnetic field of a galaxy. In the last scenario listed, the event rate of FRBs indicates a loop size consistent with strings formed during the radiation era. The emission from superconducting cosmic strings is linearly polarized - an intrinsic signature that is independent of frequency and is not affected by polarization via the ISM. Expected counterparts are other EM counterparts - specifically, GRBs, cosmic rays, and neutrinos - and GWs.

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

	To be filled in with updated draft		To be filled in with updated draft

Jake Gordin at 10:04, 11 October 2018

2018-10-11T10:04:19Z

← Older revision		Revision as of 06:04, 11 October 2018
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	\|GWCounterpart = Yes		\|GWCounterpart = Yes
	\|NeutrinoCounterpart = Yes		\|NeutrinoCounterpart = Yes
	\|References = http://adsabs.harvard.edu/abs/2015AASP....5...43Z ~~to main paper~~, http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1807.01976, http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0802.0711		\|References = http://adsabs.harvard.edu/abs/2015AASP....5...43Z, http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1807.01976, http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0802.0711

	\|Comments = High energy cosmic rays are also expected.		\|Comments = High energy cosmic rays are also expected.

Jake Gordin at 10:03, 11 October 2018

2018-10-11T10:03:58Z

← Older revision		Revision as of 06:03, 11 October 2018
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	\|GWCounterpart = Yes		\|GWCounterpart = Yes
	\|NeutrinoCounterpart = Yes		\|NeutrinoCounterpart = Yes
	\|References = **need to add: http://adsabs.harvard.edu/abs/2015AASP....5...43Z to main paper, ~~https~~://~~arxiv~~.~~org~~/~~pdf~~/1807.01976.~~pdf~~		\|References = http://adsabs.harvard.edu/abs/2015AASP....5...43Z to main paper, http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1807.01976, http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0802.0711

	~~Vachaspati~~:~~2008su~~

	\|Comments = High energy cosmic rays are also expected.		\|Comments = High energy cosmic rays are also expected.

Emma Platts at 15:04, 2 October 2018

2018-10-02T15:04:25Z

← Older revision		Revision as of 11:04, 2 October 2018
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	\|NeutrinoCounterpart = Yes		\|NeutrinoCounterpart = Yes
	\|References = **need to add: http://adsabs.harvard.edu/abs/2015AASP....5...43Z to main paper, https://arxiv.org/pdf/1807.01976.pdf		\|References = **need to add: http://adsabs.harvard.edu/abs/2015AASP....5...43Z to main paper, https://arxiv.org/pdf/1807.01976.pdf

			Vachaspati:2008su

	\|Comments = High energy cosmic rays are also expected.		\|Comments = High energy cosmic rays are also expected.
	}}		}}

Emma Platts at 14:40, 2 October 2018

2018-10-02T14:40:52Z

← Older revision		Revision as of 10:40, 2 October 2018
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	\|OIRCounterpart = --		\|OIRCounterpart = --
	\|XrayCounterpart = --		\|XrayCounterpart = --
	\|GammarayCounterpart = GRB <\br> if jet aligned		\|GammarayCounterpart = GRB <br/> if jet aligned
	\|GWCounterpart = Yes		\|GWCounterpart = Yes
	\|NeutrinoCounterpart = Yes		\|NeutrinoCounterpart = Yes

Emma Platts at 14:40, 2 October 2018

2018-10-02T14:40:06Z

← Older revision		Revision as of 10:40, 2 October 2018
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	\|OIRCounterpart = --		\|OIRCounterpart = --
	\|XrayCounterpart = --		\|XrayCounterpart = --
	\|GammarayCounterpart = GRB <br\> if jet aligned		\|GammarayCounterpart = GRB <\br> if jet aligned
	\|GWCounterpart = Yes		\|GWCounterpart = Yes
	\|NeutrinoCounterpart = Yes		\|NeutrinoCounterpart = Yes

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

2018-10-02T14:39:49Z

Created page with "   {{FRBTableTemplate |Category = Other |Pro..."

New page

{{FRBTableTemplate
|Category = Other
|Progenitor = Superconducting Cosmic Strings
|Type = Single
|EnergyMechanism = Cusp decay
|EmissionMechanism = --
|LFRadioCounterpart = Yes
|HFRadioCounterpart = --
|MicrowaveCounterpart = --
|THzCounterpart = --
|OIRCounterpart = --
|XrayCounterpart = --
|GammarayCounterpart = GRB <br\> if jet aligned
|GWCounterpart = Yes
|NeutrinoCounterpart = Yes
|References = **need to add: http://adsabs.harvard.edu/abs/2015AASP....5...43Z to main paper, https://arxiv.org/pdf/1807.01976.pdf
|Comments = High energy cosmic rays are also expected.
}}

== Model Description ==

To be filled in with updated draft

== Observational Constraints ==

To be filled in with updated draft