Difference between revisions of "Superconducting Cosmic Strings"

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Line 15: Line 15:
 
|OIRCounterpart        = --
 
|OIRCounterpart        = --
 
|XrayCounterpart        = --
 
|XrayCounterpart        = --
|GammarayCounterpart    = GRB <\br> if jet aligned
+
|GammarayCounterpart    = GRB <br/> if jet aligned
 
|GWCounterpart          = Yes
 
|GWCounterpart          = Yes
 
|NeutrinoCounterpart    = Yes
 
|NeutrinoCounterpart    = Yes

Revision as of 10:40, 2 October 2018





Summary Table
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
Other Superconducting Cosmic Strings Single Cusp decay -- Yes -- -- -- -- -- GRB
if jet aligned
Yes Yes **need to add: http://adsabs.harvard.edu/abs/2015AASP....5...43Z to main paper, https://arxiv.org/pdf/1807.01976.pdf High energy cosmic rays are also expected.

Definitions: LF Radio (3 MHz to 3 GHz); HF Radio (3 GHz to 30 GHz); Microwave (30 to 300 GHz)


Model Description

To be filled in with updated draft

Observational Constraints

To be filled in with updated draft