Difference between revisions of "Superconducting Cosmic Strings"

From FRB Theory Wiki
Jump to: navigation, search
Line 19: Line 19:
 
|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.
 
}}
 
}}

Revision as of 11:04, 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

Vachaspati:2008su

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