Superconducting Cosmic Strings: Difference between revisions
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|GWCounterpart = Yes | |GWCounterpart = Yes | ||
|NeutrinoCounterpart = Yes | |NeutrinoCounterpart = Yes | ||
|References = http://adsabs.harvard.edu/abs/2015AASP....5...43Z | |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. | ||
Revision as of 05:04, 11 October 2018
| 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 | 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 | 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