Superconducting Cosmic Strings: Difference between revisions
Jump to navigation
Jump to search
Emma Platts (talk | contribs) No edit summary |
Emma Platts (talk | contribs) No edit summary |
||
| 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 10:04, 2 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 | **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