Is the radio emission made in the neutron star's magnetosphere or in shocks far from it?
Most likely: coherent emission within or just beyond a neutron-star magnetosphereAhead on the evidence, not yet confirmed. It needs two reviews to be accepted.
Where it stands
Three answers have been proposed. Coherent emission within or just beyond a neutron-star magnetosphere. leads, with evidence 2 for: partly supported by its tests. Two are still possible.
Answers 3
History
- Zhang puts forward: coherent emission within or just beyond a neutron-star magnetosphere.
- Zhang puts forward: synchrotron maser emission from shocks at large distances from the central engine.
- Bochenek et al.: the SGR 1935+2154 burst coincided with an X-ray burst, which STARE2 noted favours synchrotron-maser or…For: Synchrotron maser emission from shocks at large distances from the central engine.
- Nimmo et al.: fRB 20221022A has a lateral emitting region under about 3 × 10⁴ km.For: Coherent emission within or just beyond a neutron-star magnetosphere.
- Mckinven et al.: fRB 20221022A shows a 130 degree S-shaped polarisation swing fitted by the rotating vector model.For: Coherent emission within or just beyond a neutron-star magnetosphere.
- Nimmo et al.: the FRB 20221022A scintillation result is inconsistent with large-radius models.Against: Synchrotron maser emission from shocks at large distances from the central engine.
- Asked on this site