Non-Cosmological FRBs from Young Supernova Remnant Pulsars
Liam Connor, Jonathan Sievers, Ue-Li Pen

TL;DR
This paper proposes a non-cosmological model for FRBs involving young pulsars in supernova remnants, explaining high dispersion measures and polarization features, and predicts specific observational signatures.
Contribution
It introduces a novel local supernova remnant pulsar model for FRBs, contrasting with cosmological explanations, and offers testable predictions for future observations.
Findings
High DM explained by young supernova remnant environment
Large Faraday rotation measures indicate local source
Predicted polarization swings and flux distribution patterns
Abstract
We propose a new extragalactic but non-cosmological explanation for fast radio bursts (FRBs) based on very young pulsars in supernova remnants. Within a few hundred years of a core-collapse supernova the ejecta is confined within 1 pc, providing a high enough column density of free electrons for the observed 375-1600 pc cm of dispersion measure (DM). By extrapolating a Crab-like pulsar to its infancy in an environment like that of SN 1987A, we hypothesize such an object could emit supergiant pulses sporadically which would be bright enough to be seen at a few hundred megaparsecs. We hypothesize that such supergiant pulses would preferentially occur early in the pulsar's life when the free electron density is still high, which is why we do not see large numbers of moderate DM FRBs ( pc cm). In this scenario Faraday rotation at the source gives rotation…
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