A Toy Model for the Time-Frequency Structure of Fast Radio Bursts: Implications for the CHIME Burst Dichotomy
Brian D. Metzger, Navin Sridhar, Ben Margalit, Paz Beniamini, Lorenzo, Sironi

TL;DR
This paper presents a simple model for FRB time-frequency structure, showing how variations in a key parameter can explain observed diversity and the CHIME burst dichotomy, with implications for the external environments of different FRB types.
Contribution
It introduces a toy model linking spectral energy distribution evolution to burst diversity and the CHIME dichotomy, suggesting environmental differences influence FRB properties.
Findings
Varying the power-law index of frequency drift transforms burst durations.
The model explains the CHIME burst dichotomy through parameter variation.
External medium density profiles relate to burst duration differences.
Abstract
We introduce a toy model for the time-frequency structure of fast radio bursts (FRB), in which the observed emission is produced as a narrowly-peaked intrinsic spectral energy distribution sweeps down in frequency across the instrumental bandpass as a power-law in time. Though originally motivated by emission models which invoke a relativistic shock, the model could in principle apply to a wider range of emission scenarios. We quantify the burst's detectability using the frequency bandwidth over which most of its signal-to-noise ratio (SNR) is accumulated. We demonstrate that by varying just a single parameter of the toy model-the power-law index \beta of the frequency drift rate-one can transform a long (and hence preferentially time-resolved) burst with a narrow time-integrated spectrum into a shorter burst with a broad power-law time-integrated spectrum. We suggest that…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Seismic Waves and Analysis · earthquake and tectonic studies
