A broad survey of spectro-temporal properties from FRB 20121102A
Mohammed A. Chamma (1), Fereshteh Rajabi (1, 2), Aishwarya Kumar, (1), Martin Houde (1) ((1) Department of Physics, Astronomy, The, University of Western Ontario, (2) Perimeter Institute for Theoretical, Physics)

TL;DR
This study analyzes 167 bursts from FRB 20121102A across 1-7.5 GHz, confirming consistent spectro-temporal relationships and supporting the relativistic dynamical model, with implications for understanding FRB emission mechanisms.
Contribution
It provides a comprehensive survey of spectro-temporal properties of FRB 20121102A bursts, confirming key relationships and introducing a new measurement tool, Frbgui.
Findings
Inverse relation between sub-burst slope and duration.
Quadratic relationship of drift rate with frequency.
Duration decreases with increasing frequency.
Abstract
We survey the spectro-temporal properties of fast radio bursts from FRB 20121102A observed by earlier studies across a wide range of frequencies. We investigate 167 bursts from FRB 20121102A spanning frequencies 1--7.5GHz, durations of less than 1 ms to approximately 10 ms, with low and high energies, and with different wait-times. We find from this sample of bursts a strong agreement with the inverse relationship between sub-burst slope and duration and with other predictions made by the triggered relativistic dynamical model (TRDM). Earlier results found agreement with those predictions across three different repeating FRB sources. For this sample of bursts, we find that the sub-burst slope as well as the 'sad trombone' drift rate are consistent with being in a quadratic relationship with frequency and that both these quantities are inversely proportional to the duration. We also find…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Gamma-ray bursts and supernovae · Geophysics and Gravity Measurements
