Temporal Decomposition Studies of GRB Lightcurves
Narayana P. Bhat

TL;DR
This study introduces a statistical method to estimate the minimum variability time scale of GRB light curves, revealing differences between short and long bursts and linking spectral evolution to variability, aiding understanding of the GRB central engine.
Contribution
The paper develops a novel statistical approach to measure GRB minimum variability time scales and explores their relation to spectral evolution and central engine properties.
Findings
Short GRBs have shorter minimum variability time scales than long GRBs.
Estimated MVT aligns with the shortest pulse rise times.
Variability time scales are related to spectral evolution and Lorentz factors.
Abstract
Gamma-ray bursts (GRB) are extremely energetic events and produce highly diverse light curves. Light curves are believed to be resulting from internal shocks reflecting the activities of the GRB central engine. Hence their temporal studies can potentially lead to the understanding of the GRB central engine and its evolution. The light curve variability time scale is an interesting parameter which most models attribute to a physical origin e.g., central engine activity, clumpy circumburst medium, or relativistic turbulence. We develop a statistical method to estimate the GRB minimum variability time scale (MVT) for long and short GRBs detected by GBM. We find that the MVT of short bursts is distinctly shorter than that for long GRBs supprting the possibility of a more compact central engine of the former. We find that MVT estimated by this method is consistent with the shortest rise time…
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