Unification of Pulses in Long and Short Gamma-Ray Bursts: Evidence from Pulse Properties and their Correlations
Jon Hakkila, Robert D. Preece

TL;DR
This study shows that gamma-ray burst pulses, both long and short, share similar properties and correlations, suggesting a common underlying physical process responsible for all GRB pulses.
Contribution
It demonstrates that pulse properties and their correlations are consistent across long and short GRBs, proposing a unified explanation based on hard-to-soft pulse evolution.
Findings
Pulse properties correlate strongly, unaffected by redshift.
Hard-to-soft evolution explains all observed pulse characteristics.
Overlapping pulses are misclassified intensity-tracking pulses.
Abstract
We demonstrate that distinguishable gamma-ray burst pulses exhibit similar behaviors as evidenced by correlations among the observable pulse properties of duration, peak luminosity, fluence, spectral hardness, energy-dependent lag, and asymmetry. Long and Short burst pulses exhibit these behaviors, suggesting that a similar process is responsible for producing all GRB pulses. That these properties correlate in the observer's frame indicates that intrinsic correlations are strong enough to not be diluted into insignificance by the dispersion in distances and redshift. We show how all correlated pulse characteristics can be explained by hard-to-soft pulse evolution, and we demonstrate that "intensity tracking" pulses not having these properties are not single pulses; they instead appear to be composed of two or more overlapping hard-to-soft pulses. In order to better understand pulse…
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