Testing the Invariance of Cooling Rate in Gamma-Ray Burst Pulses
arXiv:astro-ph/9711101 · doi:10.1063/1.55392
Abstract
Recent studies have found that the spectral evolution of pulses within gamma-ray bursts (GRBs) is consistent with simple radiative cooling. Perhaps more interesting was a report that some bursts may have a single cooling rate for the multiple pulses that occur within it. We determine the probability that the observed "cooling rate invariance" is purely coincidental by sampling values from the observed distribution of cooling rates. We find a 0.1-26% probability that we would randomly observe a similar degree of invariance based on a variety of pulse selection methods and pulse comparison statistics. This probability is sufficiently high to warrant skepticism of any intrinsic invariance in the cooling rate.
4 pages, 1 figure, to appear in Proceedings of the Fourth Huntsville Symposium on Gamma-Ray Bursts
Cited by in corpus (5)
- On the Hardness-Intensity Correlation in Gamma-Ray Burst Pulses
- On the Variety of the Spectral and Temporal Behaviors of Long Gamma-Ray Burst Pulses
- On the Time Evolution of Gamma-Ray Burst Pulses: A Self-Consistent Description
- Spectral Hardness Decay with Respect to Fluence in BATSE Gamma-Ray Bursts
- On the Shape of Pulse Spectra in Gamma-Ray Bursts