English

Scale-invariance in soft gamma repeaters

High Energy Astrophysical Phenomena 2017-05-10 v2

Abstract

The statistical properties of the soft gamma repeater SGR J1550--5418 are investigated carefully. We find that the cumulative distributions of fluence, peak flux and duration can be well fitted by a bent power law, while the cumulative distribution of waiting time follows a simple power law. In particular, the probability density functions of fluctuations of fluence, peak flux, and duration have a sharp peak and fat tails, which can be well fitted by a qq-Gaussian function. The qq values keep approximately steady for different scale intervals, indicating a scale-invariant structure of soft gamma repeaters. Those results support that the origin of soft gamma repeaters is crustquakes of neutron stars with extremely strong magnetic fields.

Keywords

Cite

@article{arxiv.1702.05842,
  title  = {Scale-invariance in soft gamma repeaters},
  author = {Zhe Chang and Hai-Nan Lin and Yu Sang and Ping Wang},
  journal= {arXiv preprint arXiv:1702.05842},
  year   = {2017}
}

Comments

7 pages, 5 figures, 2 tables

R2 v1 2026-06-22T18:22:36.623Z