Synchrotron Radiation as the Source of GRB Spectra, Part I: Theory
Astrophysics
2018-11-06 v1
Abstract
We investigate synchrotron emission models as the source of gamma ray burst spectra. We show that allowing for synchrotron self absorption and a ``smooth cutoff'' to the electron energy distribution produces a wide range of low energy spectral behavior. We show that there exists a correlation between the value of the peak of the spectrum, , and the low energy spectral index as determined by spectral fits over a finite bandwidth. Finally, we discuss the implications of synchrotron emission from internal shocks for GRB spectral evolution.
Cite
@article{arxiv.astro-ph/9912205,
title = {Synchrotron Radiation as the Source of GRB Spectra, Part I: Theory},
author = {Nicole M. Lloyd-Ronning and Vahe' Petrosian},
journal= {arXiv preprint arXiv:astro-ph/9912205},
year = {2018}
}
Comments
To appear in the proceedings of the 5th Huntsville Symposium on Gamma Ray Bursts