The statistics of BAT-to-XRT flux ratio in GRB: Evidence for a characteristic value and its implications
Demosthenes Kazanas, Judith L. Racusin, Joseph Sultana, and Apostolos, Mastichiadis

TL;DR
This paper analyzes the ratio of prompt to afterglow fluxes in GRBs, finding a characteristic value near the proton-to-electron mass ratio, supporting a specific dissipation model.
Contribution
It provides the first statistical analysis of the BAT-to-XRT flux ratio in GRBs, revealing a log-normal distribution with a peak near the proton-to-electron mass ratio, supporting a particular dissipation model.
Findings
The flux ratio distribution peaks near 2000, close to m_p/m_e.
The distribution spans about 5 decades, indicating wide variability.
The characteristic ratio supports models involving proton-electron energy conversion.
Abstract
We present the statistics of the ratio, , between the prompt and afterglow "plateau" fluxes of GRB. This we define as the ratio between the mean prompt energy flux in {\em Swift} BAT and the {\em Swift} XRT one, immediately following the steep transition between these two states and the beginning of the afterglow stage referred to as the "plateau". Like the distribution of many other GRB observables, the histogram of ~ is log-normal with maximum at a value , FWHM of about 2 decades and with the entire distribution spanning about 5 decades in the value of . We note that the peak of the distribution is close to the proton-to-electron mass ratio , as proposed to be the case in an earlier publication, on the basis of a specific model of the GRB dissipation process. It therefore appears that, in…
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