Synchrotron Self-Absorption Process in GRBs and the Isotropic Energy - Peak Energy Fundamental Relation
M.Yu. Piotrovich, Yu.N. Gnedin, T.M. Natsvlishvili

TL;DR
This paper proposes that the observed correlation between GRB peak luminosity and energy can be explained by the synchrotron self-absorption mechanism, linking magnetic fields and relativistic effects.
Contribution
It introduces a model connecting GRB luminosity-energy correlation with synchrotron self-absorption, estimating magnetic field strengths in the central engine.
Findings
Correlation explained by SSA mechanism
Magnetic field strength estimated at ~10^{14} G
Relates Lorentz factor and redshift to emission properties
Abstract
The existence of strong correlation between the peak luminosity (and/or bolometric energetics) of Gamma Ray Bursts (GRB) is one of the most intrigue problem of GRB physics. This correlation is not yet understood. Here we demonstrate that this correlation can be explained in framework of synchrotron self-absorption (SSA) mechanism of GRB prompt emission. We estimate the magnetic field strength of the central engine at the level , where is the Lorentz factor of fireball.
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Taxonomy
TopicsGamma-ray bursts and supernovae · Astrophysics and Cosmic Phenomena · Astro and Planetary Science
