The $E_{\rm p}$ - $E_{\rm iso}$ relation and the internal shock model
R. Mochkovitch, L. Nava

TL;DR
This study investigates whether the observed $E_{p}$ - $E_{iso}$ correlation in gamma-ray bursts can be explained by internal shock models, using synthetic populations and comparing them with observed data to identify necessary conditions.
Contribution
The paper introduces a toy model of internal shocks limited to two-shell collisions and compares synthetic burst populations with observed correlations to test the model's validity.
Findings
Model can reproduce the correlation under specific constraints.
Agreement requires particular relations between flow dynamics and microphysics.
Synthetic and observed data comparison highlights key conditions for internal shock viability.
Abstract
The validity of the - correlation in gamma-ray bursts and the possibility of explaining the prompt emission with internal shocks are highly debated questions. We study whether the - correlation can be reproduced if internal shocks are indeed responsible for the prompt emission, or conversely, if the correlation can be used to constrain the internal shock scenario. We developed a toy model where internal shocks are limited to the collision of only two shells. Synthetic burst populations were constructed for various distributions of the model parameters, such as the injected power in the relativistic outflow, the average Lorentz factor, and its typical contrast between the shells. These parameters can be independent or linked by various relations. Synthetic - diagrams are obtained in the different cases and…
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