Interpretation of Radio Afterglows in the framework of the Standard Fireball and Energy Injection models
Delina Levine, Maria Dainotti, Nissim Fraija, Donald Warren, Poonam, Chandra, Nicole Lloyd-Ronning

TL;DR
This study compiles and analyzes radio afterglow data from 82 GRBs to test the standard fireball model using closure relations, revealing that less than half of the cases are compatible with the model, especially favoring the ISM environment.
Contribution
It provides the most comprehensive radio afterglow dataset to date and systematically tests the fireball model against multiple density profiles and energy injection scenarios.
Findings
46% of GRBs fulfill at least one closure relation
ISM environment with no energy injection is most consistent
Data largely incompatible with the standard fireball model
Abstract
Gamma-Ray Bursts (GRBs) are panchromatic, highly energetic transients whose energy emission mechanism is still debated. One of the possible explanations is the standard fireball model, which can be tested with the closure relations (CRs), or relations between the temporal and spectral indices of a GRB. To test these, we compile an extensive sample of radio afterglow light curves (LCs) that span from 1997 to 2020, the most comprehensive analysis of GRBs with radio observations to date. We fit 202 LCs from 82 distinct GRBs with a broken power law, obtaining a sample of 26 that display a clear break and a subsample of 14 GRBs that present a radio plateau. We test these samples against CRs corresponding to a constant-density interstellar medium (ISM) or a stellar wind medium in both fast- and slow-cooling regimes, as well as three additional density profiles, following $n…
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Taxonomy
TopicsElectromagnetic Compatibility and Measurements
