Achromatic Breaks for Swift GRBs: Any Evidence?
S. Covino (INAF/OABr), D. Malesani (NBI-Dark, SISSA), G. Tagliaferri, (INAF/OABr), S.D. Vergani (DIAS, DCU), G. Chincarini (Bicocca Univ.,, INAF/OABr), D.A. Kann (TLS Tautenburg), A.Moretti (INAF/OABr), L. Stella, (INAF/OAR)

TL;DR
This paper reviews the evidence for achromatic breaks in Swift gamma-ray burst afterglows, highlighting the lack of conclusive confirmation despite high-quality multi-wavelength data.
Contribution
It provides a critical review of observed cases, questioning the universality of achromatic breaks in the standard afterglow model.
Findings
Few confirmed achromatic breaks in Swift data
Challenges to the standard afterglow model
Highlights need for further multi-wavelength observations
Abstract
The availability of multi-wavelength high-quality data of gamma-ray burst afterglows in the Swift era, contrary to the expectations, did not allow us to fully confirm yet one of the most fundamental features of the standard afterglow picture: the presence of an achromatic break in the decaying light curve. We briefly review the most interesting cases identified so far.
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Taxonomy
TopicsGamma-ray bursts and supernovae
