Signatures of relativistic jets in the prompt and afterglow emission of gamma-ray bursts

Comparolo, Matteo (2026) Signatures of relativistic jets in the prompt and afterglow emission of gamma-ray bursts. [Laurea magistrale], Università di Bologna, Corso di Studio in Astrophysics and cosmology [LM-DM270], Documento ad accesso riservato.
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Abstract

This thesis investigates whether early-time X-ray emission in gamma-ray bursts can be explained within a geometrical framework governed by relativistic jet structure, without invoking prolonged central-engine activity. A forward-modelling and fitting pipeline is developed to test directly against the data two physically motivated components: prompt high-latitude emission (HLE) and synchrotron forward-shock (FS) afterglow emission. To the best of our knowledge, this is the first implementation of this combined framework for direct fits to plateau GRBs, and the first systematic data-driven test of an HLE interpretation for the X-ray extended emission of short GRBs. The framework is applied to two problems: X-ray plateaus in long GRBs and extended emission in short GRBs. For plateau GRBs, a unified structured-jet interpretation is tested, in which the X-ray plateau is attributed to structured-jet HLE and the contemporaneous optical emission to a structured FS component. Modelling of GRB 061121 and GRB 100814A shows that structured-jet HLE can reproduce the X-ray steep-decay/plateau/post-plateau evolution and broadly match the observed photon-index trends. However, these solutions underpredict the optical flux, whereas FS solutions fitted to the optical data overproduce the X-ray emission around plateau onset. The minimal structured-jet HLE+FS framework therefore does not provide a self-consistent unified description of these events. For short GRBs with extended emission, a top-hat HLE model is adopted. In four standard cases, it reproduces the main XRT light-curve morphology and is often consistent with the observed spectral evolution and with independent extrapolations to the BAT band. Two more complex bursts, GRB 080503 and GRB 211227A, instead favour a second prompt-like episode. Overall, extended emission in short GRBs emerges as a promising testbed for curvature-tail models, while plateaus in long GRBs require a more flexible multi-component picture.

Abstract
Tipologia del documento
Tesi di laurea (Laurea magistrale)
Autore della tesi
Comparolo, Matteo
Relatore della tesi
Correlatore della tesi
Scuola
Corso di studio
Ordinamento Cds
DM270
Parole chiave
gamma-ray bursts relativistic jets high-latitude emission forward shock X-ray plateaus extended emission structured jets afterglow modelling
Data di discussione della Tesi
27 Marzo 2026
URI

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