On the Theory of Ring Afterglows

Synchrotron and inverse Compton emission successfully explain the observed spectra of gamma-ray burst (GRB) afterglows. It is thought that most GRBs are products of extremely relativistic outflows and the afterglow marks the interaction of that ejecta with the surrounding matter. A faster decay of a...

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Main Authors: Marcus DuPont, Andrew MacFadyen, Re’em Sari
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/acffbc
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author Marcus DuPont
Andrew MacFadyen
Re’em Sari
author_facet Marcus DuPont
Andrew MacFadyen
Re’em Sari
author_sort Marcus DuPont
collection DOAJ
description Synchrotron and inverse Compton emission successfully explain the observed spectra of gamma-ray burst (GRB) afterglows. It is thought that most GRBs are products of extremely relativistic outflows and the afterglow marks the interaction of that ejecta with the surrounding matter. A faster decay of afterglow light curves at late times is indicative of nonspherical geometries, and is usually interpreted as evidence for jet geometry. Recent numerical simulations have shown that ring-like geometries are also permissible for relativistic outflows. We therefore extend the standard theory of afterglow evolution to ring geometries. An analytic prescription for the light curves and spectra produced by relativistic toroidal blast waves is presented. We compare these to their spherical and jet-like counterparts, and show that ring afterglows decay faster than spherical outflows but not as fast as jets.
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spelling doaj.art-ef7c57191baa440d929cdafb67b27d752023-10-25T08:21:53ZengIOP PublishingThe Astrophysical Journal1538-43572023-01-0195712910.3847/1538-4357/acffbcOn the Theory of Ring AfterglowsMarcus DuPont0https://orcid.org/0000-0003-3356-880XAndrew MacFadyen1https://orcid.org/0000-0002-0106-9013Re’em Sari2https://orcid.org/0000-0002-1084-3656Center for Cosmology and Particle Physics, New York University , New York, NY 10003, USACenter for Cosmology and Particle Physics, New York University , New York, NY 10003, USARacah Institute, Hebrew University of Jerusalem , Jerusalem, 91904, IsraelSynchrotron and inverse Compton emission successfully explain the observed spectra of gamma-ray burst (GRB) afterglows. It is thought that most GRBs are products of extremely relativistic outflows and the afterglow marks the interaction of that ejecta with the surrounding matter. A faster decay of afterglow light curves at late times is indicative of nonspherical geometries, and is usually interpreted as evidence for jet geometry. Recent numerical simulations have shown that ring-like geometries are also permissible for relativistic outflows. We therefore extend the standard theory of afterglow evolution to ring geometries. An analytic prescription for the light curves and spectra produced by relativistic toroidal blast waves is presented. We compare these to their spherical and jet-like counterparts, and show that ring afterglows decay faster than spherical outflows but not as fast as jets.https://doi.org/10.3847/1538-4357/acffbcGamma-ray burstsLight curvesRelativistic fluid dynamics
spellingShingle Marcus DuPont
Andrew MacFadyen
Re’em Sari
On the Theory of Ring Afterglows
The Astrophysical Journal
Gamma-ray bursts
Light curves
Relativistic fluid dynamics
title On the Theory of Ring Afterglows
title_full On the Theory of Ring Afterglows
title_fullStr On the Theory of Ring Afterglows
title_full_unstemmed On the Theory of Ring Afterglows
title_short On the Theory of Ring Afterglows
title_sort on the theory of ring afterglows
topic Gamma-ray bursts
Light curves
Relativistic fluid dynamics
url https://doi.org/10.3847/1538-4357/acffbc
work_keys_str_mv AT marcusdupont onthetheoryofringafterglows
AT andrewmacfadyen onthetheoryofringafterglows
AT reemsari onthetheoryofringafterglows