Light Curves of Swift Gamma Ray Bursts

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dc.creatorCea, Paolo
dc.date2006-06-05
dc.date2006-09-22
dc.date.accessioned2026-07-07T10:39:11Z
dc.date.available2026-07-07T10:39:11Z
dc.descriptionRecent observations from the Swift gamma-ray burst mission indicate that a fraction of gamma ray bursts are characterized by a canonical behaviour of the X-ray afterglows. We present an effective theory which allows us to account for X-ray light curves of both (short - long) gamma ray bursts and X-ray rich flashes. We propose that gamma ray bursts originate from massive magnetic powered pulsars.
dc.description21 pages, 13 figures; accepted for publication in ApJ
dc.identifierhttps://arxiv.org/abs/astro-ph/0606086
dc.identifierhttp://arxiv.org/abs/astro-ph/0606086
dc.identifierAstrophys.J.654:998-1005,2007
dc.identifierdoi:10.1086/509630
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/180940
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titleLight Curves of Swift Gamma Ray Bursts
dc.typetext

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