The time ending the shallow decay of the X-ray light curves of long GRBs

We show that the mean values and distributions of the time ending the shallow decay of the light curve of the X-ray afterglow of long gamma ray bursts (GRBs), the equivalent isotropic energy in the X-ray afterglow up to that time and the equivalent isotropic GRB energy, as well as the correlations b...

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Detalles Bibliográficos
Autores principales: Dado, Shlomo, Dar, Arnon, De Rujula, A.
Lenguaje:eng
Publicado: 2007
Materias:
Astrophysics and Astronomy
Acceso en línea:http://cds.cern.ch/record/1026028
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author Dado, Shlomo
Dar, Arnon
De Rujula, A.
author_facet Dado, Shlomo
Dar, Arnon
De Rujula, A.
author_sort Dado, Shlomo
collection CERN
description We show that the mean values and distributions of the time ending the shallow decay of the light curve of the X-ray afterglow of long gamma ray bursts (GRBs), the equivalent isotropic energy in the X-ray afterglow up to that time and the equivalent isotropic GRB energy, as well as the correlations between them, are precisely those predicted by the cannonball (CB) model of GRBs. Correlations between prompt and afterglow observables are important in that they test the overall consistency of a GRB model. In the CB model, the prompt and afterglow spectra, the endtime, the complex canonical shape of the X-ray afterglows and the correlations between GRB observables are not surprises, but predictions.
id cern-1026028
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2007
record_format invenio
spelling cern-10260282023-03-14T20:06:04Zhttp://cds.cern.ch/record/1026028engDado, ShlomoDar, ArnonDe Rujula, A.The time ending the shallow decay of the X-ray light curves of long GRBsAstrophysics and AstronomyWe show that the mean values and distributions of the time ending the shallow decay of the light curve of the X-ray afterglow of long gamma ray bursts (GRBs), the equivalent isotropic energy in the X-ray afterglow up to that time and the equivalent isotropic GRB energy, as well as the correlations between them, are precisely those predicted by the cannonball (CB) model of GRBs. Correlations between prompt and afterglow observables are important in that they test the overall consistency of a GRB model. In the CB model, the prompt and afterglow spectra, the endtime, the complex canonical shape of the X-ray afterglows and the correlations between GRB observables are not surprises, but predictions.We show that the mean values and distributions of the time ending the shallow decay of the light curve of the X-ray afterglow of long gamma ray bursts (GRBs), the equivalent isotropic energy in the X-ray afterglow up to that time and the equivalent isotropic GRB energy, as well as the correlations between them, are precisely those predicted by the cannonball (CB) model of GRBs. Correlations between prompt and afterglow observables are important in that they test the overall consistency of a GRB model. In the CB model, the prompt and afterglow spectra, the endtime, the complex canonical shape of the X-ray afterglows and the correlations between GRB observables are not surprises, but predictions.astro-ph/0703700oai:cds.cern.ch:10260282007-03-27
spellingShingle Astrophysics and Astronomy
Dado, Shlomo
Dar, Arnon
De Rujula, A.
The time ending the shallow decay of the X-ray light curves of long GRBs
title The time ending the shallow decay of the X-ray light curves of long GRBs
title_full The time ending the shallow decay of the X-ray light curves of long GRBs
title_fullStr The time ending the shallow decay of the X-ray light curves of long GRBs
title_full_unstemmed The time ending the shallow decay of the X-ray light curves of long GRBs
title_short The time ending the shallow decay of the X-ray light curves of long GRBs
title_sort time ending the shallow decay of the x-ray light curves of long grbs
topic Astrophysics and Astronomy
url http://cds.cern.ch/record/1026028
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AT dararnon thetimeendingtheshallowdecayofthexraylightcurvesoflonggrbs
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AT dadoshlomo timeendingtheshallowdecayofthexraylightcurvesoflonggrbs
AT dararnon timeendingtheshallowdecayofthexraylightcurvesoflonggrbs
AT derujulaa timeendingtheshallowdecayofthexraylightcurvesoflonggrbs

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