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Prompt TeV Emission from Cosmic Rays Accelerated by Gamma Ray Bursts Interacting with Surrounding Stellar Wind

Repositori DSpace/Manakin

dc.contributor.author	Razzaque, Soebur
dc.contributor.author	Mena Requejo, Olga
dc.contributor.author	Dermer, Charles D.
dc.date.accessioned	2014-09-11T08:31:36Z
dc.date.available	2014-09-11T08:31:36Z
dc.date.issued	2009
dc.identifier.citation	Razzaque, Soebur Mena Requejo, Olga Dermer, Charles D. 2009 Prompt TeV Emission from Cosmic Rays Accelerated by Gamma Ray Bursts Interacting with Surrounding Stellar Wind Astrophysical Journal Letters 691 1 L37 L40
dc.identifier.uri	http://hdl.handle.net/10550/37735
dc.description.abstract	Protons accelerated in the internal shocks of a long-duration gamma-ray burst (GRB) can escape the fireball as cosmic rays by converting to neutrons. Hadronic interactions of these neutrons inside a stellar wind bubble created by the progenitor star will produce TeV gamma-rays via neutral meson decay and synchrotron radiation by charged pion-decay electrons in the wind magnetic field. Such gamma-rays should be observable from nearby GRBs by currently running and upcoming ground-based detectors.
dc.language.iso	eng
dc.relation.ispartof	Astrophysical Journal Letters, 2009, vol. 691, num. 1, p. L37-L40
dc.subject	Astrofísica
dc.title	Prompt TeV Emission from Cosmic Rays Accelerated by Gamma Ray Bursts Interacting with Surrounding Stellar Wind
dc.type	journal article	es_ES
dc.date.updated	2014-09-11T08:31:36Z
dc.identifier.doi	10.1088/0004-637X/691/1/L37
dc.identifier.idgrec	097548
dc.rights.accessRights	open access	es_ES