Open AccessPrecursors and e ± pair loading from erupting fireballs
Author(s) -
RamirezRuiz Enrico,
MacFadyen Andrew I.,
Lazzati Davide
Publication year - 2002
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1046/j.1365-8711.2002.05176.x
Subject(s) - physics , astrophysics , lorentz factor , radiative transfer , shock wave , thermal , gamma ray burst , radius , jet (fluid) , collimated light , blast wave , astronomy , lorentz transformation , mechanics , optics , classical mechanics , laser , computer science , computer security , meteorology
Recent observations suggest that long‐duration γ ‐ray bursts and their afterglows are produced by highly relativistic jets emitted in core‐collapse explosions. As the jet makes its way out of the stellar mantle, a bow shock runs ahead and a strong thermal precursor is produced as the shock breaks out. Such erupting fireballs produce a very bright γ ‐ray precursor as they interact with the thermal break‐out emission. The prompt γ ‐ray emission propagates ahead of the fireball before it becomes optically thin, leading to e ± pair loading and radiative acceleration of the external medium. The detection of such precursors would offer the possibility of diagnosing not only the radius of the stellar progenitor and the initial Lorentz factor of the collimated fireball, but also the density of the external environment.