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FireballsThe sudden release of copiuos gamma-ray photons into a compact region creates an opaque photon-lepton fireball due to the prolific production of electron-positron pairs. The photons that we observe in the bursts emerge only at the end of the fireball phase after it expanded sufficiently to become optically thin or after it converted its energy to the kinetic energy of relativistic baryons which convert it, in turn, to electromagnetic pulse via the interaction with interstellar matter. It is essential, therefore, to analyze the eveolution of a fireball in order to comprehend the observed features of gamma-ray bursts. We discuss various aspects of fireball hydrodynamics and the resulting emitted spectra.
Document ID
19960010269
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Piran, Tsvi
(Hebrew Univ. Jerusalem, Israel)
Date Acquired
September 6, 2013
Publication Date
January 1, 1993
Subject Category
Space Radiation
Report/Patent Number
NASA-CR-199518
NAS 1.26:199518
Accession Number
96N17435
Funding Number(s)
CONTRACT_GRANT: NSG-1904
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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