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Annihilation radiation from a hot e(+)-e(-) plasmaPair annihilation in hot e(+)-e(-) plasmas is studied. The annihilation rate, luminosity and spectrum of optically thin plasmas of temperatures above 10 to the 8th power K are calculated by means of a Monte Carlo simulation. For a given temperature, the spectrum is peaked at an energy equal to 0.511 MeV plus a positive definite quantity of order kT. In high temperature sources, such as gamma ray bursts, this blue shift can amount to a significant fraction of 0.511 MeV. The annihilation line is also temperature broadened. The width varies as T to the 1/2 power for kT much less than 0.511 MeV, and as T for kT much greater than 0.511 MeV. The widths of the 400 to 460 keV emission lines observed from several gamma ray bursts set limits on the temperatures of the pair annihilation region in burst sources. The burst emission is either nonthermal or the pair annihilation region is spatially distinct from the site of the outburst itself.
Document ID
19810016390
Acquisition Source
Legacy CDMS
Document Type
Preprint (Draft being sent to journal)
Authors
Ramaty, R.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Meszaros, P.
(Maryland Univ. College Park, United States)
Date Acquired
September 4, 2013
Publication Date
April 1, 1981
Subject Category
Plasma Physics
Report/Patent Number
NASA-TM-82124
Report Number: NASA-TM-82124
Accession Number
81N24925
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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