NASA NTRS · 19820031732
Annihilation radiation from a hot e/+/-e/-/ plasma
Abstract
The radiation from electron-positron annihilations in a plasma of temperature above 10 to the 8th K is investigated as a possible source of the emission line at energies between 400 and 460 keV frequently seen in gamma-ray bursts. The annihilation rate and luminosity of an optically thin electron-positron plasma and the energy distribution of the resulting annihilation radiation are calculated by the use of a Monte Carlo technique as functions of temperature. Results indicate the annihilation spectrum to be peaked at an energy of 0.511 MeV plus a temperature-dependent blueshift, and the annihilation line to be significantly temperature-broadened. The widths of the observed burst emission lines set an upper limit of 3 x 10 to the 8th K on the temperature of any pair annihilation region in burst sources, which is considerably lower than the typical kinetic temperatures of the radiating particles. It is thus inferred that either the annihilation region is nonthermal, or spatially distinct from the burst site.
Keep this discovery
Explore connections, maps & timelines
Ramaty, R., Meszaros, P.. 1981-11-01. Annihilation radiation from a hot e/+/-e/-/ plasma. https://ntrs.nasa.gov/citations/19820031732
Cite the original work for its findings. Save a collection to share your selection of sources.