Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..83..117z&link_type=abstract
Astrophysics and Space Science, vol. 83, no. 1-2, Apr. 1982, p. 117-125.
Astronomy and Astrophysics
Astrophysics
12
Gamma Ray Bursts, Neutron Stars, Positron Annihilation, Stellar Magnetic Fields, Stellar Spectra, Bremsstrahlung, Electron-Positron Pairs, Gamma Ray Spectra, Line Spectra, Pair Production, Stellar Radiation
Scientific paper
The formation mechanism of an annihilation line 0.5 MeV in gamma-ray bursts due to electron-positron pair production in strong magnetic fields of neutron stars is discussed. Positron production due to isotope decay and due to nu-meson production is considered. It is shown that a large part of radiation with the energy E greater than 2mc-squared per quantum is consumed by pair production and does not escape from the gamma bursts, which indicates a possible strong gap in continuum radiation at energies higher than 1 MeV. The expected annihilation line intensity in gamma-ray burst spectra is estimated, and agrees with observational data.
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