Statistics – Computation
Scientific paper
Jun 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986acaps...6...58x&link_type=abstract
(Acta Astrophysica Sinica, vol. 6, no. 1, 1986, p. 58-65) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 10, June 198
Statistics
Computation
Compton Effect, Cosmic Plasma, Gamma Ray Bursts, Particle Motion, Photons, Scattering Cross Sections, Computational Astrophysics, Gamma Ray Spectra, Lorentz Transformations, Magnetic Field Configurations, Plasma Temperature, Polarization Characteristics, Red Shift, Spectral Line Width, Transport Theory
Scientific paper
To provide the necessary data for solving the mystery of the gamma-ray burst spectrum, the equation of transport of gamma protons was solved in a strongly magnetized, purely scattering plasma. The effect of multiple scattering on the annihilation line photons and gamma-ray continuum was discussed. In the calculations, the scattering layer was assumed to be a nondegenerate plasma with a temperature between (+7)K and (+8)K, and a strong magnetic field of 4.414(+12)G. The precise Compton cross-section for a strong field was used. The effect of the strong field as shown by the results of the calculation will help to gain a deeper understanding of the gamma-ray burst spectrum.
Qu Qin-Yue
Xu Yan-Mei
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