Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986cha%26a..10...88x&link_type=abstract
Chinese Astronomy and Astrophysics, Volume 10, Issue 2, p. 88-93.
Astronomy and Astrophysics
Astrophysics
Plasma, Γ Rays, Γ Ray Bursts
Scientific paper
To provide the necessary data for solving the mystery of the γ-ray burst spectrum, we solved the equation of transport of γ photons in a strongly magnetized, purely scattering plasma. We mainly discussed the effect of multiple scattering on the annihilation line photons and γ-ray continuum. In our calculations we assumed the scattering layer to be a non-degenerate plasma with a temperature between (+7)K and (+8)K, and a strong magnetic field of 4.414(+12)G. We used the precise Compton cross-section for a strong field. The effect of the strong field as shown by the results of our calculation will help to gain a deeper understanding of the γ-ray burst spectrum.
Qu Qin-Yue
Xu Yao-Ming
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