A model for the diffuse γ-ray spectrum

Details A model for the diffuse γ-ray spectrum A model for the diffuse γ-ray spectrum

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984phla..101..305h&link_type=abstract

Physics Letters A, Volume 101, Issue 5-6, p. 305-307.

Physics

1

Scientific paper

A model is proposed to describe the observed shelf in the cosmic diffuse radiation spectrum just above 1 MeV. This model is based on induced positronium annihilation, which at incident photon energy 2mc2 gives rise to enhancement of the radiative field. It is proposed that this amplification may occur in double radio sources or other accreting objects. Recent observation of γ-ray line emission from the double radio source SS 433 at 1.2 and 1.5 MeV is in good agreement with the proposed model.

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