e+-e- annihilation and the cosmic x-ray background

Details e+-e- annihilation and the cosmic x-ray background e+-e- annihilation and the cosmic x-ray background

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983aipc..101..343k&link_type=abstract

AIP Conference Proceedings, Volume 101, pp. 343-347 (1983).

Computer Science

Background Radiations, Radiation Mechanisms, Polarization

Scientific paper

The possibility that the processes responsible for the Cosmic x-ray Background (CXB) would also produce an e--e+ annihilation feature is examined. Under the assumption that these processes are thermal, the absence of a strong e-=e+ annihilation feature places constraints on the compactness (L/R ratio) of these sources. Observations favor sources of small compactness ratio.

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