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Possible discovery of threeγ-ray pulsars

✍ Scribed by Yuqian Ma; Tan Lu; K. N. Yu; C. M. Young


Publisher
Springer Netherlands
Year
1993
Tongue
English
Weight
389 KB
Volume
201
Category
Article
ISSN
0004-640X

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We consider a possible contribution of mature γ-ray pulsars to cosmic ray positrons based on the revised outer gap model, e ± pairs in the pulsars magnetosphere are produced by the cascade of e ± pairs through synchrotron radiation of the return current from the outer gap. Using a Monte Carlo method