Influence of small-scale magnetic field on the reverse positron current in the inner gaps of radio pulsars


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The reverse positron current flowing through the inner gap of an old radio pulsar in the presence of a small-scale magnetic field is found. Computations for the case of both strong and weak screening of the longitudinal electric field by the electron–positron plasma are presented.

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D. Barsukov

Ioffe Physical–Technical Institute; Peter the Great St. Petersburg Polytechnic University

Email: tsygan@astro.ioffe.ru
俄罗斯联邦, St. Petersburg, 194021; St. Petersburg

O. Goglichidze

Ioffe Physical–Technical Institute

Email: tsygan@astro.ioffe.ru
俄罗斯联邦, St. Petersburg, 194021

A. Tsygan

Ioffe Physical–Technical Institute

编辑信件的主要联系方式.
Email: tsygan@astro.ioffe.ru
俄罗斯联邦, St. Petersburg, 194021

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