Influence of small-scale magnetic field on the reverse positron current in the inner gaps of radio pulsars
- 作者: Barsukov D.P.1,2, Goglichidze O.A.1, Tsygan A.I.1
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隶属关系:
- Ioffe Physical–Technical Institute
- Peter the Great St. Petersburg Polytechnic University
- 期: 卷 60, 编号 6 (2016)
- 页面: 586-597
- 栏目: Article
- URL: https://journals.rcsi.science/1063-7729/article/view/189943
- DOI: https://doi.org/10.1134/S106377291604003X
- ID: 189943
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详细
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.
作者简介
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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