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


Cite item

Full Text

Open Access Open Access
Restricted Access Access granted
Restricted Access Subscription Access

Abstract

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.

About the authors

D. P. Barsukov

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

Email: tsygan@astro.ioffe.ru
Russian Federation, St. Petersburg, 194021; St. Petersburg

O. A. Goglichidze

Ioffe Physical–Technical Institute

Email: tsygan@astro.ioffe.ru
Russian Federation, St. Petersburg, 194021

A. I. Tsygan

Ioffe Physical–Technical Institute

Author for correspondence.
Email: tsygan@astro.ioffe.ru
Russian Federation, St. Petersburg, 194021

Supplementary files

Supplementary Files
Action
1. JATS XML

Copyright (c) 2016 Pleiades Publishing, Ltd.