Influence of Space Curvature on the Moment of Inertia of a Pulsar Magnetic Field

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We consider the influence of space curvature in the Schwarzschild metric on the contribution of the magnetic field outside the neutron star to the moment of inertia of a radio pulsar. Our consideration
is restricted only to the simplest configuration of the magnetic field, when it can be described by only one harmonic. We show that at a fixed magnetic field strength on the stellar surface the influence of space curvature reduces the contribution of the magnetic field outside the star to the departure of the inertia tensor from the spherical one several-fold.

作者简介

A. Matevosyan

Peter the Great St. Petersburg Polytechnic University, St. Petersburg, 195251 Russian

Email: bars.astro@mail.ioffe.ru
Россия, Санкт-Петербург

D. Barsukov

Ioffe Physical–Technical Institute,
Russian Academy of Sciences, St. Petersburg, 194021 Russia

编辑信件的主要联系方式.
Email: bars.astro@mail.ioffe.ru
Россия, Санкт-Петербург

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