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- W2158081316 abstract "Some of radiopulsars have anomalous braking index values $n = Omega ddot{Omega} / dot{Omega}^2 sim pm (10^3 div 10^4) $. It is shown that such values may be related with nondipolar magnetic field. The precession of neutron star lead to rotation (in reference frame related with neutron star) of vector of angular velocity $vec{Omega}$ along direction of neutron star magnetic dipole moment $vec{m}$ with angular velocity $vec{Omega}_{p}$. This process may cause the altering of electric current flow through inner gap and consequently the current losses with the same time scale as precession period $T_{p} = 2pi / Omega_{p}$. It occurs because of electric current in inner gaps is determined by Goldreich-Julian charge density $rho_{GJ} = -frac{vec{Omega} cdot vec{B}}{2pi c}$, which are depend on angle between direction of small scale magnetic field and angular velocity $vec{Omega}$. It is essential that pulsar tubes nearby neutron star surface are curved. In current paper it is considered the only inner gaps with steady, electron charge limited flow regime." @default.
- W2158081316 created "2016-06-24" @default.
- W2158081316 creator A5022671049 @default.
- W2158081316 creator A5051309775 @default.
- W2158081316 date "2010-09-28" @default.
- W2158081316 modified "2023-09-27" @default.
- W2158081316 title "The influence of nondipolar magnetic field and neutron star precession on braking indices of radiopulsars" @default.
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- W2158081316 doi "https://doi.org/10.1111/j.1365-2966.2010.17365.x" @default.
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