Astrophysics, abstract
astro-ph/0604364

From: Andrei Gruzinov [view email]

Date: Mon, 17 Apr 2006 23:19:29 GMT (122kb)

Force-Free Electrodynamics of Pulsars

Authors: Andrei Gruzinov (CCPP, NYU)

Comments: 9 pages, 5 figures

We show that FFE (Force-Free Electrodynamics) describes pulsar magnetospheres -- even when radiation and particle wind power are comparable to the spin-down power. At the same time, we show that FFE is insufficient for calculating pulsar magnetospheres. This is because FFE admits a large family of stationary solutions with different currents flowing in the closed line region. To choose the actual solution one needs a model of current generation which goes beyond pure FFE.

We calculate several FFE magnetospheres for the aligned rotator. The Poynting power of these solutions fills the range $c^{-3}\mu ^2\Omega^4~< ~L~ <~ 0.67 c^{-3}\mu ^2\Omega^4(c/\Omega R_s)^2$, for angular velocity $\Omega$ and magnetic field which is a pure dipole $\mu$ on the surface of the star of radius $R_s$.

Anomalous braking indices of young pulsars might be explained by currents flowing in the closed-line region.

http://arxiv.org/abs/astro-ph/0604364