The magnetic field topology in the reconnecting pulsar magnetosphere

Abstract

We show that toroidal magnetic field annihilation in the equatorial current sheet of the pulsar magnetosphere is related to how fast poloidal magnetic field lines close as we move away from the light cylinder. This determines the reconnection radial electric field which directly accelerates particles in the neutral layer inside the equatorial current sheet. The efficiency of poloidal magnetic field closure near the light cylinder may be measurable through the pulsar braking index. We argue that, the lower the efficiency of pair formation, the higher the braking index. We also argue that synchrotron radiation reaction in the neutral layer does not inhibit the accelerated particles from reaching the maximum energy of about 10^16 eV available in the open pulsar magnetosphere.

Accepted for publication in Astronomy and Astrophysics

References in corpus (4)

• Relativistic MHD Winds from Rotating Neutron Stars
• Relativistic Force-Free Electrodynamic Simulations of Neutron Star Magnetospheres
• The role of reconnection in the pulsar magnetosphere
• Jets and Disk-Winds from Pulsar Magnetospheres

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