A&A 442, 579-586 (2005)
DOI: 10.1051/0004-6361:20053143
The coughing pulsar magnetosphere
I. Contopoulos200 Akti Themistokleous Str., Piraeus 18539, Greece
e-mail: icontop@academyofathens.gr
(Received 28 March 2005 / Accepted 28 June 2005 )
Abstract
Polar magnetospheric gaps consume a fraction of the electric
potential that develops
across open field lines. This effect modifies significantly
the structure of the axisymmetric pulsar magnetosphere.
We present numerical
steady-state solutions for various values of the
gap potential.
We show that a charge starved magnetosphere contains significantly
less electric current than one with freely
available electric charges.
As a result, electromagnetic neutron star braking becomes
inefficient.
We argue that the magnetosphere may spontaneously rearrange
itself to a lower energy configuration through
a dramatic release of electromagnetic field energy
and magnetic flux. Our results might be relevant
in understanding the recent December 27, 2004 burst observed in
SGR 1806-20.
Key words: magnetohydrodynamics (MHD) -- pulsars: general -- stars: magnetic fields -- gamma ray: bursts
SIMBAD Objects
© ESO 2005

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