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Issue A&A
Volume 442, Number 2, November I 2005
Page(s) 579 - 586
Section Stellar structure and evolution
DOI http://dx.doi.org/10.1051/0004-6361:20053143



A&A 442, 579-586 (2005)
DOI: 10.1051/0004-6361:20053143

The coughing pulsar magnetosphere

I. Contopoulos

200 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

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