Evolution of superhigh magnetic fields of magnetars

Details Evolution of superhigh magnetic fields of magnetars Evolution of superhigh magnetic fields of magnetars

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ap%26ss.333..427g&link_type=abstract

Astrophysics and Space Science, Volume 333, Issue 2, pp.427-435

Astronomy and Astrophysics

Astrophysics

1

Magnetar, Superhigh Magnetic Fields, Electron Capture Rate

Scientific paper

In this paper, we consider the effect of Landau levels on the decay of superhigh magnetic fields of magnetars. Applying 3 P 2 anisotropic neutron superfluid theory yield a second-order differential equation for a superhigh magnetic field B and its evolutionary timescale t. The superhigh magnetic fields may evolve on timescales ˜(106-107) yrs for common magnetars. According to our model, the activity of a magnetar may originate from instability caused by the high electron Fermi energy.

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