It appears that there is a genuine shortage of radio pulsars with surface magnetic fields significantly smaller than ∼10 8 G. We propose that the pulsars with very low magnetic fields are actually strange stars locked in a state of minimum free energy and therefore at a limiting value of the magnetic field which cannot be lowered by the system spontaneously. © 2005 RAS.

Monika Sinha

Department of Physics

IIT Jodhpur

R.D.R. Mandal

M. Bagchi

S. Konar

M. Dey

J. Dey

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Monthly Notices of the Royal Astronomical Society

Strange pulsar hypothesis

Journal	Monthly Notices of the Royal Astronomical Society
ISSN	00358711