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Strange pulsar hypothesis
R.D.R. Mandal, , M. Bagchi, S. Konar, M. Dey, J. Dey
Published in
Volume: 365
Issue: 4
Pages: 1383 - 1386
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.
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JournalMonthly Notices of the Royal Astronomical Society