Popov et al. outline the most comprehensive simulations of the production of neutron stars as a function of magnetic field, so far. They include field decay, accretion, spin evolution and other effects to account for the Log N-Log S relation of pulsars as well as the Log N-Log L relation for magnetars. I look forward to see an more thorough description of their results than this conference proceeeding.
http://www.arxiv.org/abs/1009.5888 Extensive population synthesis of isolated neutron stars with field decay
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