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   PR # 11048
    It has been confirmed that approximately 30 rotation-powered pulsars
    locate in the galactic globular clusters.Their progenitor is believed
    to be LMXBs. However, the number of LMXBs in the globular clusters
    are smaller than what is expected from the number of rotation-powered
    pulsars by more than an order of magnitude.  Alternatively, we
    consider that the white dwarf binary probably makes significant
    contribution to the formation of the rotation-powered pulsars because
    the white dwarf is more popular in the galaxy than the neutron star,
    We therefore propose deep surveys of the galactic globular clusters
    in order to find new white dwarf binaries.


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