A lognormal gamma-ray luminosity model implies about 5,000 millisecond pulsars in globular clusters, six to seven times the 770 predicted by the fundamental-plane model.
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Gamma-ray and radio populations of millisecond pulsars in globular clusters
A lognormal gamma-ray luminosity model implies about 5,000 millisecond pulsars in globular clusters, six to seven times the 770 predicted by the fundamental-plane model.