Neutrino rocket model to explain the origin of high-velocity pulsars - Phys.org
Li Yuan |
Technology |
Phys.Org |
08-12-2022 |
109
The spin-down rate of the observed pulsars, , vs. their spin period, P. The dots in blue, green, and red stand for normal pulsars, pulsars in binary systems, and magnetars with a magnetic field B >â
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