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Radio Ejection and the Orbital Period Gap in the Distribution of Wide Binary Millisecond Pulsars
AIP Conference Proceedings
When a radio pulsar brakes down due to magnetodipole emission,its gravitational mass decreases accordingly. If the pulsar is hosted in a binary system, this mass loss will increase the orbital period of the system. We show that this relativistic effect can be indeed observable if the neutron star is fast and magnetized enough and that, if observed, it will help to put tight constraints to the equation of state of ultradense matter. Moreover, in Low Mass X-ray Binaries that evolve towards shortdoi:10.1063/1.2900284 fatcat:jzcprj5xe5gr7ejwtr53fxqlnq