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A possible model of pulsar timing. Biping Gong Collaborator Yaping Li. KIAA Oct 19, 2012. quasi-periodic feature ?. Possible mechanisms. free precession. exact period. un-modeled companion. Random processes. quasi-periodic feature ? multi-planets ?.
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A possible model of pulsar timing Biping Gong Collaborator Yaping Li KIAA Oct 19, 2012
Possible mechanisms free precession exact period un-modeled companion Random processes quasi-periodic feature? multi-planets ?
Long-term orbital effects? Like the effect of free precession, it also predicts a periodic timing delay, without considering the motion of the orbital plane. geodetic precession of spin axis , BO equation
BO’s two-body equation negligible
AK’stwo-body equation(J=const) J=L+S=const (J=const ?) Just with the basic binary parameters like, orbital period, mass, and spin parameters like, spin angular momentum, we have the following results.
Companion star? Orbital period,0.20-0.34 hr Companion mass,0.16-0.68 solar mass • Are there binary pulsars with • orbital period less than 90min ? Spin angular momentum, -