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A possible model of pulsar timing
Biping Gong Collaborator Yaping Li KIAA Oct 19, 2012
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quasi-periodic feature?
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Possible mechanisms free precession exact period un-modeled companion
Random processes quasi-periodic feature? multi-planets ?
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Long-term orbital effects?
geodetic precession of spin axis , BO equation Like the effect of free precession, it also predicts a periodic timing delay, without considering the motion of the orbital plane.
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BO’s two-body equation
negligible
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AK’s two-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.
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PSR B
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PSR B
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PSR B
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PSR B
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PSR J
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Companion star? Are there binary pulsars with
Spin angular momentum, Orbital period, hr Companion mass, solar mass Are there binary pulsars with orbital period less than 90min ?
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4U 1626-67 an evidence of such a scenario?
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Thanks!
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