On the evolution of high-B radio pulsars with measured braking indices

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چکیده

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Why the braking indices of young pulsars are less than 3 ?

In this letter we discuss two possible reasons which cause the observed braking indices n of young radio pulsars to be smaller than 3: (a) the evolving spin-down model of the magnetic field component B⊥ increases with time; (b) the extrinsic braking torque model in which the tidal torques exerted on the pulsar by the fallback disk, and carries away the spin angular momentum from the pulsar. Bas...

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ژورنال

عنوان ژورنال: Monthly Notices of the Royal Astronomical Society

سال: 2017

ISSN: 0035-8711,1365-2966

DOI: 10.1093/mnras/stx1735