Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26a...308..507p&link_type=abstract
Astronomy and Astrophysics, v.308, p.507-510
Astronomy and Astrophysics
Astrophysics
5
Pulsars: General, Stars: Magnetic Fields
Scientific paper
We have derived an analytic equation for time evolution of inclination angle ξ between the magnetic moment and the spin axis of radio pulsars under the assumption of magnetic dipole braking model. We find that ξ is sensitive to the characteristic time t_c_ and the initial inclination angle ξ_0_ for a magnetic dipole torque. We note the maximum effect of alignment torque for pulsars born as almost orthogonal rotator. Implications of the alignment scenario are discussed.
Pandey U. S.
Prasad Shiva
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