  In this study, we model a pulsar as a general relativistic oblique rotator,
where the oblique rotator is a rotationally deformed neutron star whose
rotation and magnetic axis are inclined at an angle. The oblique rotator spins
down, losing rotational energy through the magnetic poles. The magnetic field
is assumed to be dipolar; however, the star has a non-zero azimuthal component
due to the misalignment. The magnetic field induces an electric field for a
force-free condition. The magnetic field decreases as the misalignment
increases and is minimum along the equatorial plane of the star. In contrast,
the electric field remains almost constant initially but decreases rapidly at a
high misalignment angle. The charge separation at the star surface is
qualitatively similar to that of Newtonian calculation. We find that the power
loss for a general relativistic rotator is minimum for either an aligned or an
orthogonal rotator, which contrasts with Newtonian calculation, where the power
loss increases with an increase in the misalignment angle.
