The location of radio pulsars in the period-period derivative (P-Ṗ) plane has been a key diagnostic tool since the early days of pulsar astronomy. Of particular importance is how pulsars evolve through the P-Ṗ diagram with time. Here we show that the decay of the inclination angle (...) between the magnetic and rotation axes plays a critical role. In particular, ... strongly impacts on the braking torque, an effect that has been largely ignored in previous work. We carry out simulations that include a negative ... term, and show that it is possible to reproduce the observational P-Ṗ diagram without the need for either pulsars with long birth periods or magnetic field decay. Our best model indicates a birth rate of one radio pulsar per century and a total Galactic population of ~20 000 pulsars beaming towards Earth. [ABSTRACT FROM AUTHOR]
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