volume 13, issue S337, P100-103 2017
DOI: 10.1017/s1743921317010328
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Aris Karastergiou, Simon Johnston

Abstract: AbstractOver the last decade or so, it has become clear that pulsars exhibit sudden and significant changes in their spin properties. At the same time, a better understanding of the geometry of young and older pulsars, is providing clues about the long-term evolution of the magnetic inclination angle. In this talk, we present a simple simulation of the pulsar population that takes into account current observational facts. We show how, with very few assumptions, the observed P-Ṗ diagram can be reproduced for a …

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