Visualizing the pulsar population using graph theory
C. R. Garc\'ia, Diego F. Torres, Alessandro Patruno

TL;DR
This paper reevaluates pulsar population visualization by applying principal components analysis and graph theory, revealing limitations of the traditional $P ext{--}\dot P$ diagram and introducing a new pulsar tree visualization tool.
Contribution
It introduces a novel analysis using PCA and graph theory to better understand pulsar similarities beyond the traditional $P ext{--}\dot P$ diagram, including a new visualization website.
Findings
$P$ and $\dot P$ are not principal components of pulsar data.
Distance measures based solely on $P$ and $\dot P$ can be misleading.
The pulsar tree reveals similarities not visible in the traditional diagram.
Abstract
The diagram is a cornerstone of pulsar research. It is used in multiple ways for classifying the population, understanding evolutionary tracks, identifying issues in our theoretical reach, and more. However, we have been looking at the same plot for more than five decades. A fresh appraisal may be healthy. Is the -diagram the most useful or complete way to visualize the pulsars we know? Here we pose a fresh look at the information we have on the pulsar population. First, we use principal components analysis over magnitudes depending on the intrinsic pulsar's timing properties (proxies to relevant physical pulsar features), to analyze whether the information contained by the pulsar's period and period derivative is enough to describe the variety of the pulsar population. Even when the variables of interest depend on and , we show that are not…
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Taxonomy
TopicsComputational Physics and Python Applications
