Comparing models of the periodic variations in spin-down and beam-width for PSR B1828-11
G. Ashton, D.I. Jones, R. Prix

TL;DR
This study uses Bayesian analysis to compare two models explaining periodic variations in PSR B1828-11, finding that a precession model with flexible beam geometry better fits the data than a simple switching model.
Contribution
It introduces a Bayesian framework for model comparison of pulsar variability, evaluating phenomenological switching and precession models with improved statistical rigor.
Findings
Precession model with general beam geometry fits data well.
Simple circular beam precession model fails to describe the data.
Bayesian odds favor precession over switching model by approximately 10^2.7.
Abstract
We build a framework using tools from Bayesian data analysis to evaluate models explaining the periodic variations in spin-down and beam-width of PSR B1828-11. The available data consists of the time averaged spin-down rate, which displays a distinctive double-peaked modulation, and measurements of the beam-width. Two concepts exist in the literature that are capable of explaining these variations; we formulate predictive models from these and quantitatively compare them. The first concept is phenomenological and stipulates that the magnetosphere undergoes periodic switching between two meta-stable states as first suggested by Lyne et al. The second concept, precession, was first considered as a candidate for the modulation of B1828-11 by Stairs et al.. We quantitatively compare models built from these concepts using a Bayesian odds-ratio. Because the phenomenological switching model…
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