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Abstract
Phylodynamic inference has emerged as a powerful tool for research in evolutionary biology.Coalescent-based models are widely used in phylodynamics, furnishing prior distributions for
phylogenetic trees in Bayesian models and enabling inference of the effective population size,
an abstract parameter that characterizes genetic diversity and is of fundamental importance
in evolutionary biology. The Skygrid model enables the integration of external covariates
into a coalescent-based model and provides a framework to study the relationship between
past population dynamics and potential driving factors. However, the Skygrid’s complexity
makes posterior approximation challenging, and there is a need for algorithms that can
allow it to scale efficiently to large genomic data sets. Here, we evaluate the effectiveness of
a promising Markov chain Monte Carlo method, Hamiltonian Monte Carlo, for the Skygrid
model with covariates. Through an analysis of three data sets, we show that Hamiltonian
Monte Carlo generally outperforms earlier approaches.