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Automated discovery of interpretable gravitational-wave population models

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arxiv 2207.12409 v1 pith:FDRMME2X submitted 2022-07-25 astro-ph.IM astro-ph.HEcs.LGgr-qc

classification astro-ph.IMastro-ph.HEcs.LGgr-qc
keywords modelspopulationflexiblegravitational-waveinterpretableanalyticdiscoverdistribution
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We present an automatic approach to discover analytic population models for gravitational-wave (GW) events from data. As more gravitational-wave (GW) events are detected, flexible models such as Gaussian Mixture Models have become more important in fitting the distribution of GW properties due to their expressivity. However, flexible models come with many parameters that lack physical motivation, making interpreting the implication of these models challenging. In this work, we demonstrate symbolic regression can complement flexible models by distilling the posterior predictive distribution of such flexible models into interpretable analytic expressions. We recover common GW population models such as a power-law-plus-Gaussian, and find a new empirical population model which combines accuracy and simplicity. This demonstrates a strategy to automatically discover interpretable population models in the ever-growing GW catalog, which can potentially be applied to other astrophysical phenomena.

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  1. Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression

    gr-qc 2025-04 conditional novelty 4.0 of 10

    A symbolic-regression fit, k2(M, log10 Lambda), approximates neutron-star radii from gravitational-wave-only mass and tidal-deformability measurements to within a few hundred meters for the tested equations of state.

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