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Normalizing Flows for Hierarchical Bayesian Analysis: A Gravitational Wave Population Study

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arxiv 2211.09008 v3 pith:VFEOHMEJ submitted 2022-11-15 astro-ph.IM astro-ph.HEcs.LGgr-qc

Normalizing Flows for Hierarchical Bayesian Analysis: A Gravitational Wave Population Study

classification astro-ph.IM astro-ph.HEcs.LGgr-qc
keywords populationgravitationalwaveanalysisbayesiandatadistributionsflexible
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We propose parameterizing the population distribution of the gravitational wave population modeling framework (Hierarchical Bayesian Analysis) with a normalizing flow. We first demonstrate the merit of this method on illustrative experiments and then analyze four parameters of the latest LIGO/Virgo data release: primary mass, secondary mass, redshift, and effective spin. Our results show that despite the small and notoriously noisy dataset, the posterior predictive distributions (assuming a prior over the parameters of the flow) of the observed gravitational wave population recover structure that agrees with robust previous phenomenological modeling results while being less susceptible to biases introduced by less flexible models. Therefore, the method forms a promising flexible, reliable replacement for population inference distributions, even when data is highly noisy.

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Cited by 5 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Comparing astrophysical models to gravitational-wave data in the observable space

    gr-qc 2025-07 unverdicted novelty 7.0

    Demonstrates direct comparison of observable compact-binary populations from GW data to astrophysical models, with unbiased inference shown possible and applied to O3 data.

  2. Binary neutron stars in the next-generation era: Multi-messenger detection prospects and constraints on the equation of state, mass distribution, and cosmology

    astro-ph.HE 2026-07 conditional novelty 6.0

    With ET (and ET+CE), mock multi-messenger BNS catalogues yield ~40–500 EM counterparts per year and, under ideal recovery, constrain R1.4 to ~0.2 km and H0 to ~1 km s−1 Mpc−1.

  3. Normalizing flows for density estimation in multi-detector gravitational-wave searches

    astro-ph.HE 2026-04 unverdicted novelty 6.0

    Normalizing flows replace binned histograms for estimating multi-detector signal parameters in PyCBC, slashing storage by three orders of magnitude with under 0.05% sensitivity loss and up to 6.55% gains in specific cases.

  4. Model-Agnostic Population Inference for Gravitational-Wave Astronomy: From LVK to LISA

    astro-ph.IM 2026-01 conditional novelty 5.0

    A flow-guided mixture density network with Gaussian copulas recovers black-hole merger population shapes and rates from sparse, selection-biased gravitational-wave catalogs.

  5. An Implementation to Identify the Properties of Multiple Population of Gravitational Wave Sources

    gr-qc 2025-09 unverdicted novelty 4.0

    GWKokab is a new modular JAX framework that uses normalizing flow samplers for efficient inference on subpopulations of compact binary mergers.