Group equivariant neural posterior estimation
This addresses the challenge of exploiting equivariances in scientific inverse problems, offering a domain-specific improvement for fields like astrophysics.
The paper tackled the problem of simulation-based inference by incorporating geometric equivariances into neural density estimators, resulting in state-of-the-art accuracy and a three orders of magnitude reduction in inference times for astrophysical binary black hole systems.
Simulation-based inference with conditional neural density estimators is a powerful approach to solving inverse problems in science. However, these methods typically treat the underlying forward model as a black box, with no way to exploit geometric properties such as equivariances. Equivariances are common in scientific models, however integrating them directly into expressive inference networks (such as normalizing flows) is not straightforward. We here describe an alternative method to incorporate equivariances under joint transformations of parameters and data. Our method -- called group equivariant neural posterior estimation (GNPE) -- is based on self-consistently standardizing the "pose" of the data while estimating the posterior over parameters. It is architecture-independent, and applies both to exact and approximate equivariances. As a real-world application, we use GNPE for amortized inference of astrophysical binary black hole systems from gravitational-wave observations. We show that GNPE achieves state-of-the-art accuracy while reducing inference times by three orders of magnitude.