A fast deep-learning approach to probing primordial black hole populations in gravitational wave events

Fuente: arXiv
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Auteurs principaux: Jiang, Jun-Qian, Huang, Hai-Long, He, Jibin, Wang, Yu-Tong, Piao, Yun-Song
Format: Preprint
Publié: 2025
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author Jiang, Jun-Qian
Huang, Hai-Long
He, Jibin
Wang, Yu-Tong
Piao, Yun-Song
author_facet Jiang, Jun-Qian
Huang, Hai-Long
He, Jibin
Wang, Yu-Tong
Piao, Yun-Song
contents Primordial black holes (PBHs), envisioned as a compelling dark matter candidate and a window onto early-Universe physics, may contribute to the part of the gravitational-wave (GW) signals detected by the LIGO-Virgo-KAGRA network. Traditional hierarchical Bayesian analysis, which relies on precise GW-event posterior estimates, for extracting the information of potential PBH population from GW events become computationally prohibitive for catalogs of hundreds of events. Here, we present a fast deep-learning framework, leveraging Transformer and normalizing flows, that maps GW-event posterior samples to joint posterior distributions over the hyperparameters of the PBH population. Our approach yields accurate credible intervals while reducing end-to-end inference time to $\mathcal{O}(1)$ s on a single GPU. These results underscore the potential of deep learning for fast, high-accurately PBH population studies in the era of next-generation GW detectors.
format Preprint
id arxiv_https___arxiv_org_abs_2505_15530
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle A fast deep-learning approach to probing primordial black hole populations in gravitational wave events
Jiang, Jun-Qian
Huang, Hai-Long
He, Jibin
Wang, Yu-Tong
Piao, Yun-Song
General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
Instrumentation and Methods for Astrophysics
High Energy Physics - Theory
Primordial black holes (PBHs), envisioned as a compelling dark matter candidate and a window onto early-Universe physics, may contribute to the part of the gravitational-wave (GW) signals detected by the LIGO-Virgo-KAGRA network. Traditional hierarchical Bayesian analysis, which relies on precise GW-event posterior estimates, for extracting the information of potential PBH population from GW events become computationally prohibitive for catalogs of hundreds of events. Here, we present a fast deep-learning framework, leveraging Transformer and normalizing flows, that maps GW-event posterior samples to joint posterior distributions over the hyperparameters of the PBH population. Our approach yields accurate credible intervals while reducing end-to-end inference time to $\mathcal{O}(1)$ s on a single GPU. These results underscore the potential of deep learning for fast, high-accurately PBH population studies in the era of next-generation GW detectors.
title A fast deep-learning approach to probing primordial black hole populations in gravitational wave events
topic General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
Instrumentation and Methods for Astrophysics
High Energy Physics - Theory
url https://arxiv.org/abs/2505.15530