Published June 24, 2024 | Version v1
Journal article

Premerger detection of massive black hole binaries using deep learning

  • 1. School of Fundamental Physics and Mathematical Sciences, Hangzhou Institute for Advanced Study, University of Chinese Academy of Sciences, Hangzhou 310024, China
  • 2. School of Physical Sciences, University of Chinese Academy of Sciences, No.19A Yuquan Road, Beijing 100049, China
  • 3. CAS Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100190, China

Description

Coalescing massive black hole binaries (MBHBs) are one of primary sources for space-based gravitational wave (GW) observations. The mergers of these binaries are expected to give rise to detectable electromagnetic (EM) emissions with a narrow time window. The premerger detection of GW signals is vital for follow-up EM observations. The conventional approach for searching GW signals involves high computational costs. In this study, we present a deep learning model to search for GW signals from MBHBs. Our model is able to process 4.7 days of simulated data within 0.01 seconds and detect GW signals several hours to days before the final merger. The model provides the possibility of the coincident GW and EM detection of MBHBs.

Additional details

Identifiers

DOI
10.1103/PhysRevD.109.123031;
arXiv
arXiv:2402.16282;
Crossref Funder ID
10.13039/501100001809;

Publishing Information

Journal Title
Physical Review D
Journal Volume
109
Journal Issue
12
Journal Page Range
10 pgs.
ISSN
1089-4918

Optional Information

Copyright
© 2024 American Physical Society
Contract/Grant/Project number
12247140; 12075297; 12235019
Notes
Contact Email: ruanwenhong@ucas.ac.cn; Contact Email: guozk@itp.ac.cn; Record automatically processed
Funding organization
National Natural Science Foundation of China