Source-agnostic gravitational-wave detection with recurrent autoencoders
Abstract
We present an application of anomaly detection techniques based on deep recurrent autoencoders (AEs) to the problem of detecting gravitational wave (GW) signals in laser interferometers. Trained on noise data, this class of algorithms could detect signals using an unsupervised strategy, i.e. without targeting a specific kind of source. We develop a custom architecture to analyze the data from two interferometers. We compare the obtained performance to that obtained with other AE architectures and with a convolutional classifier. The unsupervised nature of the proposed strategy comes with a cost in terms of accuracy, when compared to more traditional supervised techniques. On the other hand, there is a qualitative gain in generalizing the experimental sensitivity beyond the ensemble of pre-computed signal templates. The recurrent AE outperforms other AEs based on different architectures. The class of recurrent AEs presented in this paper could complement the search strategy employed for GW detection and extend the discovery reach of the ongoing detection campaigns.
Additional Information
© 2022 The Author(s). Published by IOP Publishing Ltd. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 license. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. Received 13 August 2021; Accepted 9 February 2022; Published 4 April 2022. We are grateful to the insight and expertise of Rana Adhikari, Hang Yu, and Erik Katsavounidis from the LIGO collaboration and Elena Cuoco from the VIRGO collaboration, who guided us on a field of research which is not our own. Part of this work was conducted at 'iBanks', the AI GPU cluster at Caltech. We acknowledge NVIDIA, SuperMicro and the Kavli Foundation for their support of 'iBanks'. This work was carried on as part of the 2020 CERN OpenLab Summer Student program, which was carried on in remote mode due to the COVID pandemic. M P is supported by the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program (Grant Agreement No. 772369). E M is supported by the Institute for Research and Innovation in Software for High Energy Physics (IRIS-HEP) through a fellowship in Innovative Algorithms. This work is partially supported by the U.S. DOE, Office of Science, Office of High Energy Physics under Award Nos. DE-SC0011925, DE-SC0019227 and DE-AC02-07CH11359. Data availability statement: The data that support the findings of this study are openly available at the following URL/DOI: 10.5281/zenodo.5121514, 10.5281/zenodo.5121510, 10.5281/zenodo.5772814 and 10.5281/zenodo.5773513.Attached Files
Published - Moreno_2022_Mach._Learn.__Sci._Technol._3_025001.pdf
Submitted - 2107.12698.pdf
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Additional details
- Eprint ID
- 112532
- Resolver ID
- CaltechAUTHORS:20211217-233151582
- NVIDIA Corporation
- SuperMicro Corporation
- Kavli Foundation
- European Research Council (ERC)
- 772369
- Institute for Research and Innovation in Software for High Energy Physics
- Department of Energy (DOE)
- DE-SC0011925
- Department of Energy (DOE)
- DE-SC0019227
- Department of Energy (DOE)
- DE-AC02-07CH11359
- Created
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2021-12-20Created from EPrint's datestamp field
- Updated
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2022-04-06Created from EPrint's last_modified field