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Observability of gravitational waves excited by binary stars orbiting around a supermassive black hole by space-based gravitational wave observatory

Crossref DOI link: https://doi.org/10.1140/epjc/s10052-026-15455-z

Published Online: 2026-03-12

Update policy: https://doi.org/10.1007/springer_crossmark_policy

Authors

Meng, Kun https://orcid.org/0000-0003-4415-4127
Zhang, Hongsheng https://orcid.org/0000-0003-0309-2097
Fan, Xi-Long https://orcid.org/0000-0002-8174-0128
Yuan, Yong https://orcid.org/0009-0002-9540-9230
Du, Fei https://orcid.org/0009-0000-5117-4594
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Text and Data Mining valid from 2026-03-12

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Article History

Received: 16 September 2025

Accepted: 16 February 2026

First Online: 12 March 2026

Copyright Information

Copyright Statement: 2026 The Author(s)

Copyright Holder: The Author(s)

Copyright Year: 2026