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The LISA-Taiji network

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arxiv 2002.03603 v1 pith:KMSYTPMI submitted 2020-02-10 gr-qc astro-ph.IM

Wen-Hong Ruan , Chang Liu , Zong-Kuan Guo , Yue-Liang Wu , Rong-Gen Cai This is my paper · ORCID
classification gr-qcastro-ph.IM
keywords gravitational-wavelisa-taijinetworkaccuratelyaroundassumingdetectorsexpected
verification ladder T0 review T1 audit T2 compute T3 formal
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Both LISA and Taiji, planned space-based gravitational-wave detectors in orbit around the Sun, are expected to launch in 2030-2035. Assuming a one-year overlap, we explore a potential LISA-Taiji network to fast and accurately localize the gravitational-wave sources.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Gravitational waves and cosmic boundary

    gr-qc 2024-11 conditional novelty 6.0 of 10

    If the cosmos has a reflective boundary beyond redshift 15, gravitational waves from repeated black hole mergers could reveal it, with a TianQin+LISA network best at fixing the boundary's orientation.

  2. The Hubble tension: A decade review

    astro-ph.CO 2026-06 unverdicted novelty 3.0 of 10

    Pure early or late fixes to the Hubble tension are tightly constrained; remaining options are combined early-late interacting dark energy or new physics at the local-to-homogeneous transition.

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